Powered by Deep Web Technologies
Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


1

Des Moines Area Community College | .EDUconnections  

NLE Websites -- All DOE Office Websites (Extended Search)

Ames Laboratory Ames Laboratory is one of DOE's 10 Office of Science world-class research laboratories, located on the Iowa State University campus just 35 miles from the Des Moines Area Community College. Ames Lab is operated by Iowa State University. Ames Laboratory Ames Laboratory is one of DOE's 10 Office of Science world-class research laboratories, located on the Iowa State University campus just 35 miles from the Des Moines Area Community College. Ames Lab is operated by Iowa State University. Scientific Programs Science Undergraduate Laboratory Internships at Ames Lab Pre-Service Teacher Program DOE Ames Lab Faculty and Student Program (FaST) DOE Ames Lab Community College Institute Program Des Moines Area Community College Des Moines Area Community College Des Moines, Iowa DOE Applauds DMACC's Science and Technical Programs Agri/Natural Resources Biology Biomass Operations Biotechnology Environmental Science Information Technology Manufacturing Technology Microcomputers Civil Engineering Pre-Medical Telecommunications

2

Category:Des Moines, IA | Open Energy Information  

Open Energy Info (EERE)

IA IA Jump to: navigation, search Go Back to PV Economics By Location Media in category "Des Moines, IA" The following 16 files are in this category, out of 16 total. SVFullServiceRestaurant Des Moines IA MidAmerican Energy Co (Iowa).png SVFullServiceRestauran... 64 KB SVQuickServiceRestaurant Des Moines IA MidAmerican Energy Co (Iowa).png SVQuickServiceRestaura... 64 KB SVHospital Des Moines IA MidAmerican Energy Co (Iowa).png SVHospital Des Moines ... 73 KB SVLargeHotel Des Moines IA MidAmerican Energy Co (Iowa).png SVLargeHotel Des Moine... 72 KB SVLargeOffice Des Moines IA MidAmerican Energy Co (Iowa).png SVLargeOffice Des Moin... 73 KB SVMediumOffice Des Moines IA MidAmerican Energy Co (Iowa).png SVMediumOffice Des Moi... 69 KB SVMidriseApartment Des Moines IA MidAmerican Energy Co (Iowa).png

3

West Des Moines, Iowa: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Des Moines, Iowa: Energy Resources Des Moines, Iowa: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 41.5772115°, -93.711332° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.5772115,"lon":-93.711332,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

4

After 105 Years, Historic City Hall in West Des Moines, Iowa Goes Green |  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

After 105 Years, Historic City Hall in West Des Moines, Iowa Goes After 105 Years, Historic City Hall in West Des Moines, Iowa Goes Green After 105 Years, Historic City Hall in West Des Moines, Iowa Goes Green May 9, 2011 - 5:22pm Addthis The restored Historic City Hall building in West Des Moines' Valley Junction neighborhood. | Photo credit: Vicky Saylor The restored Historic City Hall building in West Des Moines' Valley Junction neighborhood. | Photo credit: Vicky Saylor April Saylor April Saylor Former Digital Outreach Strategist, Office of Public Affairs The city of West Des Moines, Iowa is using funding from the Recovery Act to renovate the Historic City Hall building located in Valley Junction, a charming neighborhood that boasts a weekly farmer's market, a block party during the summer months and unique shopping throughout the year.

5

A Touch of Green for Des Moines' Sherman Hill | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

A Touch of Green for Des Moines' Sherman Hill A Touch of Green for Des Moines' Sherman Hill A Touch of Green for Des Moines' Sherman Hill November 3, 2011 - 4:47pm Addthis This 1930s grocery store is currently under renovation by the Green & Main initiative. When complete in Spring 2012, the previously abandoned building will be LEED Platinum certified and feature a green roof and 54 original windows retrofitted to achieve high energy efficiency standards. | Photo courtesy of Green & Main. This 1930s grocery store is currently under renovation by the Green & Main initiative. When complete in Spring 2012, the previously abandoned building will be LEED Platinum certified and feature a green roof and 54 original windows retrofitted to achieve high energy efficiency standards. | Photo courtesy of Green & Main.

6

Des Moines County, Iowa: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Moines County, Iowa: Energy Resources Moines County, Iowa: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 40.9123374°, -91.1736994° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.9123374,"lon":-91.1736994,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

7

Des Moines, Washington: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Moines, Washington: Energy Resources Moines, Washington: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 47.4017661°, -122.3242902° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":47.4017661,"lon":-122.3242902,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

8

Installation-Restoration Program Records search for Des Moines Air National Guard Installation, Iowa  

SciTech Connect

Conclusions are: 1) Information obtained through interviews with 17 past and present installation personnel, installation records, shop folders, and field observations indicate that the Des Monies ANG Installation property has been used for disposal of small quantities of hazardous material in the past. 2) No evidence of environmental stress resulting from past disposal practices was observed at the Des Moines ANG installation. 3) In the priority listing of the three rated sites and their overall scores, the Facility 105 Vehicle Maintenance Fuel Tank, and the existing fire department training area, exhibit the most-significant potential (relative to the other Des Moines ANG Installation sites) for environmental concerns. 4) The old fire department training area located at Facility No. 228, is not considered to present significant concern for adverse effects on health or the environment.

1983-09-01T23:59:59.000Z

9

Health Consultation Des Moines (Ex) Ordnance Site Landfill and Lagoon Complex Prairie Trail Development Site  

E-Print Network (OSTI)

This letter has been prepared as a consultation to evaluate human health impacts that will remain in a commercial and residential area within Ankeny, Iowa known as the Prairie Trail Development Site. The Iowa Department of Public Healths priority is to ensure the Ankeny community has the best information possible to safeguard its health. That information is included in the following paragraphs. Background and Statement of Issues The Prairie Trail Development Area is located in the southern portion of Ankeny, Iowa. This development area is located in an area that was formally occupied by the Des Moines Ordnance Plant. The Des Moines Ordnance Plant was constructed for the production and testing of small arms munitions for use during World War II. The Landfill and Lagoon Complex was utilized for disposal of wastes from the ordnance plant and also from various entities that utilized the site property until 1991. The United States Environmental Protection Agency (EPA) is overseeing the cleanup of the Landfill and Lagoon Complex. A portion of the remainder of the site property had been used for burning of scrap explosives, the storage and disposal of chemicals, a disposal pond, testing of products, and various munitions manufacturing activities. The Iowa Department of Natural Resources (IDNR) is overseeing the cleanup of this remaining portion of the site property.

Terry E. Branstad; Kim Reynolds

2012-01-01T23:59:59.000Z

10

The 3rd International Conference of IIR on Magnetic Refrigeration at Room Temperature, Des Moines, Iowa, U.S.A, 11-15 May 2009  

E-Print Network (OSTI)

REFRIGERATION SYSTEMS USING DESIGN OF EXPERIMENTS J. ROUDAUT1,2,* , H. BOUCHEKARA1 , A. KEDOUS-LEBOUC1 , J of Design of Experiments (DOE) method in magnetic refrigeration (MR) understanding and optimizationThe 3rd International Conference of IIR on Magnetic Refrigeration at Room Temperature, Des Moines

Paris-Sud XI, Université de

11

V-059: MoinMoin Multiple Vulnerabilities | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

9: MoinMoin Multiple Vulnerabilities 9: MoinMoin Multiple Vulnerabilities V-059: MoinMoin Multiple Vulnerabilities January 1, 2013 - 5:57am Addthis PROBLEM: MoinMoin Multiple Vulnerabilities PLATFORM: Version(s): MoinMoin 1.x ABSTRACT: Multiple vulnerabilities have been reported in MoinMoin, which can be exploited by malicious users to conduct script insertion attacks and compromise a vulnerable system and by malicious people to manipulate certain data. REFERENCE LINKS: Secunia Advisory SA51663 CVE-2012-6080 CVE-2012-6081 CVE-2012-6082 IMPACT ASSESSMENT: High DISCUSSION: 1) Certain input when handling the AttachFile action is not properly verified before being used to write files. This can be exploited to overwrite arbitrary files via directory traversal sequences. 2) The application allows the upload of files with arbitrary extensions to

12

V-059: MoinMoin Multiple Vulnerabilities | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

9: MoinMoin Multiple Vulnerabilities 9: MoinMoin Multiple Vulnerabilities V-059: MoinMoin Multiple Vulnerabilities January 1, 2013 - 5:57am Addthis PROBLEM: MoinMoin Multiple Vulnerabilities PLATFORM: Version(s): MoinMoin 1.x ABSTRACT: Multiple vulnerabilities have been reported in MoinMoin, which can be exploited by malicious users to conduct script insertion attacks and compromise a vulnerable system and by malicious people to manipulate certain data. REFERENCE LINKS: Secunia Advisory SA51663 CVE-2012-6080 CVE-2012-6081 CVE-2012-6082 IMPACT ASSESSMENT: High DISCUSSION: 1) Certain input when handling the AttachFile action is not properly verified before being used to write files. This can be exploited to overwrite arbitrary files via directory traversal sequences. 2) The application allows the upload of files with arbitrary extensions to

13

Des Moines, Iowa: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

5448°, -93.6091064° 5448°, -93.6091064° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.6005448,"lon":-93.6091064,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

14

Magellan-Tutorial.pptx  

NLE Websites -- All DOE Office Websites (Extended Search)

Magellan Magellan A Test Bed to Explore Cloud Computing for Science Shane Canon and Lavanya Ramakrishnan Cray XE6 Training February 8, 2011 Magellan - Exploring Cloud Computing Co-located at two DOE-SC Facilities * Argonne Leadership Computing Facility (ALCF) * National Energy Research Scientific Computing Center (NERSC) * Funded by DOE under the American Recovery and Reinvestment Act (ARRA) 2 Magellan Mission * Determine the appropriate role for commercial and/or private cloud computing for DOE/SC midrange workloads * Deploy a test bed compute and data cloud to serve the needs of mid-range scientific computing. * Evaluate the effectiveness of this test bed for a wide spectrum of DOE/SC applications in comparison with other platform models. 3 Magellan Research Agenda

15

Magellan Final Report  

NLE Websites -- All DOE Office Websites (Extended Search)

Magellan Report on Magellan Report on Cloud Computing for Science U.S. Department of Energy Office of Advanced Scientific Computing Research (ASCR) December, 2011 CSO 23179 The Magellan Report on Cloud Computing for Science U.S. Department of Energy Office of Science Office of Advanced Scientific Computing Research (ASCR) December, 2011 Magellan Leads Katherine Yelick, Susan Coghlan, Brent Draney, Richard Shane Canon Magellan Staff Lavanya Ramakrishnan, Adam Scovel, Iwona Sakrejda, Anping Liu, Scott Campbell, Piotr T. Zbiegiel, Tina Declerck, Paul Rich Collaborators This research used resources of the Argonne Leadership Computing Facility at Argonne National Laboratory, which is supported by the Office of Science of the U.S. Department of Energy under contract DE-AC02¬06CH11357, funded through the American Recovery

16

Magellan Queues end November 30  

NLE Websites -- All DOE Office Websites (Extended Search)

Magellan Queues End November 30 Magellan Queues End November 30 November 15, 2011 by Francesca Verdier (0 Comments) Schedule and Status Mon, Nov 28 westmere queue drain - 08:00 - DONE remove - 10:20 - DONE serial queue add westmere nodes - 10:40 - DONE Tue, Nov 29 mag_xlmem queue drain - 08:00 - DONE remove - 09:15 - DONE reg_xlmem queue create - 14:00 - DONE enable - 17:00 Wed, Nov 30 no queue modifications Thu, Dec 1 magellan queue drain - 08:00 - DONE remove - 09:30 - DONE mag_serial queue drain - 08:00 - DONE remove - 09:30 - DONE Overview The "magellan" and "mag_serial" batch queues will be drained and disabled at 08:00, Thursday, December 1. Any jobs left in those queues will be discarded. The "mag_xlmem" queue, which provides shared access to a single node that

17

Targeted Eneregy Efficiency Expert Evaluation Report: Neal Smith Federal Building, Des Moines, IA  

SciTech Connect

This report summarizes the energy efficiency measures identified and implemented, and an analysis of the energy savings realized using low-cost/no-cost control system measures identified.

Fernandez, Nicholas; Goddard, James K.; Underhill, Ronald M.; Gowri, Krishnan

2013-03-01T23:59:59.000Z

18

Targeted Energy Efficiency Expert Evaluation Report: Neal Smith Federal Building, Des Moines, IA  

SciTech Connect

This report summarizes the energy efficiency measures identified and implemented, and an analysis of the energy savings realized using low-cost/no-cost control system measures identified.

Fernandez, Nicholas; Goddard, James K.; Underhill, Ronald M.; Gowri, Krishnan

2013-03-01T23:59:59.000Z

19

The Magellan Final Report on Cloud Computing  

E-Print Network (OSTI)

Leadership Computing Facility (ALCF) and the National EnergyLeadership Computing Facility (ALCF) and the National EnergyHPC compute cluster into the ALCF Magellan testbed, allowing

Coghlan, Susan

2013-01-01T23:59:59.000Z

20

Magellan Resources Group LLC | Open Energy Information  

Open Energy Info (EERE)

Magellan Resources Group LLC Magellan Resources Group LLC Jump to: navigation, search Name Magellan Resources Group LLC Place Chantilly, Virginia Zip 20151 Product Magellan Resources is an energy development and investment company primarily focused on alternative energy projects. Coordinates 38.883607°, -77.439755° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":38.883607,"lon":-77.439755,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


21

Magellan Tackles the Mysterious Proton Spin  

NLE Websites -- All DOE Office Websites (Extended Search)

Magellan Tackles Magellan Tackles Mysterious Proton Spin Magellan Tackles Mysterious Proton Spin July 28, 2011 | Tags: Accelerator Science, Data Transfer, ESnet, Magellan Linda Vu, lvu@lbl.gov, +1 510 495 2402 The STAR experiment's detector records the decay of subatomic smash-ups to uncover how the fundamental building blocks of the universe work. What makes a proton spin? That is one of the biggest mysteries in physics. Although researchers do not fully understand the underlying physics of this phenomenon, they do know that it contributes to the stability of the universe, magnetic interactions, and are a vital component of technologies like Magnetic Resonance Imaging (MRI) machines that are used in hospitals around the globe. To solve this mystery, researchers are smashing together polarized proton

22

Dr. Mostafa Moin, Minister of Science, Research and Technology, Islamic Republic of Iran  

E-Print Network (OSTI)

L. to. r.:Dr Henrik Foeth, Team Leader, CMS experiment; Dr Daniel Denegri, Physics Coordinator, CMS experiment; Prof. Tejinder Virdee, Deputy Spokesman, CMS experiment; Prof. Luciano Maiani, CERN Director-General (signing); Mr Jean-Marie Dufour, Head of the Legal Service, Mr Ghodratollah Habibpour Gharakol (back); Dr Abdolali Sharghi, Advisor to the Minister and Director General, Office of International Scientific Cooperation, Ministry of Science, Research and Technology; Dr Mostafa Moin, Minister of Science, Research and Technology, Islamic Republic of Iran (signing); Dr Reza Mansouri, Director, International Scientific Meetings Office, Ministry of Science, Research and Technology; H. E. Dr Ali Khorram, Extraordinary and plenipotentiary Ambassador to the United Nations in Geneva and Dr Hans F. Hoffmann, CERN Director for Technology Transfer & for Scientific Computing. _

Patrice Loez

2001-01-01T23:59:59.000Z

23

et les mtadonnes CMIP5 Sieste Globc -Marie-Pierre Moine -2 dcembre 2010  

E-Print Network (OSTI)

outils de création d'instances CIM (WP6) Questionnaire CMIP5 : collecte des métadonnées sur les modèles et simulations) Interface d'instanciation du CIM : Geonetwork Développer des services d'accès et produit ces données; les modèles utilisés pour ces simulations. CIM : « Common Information Model » Ce

24

The Chemical Enrichment History of the Magellanic Clouds Field Populations  

E-Print Network (OSTI)

We report the results of our project devoted to study the chemical enrichment history of the field population in the Magellanic Clouds using Ca II triplet spectroscopy.

R. Carrera; C. Gallart; A. Aparicio; E. Costa; E. Hardy; R. A. Mendez; N. E. D. Noel; R. Zinn

2008-09-24T23:59:59.000Z

25

The Magellan Final Report on Cloud Computing  

Science Conference Proceedings (OSTI)

The goal of Magellan, a project funded through the U.S. Department of Energy (DOE) Office of Advanced Scientific Computing Research (ASCR), was to investigate the potential role of cloud computing in addressing the computing needs for the DOE Office of Science (SC), particularly related to serving the needs of mid- range computing and future data-intensive computing workloads. A set of research questions was formed to probe various aspects of cloud computing from performance, usability, and cost. To address these questions, a distributed testbed infrastructure was deployed at the Argonne Leadership Computing Facility (ALCF) and the National Energy Research Scientific Computing Center (NERSC). The testbed was designed to be flexible and capable enough to explore a variety of computing models and hardware design points in order to understand the impact for various scientific applications. During the project, the testbed also served as a valuable resource to application scientists. Applications from a diverse set of projects such as MG-RAST (a metagenomics analysis server), the Joint Genome Institute, the STAR experiment at the Relativistic Heavy Ion Collider, and the Laser Interferometer Gravitational Wave Observatory (LIGO), were used by the Magellan project for benchmarking within the cloud, but the project teams were also able to accomplish important production science utilizing the Magellan cloud resources.

,; Coghlan, Susan; Yelick, Katherine

2011-12-21T23:59:59.000Z

26

MMTF: THE MARYLAND-MAGELLAN TUNABLE FILTER  

Science Conference Proceedings (OSTI)

This paper describes the Maryland-Magellan Tunable Filter (MMTF) on the Magellan-Baade 6.5 m telescope. MMTF is based on a 150 mm clear aperture Fabry-Perot (FP) etalon that operates in low orders and provides transmission bandpass and central wavelength adjustable from {approx}5 A to {approx}15 A and from {approx}5000 A to over {approx}9200 A, respectively. It is installed in the Inamori Magellan Areal Camera and Spectrograph and delivers an image quality of {approx}0.''5 over a field of view of 27' in diameter (monochromatic over {approx}10'). This versatile and easy-to-operate instrument has been used over the past three years for a wide variety of projects. This paper first reviews the basic principles of FP tunable filters, and then provides a detailed description of the hardware and software associated with MMTF and the techniques developed to observe with this instrument and reduce the data. The main lessons learned in the course of the commissioning and implementation of MMTF are highlighted next, before concluding with a brief outlook on the future of MMTF and of similar facilities which are soon coming on line.

Veilleux, S.; Weiner, B. J.; Rupke, D. S. N. [Department of Astronomy, University of Maryland, College Park, MD 20742 (United States)], E-mail: veilleux@astro.umd.edu, E-mail: bjw@as.arizona.edu, E-mail: drupke@ifa.hawaii.edu (and others)

2010-01-15T23:59:59.000Z

27

How Common are the Magellanic Clouds  

SciTech Connect

We introduce a probabilistic approach to the problem of counting dwarf satellites around host galaxies in databases with limited redshift information. This technique is used to investigate the occurrence of satellites with luminosities similar to the Magellanic Clouds around hosts with properties similar to the Milky Way in the object catalog of the Sloan Digital Sky Survey. Our analysis uses data from SDSS Data Release 7, selecting candidate Milky-Way-like hosts from the spectroscopic catalog and candidate analogs of the Magellanic Clouds from the photometric catalog. Our principal result is the probability for a Milky-Way-like galaxy to host N{sub sat} close satellites with luminosities similar to the Magellanic Clouds. We find that 81 percent of galaxies like the Milky Way have no such satellites within a radius of 150 kpc, 11 percent have one, and only 3.5 percent of hosts have two. The probabilities are robust to changes in host and satellite selection criteria, background-estimation technique, and survey depth. These results demonstrate that the Milky Way has significantly more satellites than a typical galaxy of its luminosity; this fact is useful for understanding the larger cosmological context of our home galaxy.

Liu, Lulu; Gerke, Brian F.; Wechsler, Risa H.; Behroozi, Peter S.; Busha, Michael T.; /KIPAC, Menlo Park /SLAC

2011-05-20T23:59:59.000Z

28

Magellan at NERSC Progress Report for June 2010  

Science Conference Proceedings (OSTI)

The Magellan Project was funded by the American Recovery and Reinvestment Act to investigate the applicability of cloud computing for the Department of Energy's Office of Science (DOE-SC). This report covers the progress for the Magellan Project at NERSC since it began in September 2009and focuses on the research aspects of the project.

Broughton, Richard Canon, Lavanya Ramakrishnan, Brent Draney, Jeff

2010-06-30T23:59:59.000Z

29

The FIRE infrared spectrometer at Magellan: construction and commissioning  

E-Print Network (OSTI)

We describe the construction and commissioning of FIRE, a new 0.8-2.5?m echelle spectrometer for the Magellan/ Baade 6.5 meter telescope. FIRE delivers continuous spectra over its full bandpass with nominal spectral ...

Simcoe, Robert A.

30

Magellan at NERSC Progress Report for June 2010  

E-Print Network (OSTI)

NERSC in partnership with ESNet was able to provisionof Magellan to JGI. Using ESnets OSCARS [6] and the Scienceare adjacent on the ESnet Bay Area MAN (Metropolitan Area

Broughton, Richard Canon, Lavanya Ramakrishnan, Brent Draney, Jeff

2011-01-01T23:59:59.000Z

31

CX-006500: Categorical Exclusion Determination | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

00: Categorical Exclusion Determination 00: Categorical Exclusion Determination CX-006500: Categorical Exclusion Determination Magellan Des Moines Biodiesel Terminal Project CX(s) Applied: B5.1 Date: 09/06/2011 Location(s): Des Moines, Iowa Office(s): Energy Efficiency and Renewable Energy, Golden Field Office The Department of Energy is proposing to provide $500,000 in State Energy Program American Recovery and Reinvestment Act (SEP ARRA) funding to Magellan Midstream Partners, LP (Magellan) to install a new B99 - 210,000 gallon (5,000 barrel) above-ground storage tank, piping, and in-line meter blending equipment to handle biodiesel at six loading positions at its bulk fuel storage terminal facility. DOCUMENT(S) AVAILABLE FOR DOWNLOAD CX-006500.pdf More Documents & Publications Year-in-Review: 2012 Energy Infrastructure Events and Expansions (July

32

Linguistique Des mots et Des hommes  

E-Print Network (OSTI)

Linguistique Des mots et Des hommes Le jour où le Léman s'est soulevé Raphaël grandeur natureTo DE CoUvErTUrE: TAGXEDo.CoM 12 ­ 29 DOSSIER LINGUISTIqUE: DES MOTS ET DES HOMMES -- A l'occasion du, présentation des enjeux de cet événement -- Considéré comme le fondateur de la linguistique moderne, Ferdinand

Loewith, Robbie

33

New lightweight DES variants  

Science Conference Proceedings (OSTI)

In this paper we propose a new block cipher, DESL (DES Lightweight), which is based on the classical DES (Data Encryption Standard) design, but unlike DES it uses a single S-box repeated eight times. On this account we adapt well-known DES S-box design ... Keywords: DES, DESL, RFID, S-box design criteria, lightweight cryptography

Gregor Leander; Christof Paar; Axel Poschmann; Kai Schramm

2007-03-01T23:59:59.000Z

34

A propos de l'usage des termes nyin et srib dans le mDo smad chos 'byung  

E-Print Network (OSTI)

l'dition mDo smad chos 'byung, Lanzhou, Kan su'u mi rigs dpe skrun khang, 1982. 2 J'en ai dj trait, pour un autre point ("A propos de notations gographiques dans l'A mdo chos 'byung", Tibet, Past and Present, Tibetan Studies I, Leiden... 63 : " sPu rang nas shar smad kyi phyogs su mi ring bar Klo bo sMan thang zer ba'i yul yod pa": "Not far in a direction down eastward from Spu-rangs is the region called Klo-bo sman-thang"), elle ne l'est pas pour une rgion moins connue ou des...

Chayet, Anne

2008-01-01T23:59:59.000Z

35

Variability-selected quasars behind the Small Magellanic Cloud  

E-Print Network (OSTI)

We present followup spectroscopic observations of quasar candidates in the Small Magellanic Cloud selected by Eyer from the OGLE database. Of twelve observed objects identified as "QSO Candidate", five are confirmed quasars, with the emission redshifts ranging from 0.28 to 2.16. Two of those quasars were also recently identified independently in the MACHO database by Geha et al. We discuss the prospects of using variability-based selection technique for quasar searches behind other dense stellar fields. An additional criterion utilizing the color-color diagram should reduce the number of stars in the candidate lists.

A. Dobrzycki; L. M. Macri; K. Z. Stanek; P. J. Groot

2002-10-28T23:59:59.000Z

36

Data reduction pipeline for the MMT Magellan Infrared Spectrograph  

E-Print Network (OSTI)

We describe principal components of the new spectroscopic data pipeline for the multi-object MMT/Magellan Infrared Spectrograph (MMIRS). The pipeline is implemented in IDL and C++. The performance of the data processing algorithms is sufficient to reduce a single dataset in 2--3 min on a modern PC workstation so that one can use the pipeline as a quick-look tool during observations. We provide an example of the spectral data processed by our pipeline and demonstrate that the sky subtraction quality gets close to the limits set by the Poisson photon statistics.

Chilingarian, Igor; Fabricant, Daniel; McLeod, Brian; Roll, John; Szentgyorgyi, Andrew

2012-01-01T23:59:59.000Z

37

YELLOW AND RED SUPERGIANTS IN THE LARGE MAGELLANIC CLOUD  

SciTech Connect

Due to their transitionary nature, yellow supergiants (YSGs) provide a critical challenge for evolutionary modeling. Previous studies within M31 and the Small Magellanic Cloud show that the Geneva evolutionary models do a poor job at predicting the lifetimes of these short-lived stars. Here, we extend this study to the Large Magellanic Cloud (LMC) while also investigating the galaxy's red supergiant (RSG) content. This task is complicated by contamination by Galactic foreground stars that color and magnitude criteria alone cannot weed out. Therefore, we use proper-motions and the LMC's large systemic radial velocity ({approx}278 km s{sup -1}) to separate out these foreground dwarfs. After observing nearly 2000 stars, we identified 317 probable YSGs, 6 possible YSGs, and 505 probable RSGs. Foreground contamination of our YSG sample was {approx}80%, while that of the RSG sample was only 3%. By placing the YSGs on the Hertzsprung-Russell diagram and comparing them against the evolutionary tracks, we find that new Geneva evolutionary models do an exemplary job at predicting both the locations and the lifetimes of these transitory objects.

Neugent, Kathryn F.; Massey, Philip; Skiff, Brian [Lowell Observatory, 1400 W Mars Hill Road, Flagstaff, AZ 86001 (United States); Meynet, Georges, E-mail: kneugent@lowell.edu, E-mail: phil.massey@lowell.edu, E-mail: bas@lowell.edu, E-mail: georges.meynet@unige.ch [Geneva Observatory, Geneva University, CH-1290 Versoix (Switzerland)

2012-04-20T23:59:59.000Z

38

A Calibrated Measurement of the Near-IR Continuum Sky Brightness Using Magellan/FIRE  

E-Print Network (OSTI)

We characterize the near-IR sky background from 308 observations with the Folded-port InfraRed Echellette (FIRE) spectrograph at Magellan. A subset of 105 observations selected to minimize lunar and thermal effects gives ...

Sullivan, Peter William

39

Velocity and density spectra of the Small Magellanic Cloud  

E-Print Network (OSTI)

This paper reports results on the statistical analysis of HI turbulence in the Small Magellanic Cloud (SMC). We use 21 cm channel maps, obtained with the Australia Telescope Compact Array and the Parkes telescope, and analyze the spectrum of observed intensity fluctuations as a function of the velocity slice thickness. We confirm predictions by Lazarian & Pogosyan (2000) on the change of the power law index and establish the spectra of 3-D density and velocity. The obtained spectral indices, -3.3 and -3.4, are slightly more shallow than the predictions for the Kolmogorov spectrum. This contrasts to the predictions for the shock-type spectra that are steeper than the Kolmogorov one. The nature of the energy injection in the SMC is unclear as no distinct energy injection scales are observed up to the entire scale of the SMC.

S. Stanimirovi?; A. Lazarian

2001-02-11T23:59:59.000Z

40

Infrared Emission from Interstellar Dust. III. The Small Magellanic Cloud  

E-Print Network (OSTI)

The infrared (IR) emission from interstellar dust in the Small Magellanic Cloud (SMC) is modelled using a mixture of amorphous silicate and carbonaceous grains, including a population of polycyclic aromatic hydrocarbon (PAH) molecules. (1) It is shown that this dust model is able to reproduce the spectral energy distribution from near-IR to far-IR for the entire SMC Bar region, provided the PAH abundance in the SMC Bar region is very low. (2) The IR spectrum of the SMCB1#1 molecular cloud can also be reproduced by our dust model provided the PAH abundance is increased relative to the overall SMC Bar. The PAHs in SMCB1#1 incorporate ~3% of the SMC C abundance, compared to environmental conditions. Other possibilities such as super-hydrogenation of PAHs and softening of the starlight spectrum are also discussed.

Aigen Li; B. T. Draine

2001-12-05T23:59:59.000Z

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


41

Variable Stars in Large Magellanic Cloud Globular Clusters III: Reticulum  

E-Print Network (OSTI)

This is the third in a series of papers studying the variable stars in old globular clusters in the Large Magellanic Cloud. The primary goal of this series is to look at how the characteristics and behavior of RR Lyrae stars in Oosterhoff-intermediate systems compare to those of their counterparts in Oosterhoff-I/II systems. In this paper we present the results of our new time-series BVI photometric study of the globular cluster Reticulum. We found a total of 32 variables stars (22 RRab, 4 RRc, and 6 RRd stars) in our field of view. We present photometric parameters and light curves for these stars. We also present physical properties, derived from Fourier analysis of light curves, for some of the RR Lyrae stars. We discuss the Oosterhoff classification of Reticulum and use our results to re-derive the distance modulus and age of the cluster.

Kuehn, Charles A; Smith, Horace A; Catelan, Mrcio; Jeon, Young-Beom; Nemec, James M; Walker, Alistair R; Kunder, Andrea; Pritzl, Barton J; De Lee, Nathan; Borissova, Jura

2013-01-01T23:59:59.000Z

42

LINGUISTIQUE Facult des arts  

E-Print Network (OSTI)

gardé les idiomes romans. C'est l'origine de la frontière linguistique. A partir du IXe siècle, des

Petriu, Emil M.

43

SPATIAL VARIATIONS OF DUST ABUNDANCES ACROSS THE LARGE MAGELLANIC CLOUD  

SciTech Connect

Using the data obtained with the Spitzer Space Telescope as part of the Surveying the Agents of a Galaxy's Evolution (SAGE) legacy survey, we have studied the variations of the dust composition and abundance across the Large Magellanic Cloud (LMC). Such variations are expected, as the explosive events which have lead to the formation of the many H I shells observed should have affected the dust properties. Using a model and comparing with a reference spectral energy distribution from our Galaxy, we deduce the relative abundance variations of small dust grains across the LMC. We examined the infrared color ratios as well as the relative abundances of very small grains (VSGs) and polycyclic aromatic hydrocarbons (PAHs) relative to the big grain abundance. Results show that each dust component could have different origins or evolution in the interstellar medium (ISM). The VSG abundance traces the star formation activity and could result from shattering of larger grains, whereas the PAH abundance increases around molecular clouds as well as in the stellar bar, where they could have been injected into the ISM during mass loss from old stars.

Paradis, Deborah; Reach, William T. [Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States); Bernard, Jean-Philippe [Universite de Toulouse, UPS, CESR, 9 av. du Colonel Roche, F-31028 Toulouse cedex 9 (France); Block, Miwa; Engelbracht, Chad W.; Gordon, Karl [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Hora, Joseph L. [Harvard-Smithsonian Center for Astrophysics, 60 Garden St., MS-65, Cambridge, MA, 02138-1516 (United States); Indebetouw, Remy [7 National Radio Astronomy Observatory and Department of Astronomy, University of Virginia, P.O. Box 3818, Charlottesville, VA 22903-0818 (United States); Kawamura, Akiko [Nagoya University, Department of Astrophysics, Chikusa-Ku, Nagoya, 464-01 (Japan); Meade, Marilyn [Department of Astronomy, University of Wisconsin, Madison, 475 N. Charter St., Madison, WI 53706 (United States); Meixner, Margaret; Sewilo, Marta [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Vijh, Uma P. [Ritter Astrophysical Research Center, University of Toledo, Toledo, OH 43606 (United States); Volk, Kevin [Gemini Observatory, Northern Operations Center, 670 N. Aohuku Place, Hilo, HI 96720 (United States)

2009-07-15T23:59:59.000Z

44

Spitzer spectroscopy of carbon stars in the Small Magellanic Cloud  

E-Print Network (OSTI)

We present Spitzer Space telescope spectroscopic observations of 14 carbon-rich AGB stars in the Small Magellanic Cloud. SiC dust is seen in most of the carbon-rich stars but it is weak compared to LMC stars. The SiC feature is strong only for stars with significant dust excess, opposite to what is observed for Galactic stars. We argue that in the SMC, SiC forms at lower temperature than graphite dust, whereas the reverse situation occurs in the Galaxy where SiC condenses at higher temperatures and forms first. Dust input into the interstellar medium by AGB stars consists mostly of carbonaceous dust, with little SiC or silicate dust. Only the two coolest stars show a 30-micron band due to MgS dust. We suggest that this is due to the fact that, in the SMC, mass-losing AGB stars generally have low circumstellar (dust) optical depth and therefore effective heating of dust by the central star does not allow temperatures below the 650 K necessary for MgS to exist as a solid. Gas phase C$_2$H$_2$ bands are stronger...

Lagadec, E; Sloan, G C; Matsuura, M; Wood, P; Harris, G J; Van Loon, J T; Blommaert, J A D L; Hony, S; Groenewegen, M A T; Feast, M W; Whitelock, P A; Menzies, J W; Cioni, M R; Waters, L B F M; Lagadec, Eric; Zijlstra, Albert A.; Matsuura, Mikako; Wood, Peter; Loon, Jacco Th. van

2006-01-01T23:59:59.000Z

45

Universit de Montral Facult des arts et des sciences  

E-Print Network (OSTI)

ATTESTATION DE COMP?TENCE LINGUISTIQUE Nom de l'étudiante 1l'étudiant : _ Date de naissance: _ Programme à l linguistique sera rédigée par la personne responsable à la Direction de l'enseignement des langues et des langue, comme un voyage d'immersion linguistique, des cours que vous avez suivis, des échanges

Parrott, Lael

46

THE 200{sup 0} LONG MAGELLANIC STREAM SYSTEM  

Science Conference Proceedings (OSTI)

We establish with certainty that the Magellanic Stream (MS) is some 40{sup 0} longer than previously known and that the entire MS and Leading Arm system is thus at least 200{sup 0} long. With the Green Bank Telescope (GBT), we conducted a {approx}200 deg{sup 2}, 21 cm survey at the tip of the MS to substantiate the continuity of the MS between the Hulsbosch and Wakker data and the MS-like emission reported by Braun and Thilker. Our survey, in combination with the Arecibo survey by Stanimirovic et al., shows that the MS gas is continuous in this region and that the MS is at least {approx}140{sup 0} long. The MS tip is composed of a multitude of forks and filaments. We identify a new filament on the eastern side of the MS that significantly deviates from the equator of the MS coordinate system for more than {approx}45{sup 0}. Additionally, we find a previously unknown velocity inflection in the MS tip near MS longitude L{sub MS} {approx}-120{sup 0} at which the velocity reaches a minimum and then starts to increase. We find that five compact high-velocity clouds cataloged by de Heij et al. as well as Wright's Cloud are plausibly associated with the MS because they match the MS in position and velocity. The mass of the newly confirmed {approx}40{sup 0} extension of the MS tip is {approx}2 x 10{sup 7} M{sub sun} (d/120 kpc){sup 2} (including Wright's Cloud increases this by {approx}50%) and increases the total mass of the MS by {approx}4%. However, projected model distances of the MS at the tip are generally quite large and, if true, indicate that the mass of the extension might be as large as {approx}10{sup 8} M{sub sun}. From our combined map of the entire MS, we find that the total column density (integrated transverse to the MS) drops markedly along the MS and follows an exponential decline with L{sub MS} of N{sub H{sub i}} = 5.9 x 10{sup 21}exp(L{sub MS}/19.{sup 0}3) cm{sup -2}. Under the assumption that the observed sinusoidal velocity pattern of the LMC filament of the MS is due to the origin of the MS from a rotating LMC, we estimate that the age of the {approx}140{sup 0} long MS is {approx}2.5 Gyr. This coincides with bursts of star formation in the Magellanic Clouds and a possible close encounter of these two galaxies with each other that could have triggered the formation of the MS. These newly observed characteristics of the MS offer additional constraints for MS simulations. In the Appendix, we describe a previously little discussed problem with a standing wave pattern in GBT H I data and detail a method for removing it.

Nidever, David L.; Majewski, Steven R. [Department of Astronomy, University of Virginia, Charlottesville, VA 22904-4325 (United States); Burton, W. Butler [Sterrewacht Leiden, P.O. Box 9513, 2300 RA Leiden (Netherlands); Nigra, Lou, E-mail: dnidever@virginia.ed, E-mail: srm4n@virginia.ed, E-mail: bburton@nrao.ed, E-mail: nigra@astro.wisc.ed [Department of Astronomy, University of Wisconsin, 475 North Charter Street, Madison, WI 53706-1582 (United States)

2010-11-10T23:59:59.000Z

47

Spitzer spectroscopy of carbon stars in the Small Magellanic Cloud  

E-Print Network (OSTI)

We present Spitzer Space telescope spectroscopic observations of 14 carbon-rich AGB stars in the Small Magellanic Cloud. SiC dust is seen in most of the carbon-rich stars but it is weak compared to LMC stars. The SiC feature is strong only for stars with significant dust excess, opposite to what is observed for Galactic stars. We argue that in the SMC, SiC forms at lower temperature than graphite dust, whereas the reverse situation occurs in the Galaxy where SiC condenses at higher temperatures and forms first. Dust input into the interstellar medium by AGB stars consists mostly of carbonaceous dust, with little SiC or silicate dust. Only the two coolest stars show a 30-micron band due to MgS dust. We suggest that this is due to the fact that, in the SMC, mass-losing AGB stars generally have low circumstellar (dust) optical depth and therefore effective heating of dust by the central star does not allow temperatures below the 650 K necessary for MgS to exist as a solid. Gas phase C$_2$H$_2$ bands are stronger in the SMC than in the LMC or Galaxy. This is attributed to an increasing C/O ratio at low metallicity. We present a colour-colour diagram based on Spitzer IRAC and MIPS colours to discriminate between O- and C-rich stars. We show that AGB stars in the SMC become carbon stars early in the thermal-pulsing AGB evolution, and remain optically visible for $\\sim 6 \\times 10^5$ yr. For the LMC, this lifetime is $\\sim 3 \\times 10^5$ yr. The superwind phase traced with Spitzer lasts for $\\sim 10^4$ yr. Spitzer spectra of a K supergiant and a compact HII region are also given.

Eric Lagadec; Albert A. Zijlstra; G. C. Sloan; Mikako Matsuura; Peter Wood; G. J. Harris; Jacco Th. van Loon; J. A. D. L. Blommaert; S. Hony; M. A. T. Groenewegen; M. W. Feast; P. A. Whitelock; J. W. Menzies; M. -R. Cioni; L. B. F. M. Waters

2006-11-02T23:59:59.000Z

48

Chemical abundances of metal-poor RR Lyrae stars in the Magellanic Clouds  

E-Print Network (OSTI)

We present for the first time a detailed spectroscopic study of chemical element abundances of metal-poor RR Lyrae stars in the Large and Small Magellanic Cloud (LMC and SMC). Using the MagE echelle spectrograph at the 6.5 ...

Haschke, Raoul

49

HORAIRE DES COURS Facult des lettres  

E-Print Network (OSTI)

, l'histoire de l'art, la linguistique ou encore l'informatique pour les sciences humaines. La Faculté humaines p. 25 Italien p. 81 Japonais p. 115 Latin p. 135 Linguistique p. 20 Littérature comparée p. 287 Département de linguistique Prendre contact par courriel : Eric.Haeberli@unige.ch #12;Début des cours

Halazonetis, Thanos

50

Linguistique, apprentissage des langues, informatique  

E-Print Network (OSTI)

Linguistique, apprentissage des langues, informatique Mention : Sciences du langage Nature de la;2 Linguistique, apprentissage des langues, informatique UFR Lettres, Langues et Sciences Humaines PR?SENTATION Objectifs Cette formation balaye un large spectre des sciences du langage dans la partie linguistique

Sart, Remi

51

Facult des arts et des sciences Dpartement de linguistique et de traduction  

E-Print Network (OSTI)

Faculté des arts et des sciences Département de linguistique et de traduction DEMANDE DE STAGE COOP

Parrott, Lael

52

VLT-FLAMES observations of young stellar clusters in the Magellanic Clouds  

E-Print Network (OSTI)

We introduce our VLT-FLAMES survey of massive stars in the Galaxy and the Magellanic Clouds, giving details of the observations in our younger fields in the LMC and SMC. In particular we highlight a new O2.5-type star discovered in N11, and Be-type stars in NGC 346 with permitted Fe II emission lines in their spectra. We give an overview of the distribution of spectral types in these fields and summarize the observed binary fraction.

C. J. Evans; D. J. Lennon; S. J. Smartt

2005-08-30T23:59:59.000Z

53

DISCOVERY OF A LARGE STELLAR PERIPHERY AROUND THE SMALL MAGELLANIC CLOUD  

Science Conference Proceedings (OSTI)

The Magellanic Clouds are a local laboratory for understanding the evolution and properties of dwarf irregular galaxies. To reveal the extended structure and interaction history of the Magellanic Clouds we have undertaken a large-scale photometric and spectroscopic study of their stellar periphery (the MAgellanic Periphery Survey, MAPS). We present first MAPS results for the Small Magellanic Cloud (SMC): Washington M, T{sub 2} + DDO51 photometry reveals metal-poor red giant branch stars in the SMC that extend to large radii ({approx}11 kpc), are distributed nearly azimuthally symmetrically (ellipticity = 0.1), and are well fitted by an exponential profile (out to R {approx} 7.{sup 0}5). An {approx}6 Gyr old, [Fe/H] {approx} -1.3 main-sequence turnoff is also evident to at least R = 7.{sup 0}3, and as far as 8.{sup 0}4 in some directions. We find evidence for a 'break' population beyond {approx}8 radial scale lengths having a very shallow radial density profile that could be either a bound stellar halo or a population of extratidal stars. The distribution of the intermediate stellar component (3{sup 0}{approx}< R {approx}< 7.{sup 0}5) contrasts with that of the inner stellar component (R {approx}< 3{sup 0}), which is both more elliptical ({epsilon} {approx} 0.3) and offset from the center of the intermediate component by 0.{sup 0}59, although both components share a similar radial exponential scale length. This offset is likely due to a perspective effect because stars on the eastern side of the SMC are closer on average than stars on the western side. This mapping of its outer stellar structures indicates that the SMC is more complex than previously thought.

Nidever, David L.; Majewski, Steven R.; Beaton, Rachael L.; Patterson, Richard J. [Department of Astronomy, University of Virginia, Charlottesville, VA 22904-4325 (United States); Munoz, Ricardo R. [Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago (Chile); Kunkel, William E., E-mail: dnidever@virginia.edu, E-mail: srm4n@virginia.edu, E-mail: rlb9n@virginia.edu, E-mail: rjp0i@virginia.edu, E-mail: rmunoz@das.uchile.cl, E-mail: kunkel@lco.cl [Las Campanas Observatory, Carnegie Institution of Washington, Casilla 601, La Serena (Chile)

2011-05-20T23:59:59.000Z

54

Choix d'investissement sous incertitude des gestionnaires des rseaux de distribution (GRD) en Europe l'horizon 2030.  

E-Print Network (OSTI)

??La distribution reste le segment du secteur de l'lectricit le moins tudi. Mais les dbats s'animent autour d'elle depuis deux ou trois ans quant aux (more)

Andaluz-Alcazar, Alvaro

2012-01-01T23:59:59.000Z

55

FACULT DES ARTS ET DES SCIENCES BUREAU DU SECRTAIRE  

E-Print Network (OSTI)

mandat au CONFAS se termine. QUORUM Le quorum est fixé à la majorité simple. LISTE DES MEMBRES Date d présenter d'une façon pratique la liste des membres ainsi que les principes de composition et le mandat des (LNG-TRA) 2013-05-31 * Philosophie Louis-André DORION 2013-05-31 Centre d'études classiques Louis

Charette, André

56

Des ressources aux traitements linguistiques : le rle dune architecture linguistique.  

E-Print Network (OSTI)

??Les systmes intgrant des traitements venant du traitement automatique des langues reposent souvent sur des lexiques et des grammaires, parfois indirectement sur des corpus. A (more)

Cailliau, Frederik

2010-01-01T23:59:59.000Z

57

Star Formation History across the Magellanic Clouds and other Local Group galaxies  

E-Print Network (OSTI)

The Ks magnitude distribution of asymptotic giant branch stars provides important constraints on the spatial variation of metallicity and mean-age of the stellar population of galaxies. Here, I present results of the investigation of these parameters across the Magellanic Clouds, M33, NGC 6822 and SagDIG and I discuss the tremendous improvement that new wide-field near-infrared instruments (i.e. VISTA) will provide on our understanding of the global intrinsic as well as dynamical history of these systems.

M. -R. L. Cioni

2006-11-13T23:59:59.000Z

58

Dense Star-forming Gas and Dust in the Magellanic Clouds  

E-Print Network (OSTI)

The early stages of star formation are closely related to the ambient conditions in the interstellar medium. Important questions such as dust abundance, size distribution, temperature distribution, fraction of molecular gas, fraction of dense gas, gas surface density and total amount of gas and dust require separation of metallicity and radiation effects. The Magellanic Clouds provide an ideal laboratory to carry out such studies. They are prominent targets for space observatories (Spitzer, Herschel), but an important role remains for large groundbased facilities, such as a 25 m class sub-millimeter telescope on Dome C.

Israel, F P

2009-01-01T23:59:59.000Z

59

Des Plaines Landfill Biomass Facility | Open Energy Information  

Open Energy Info (EERE)

Des Plaines Landfill Biomass Facility Jump to: navigation, search Name Des Plaines Landfill Biomass Facility Facility Des Plaines Landfill Sector Biomass Facility Type Landfill Gas...

60

Etude des dsintgrations charmonium des msons B dans l'exprience BaBar.  

E-Print Network (OSTI)

??Nous avons prsent dans cette habilitation diriger des recherches une tude dtaille des dsintgrations hadroniques des msons B en rsonance charmonium et kaon B?(J/?,?(2S),?c0,?c1,?c2)K(*). (more)

Grenier, P.

2006-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


61

Spectral distribution of Be/X-ray binaries in the Small Magellanic Cloud  

E-Print Network (OSTI)

The spectral distributions of Be/X-ray binaries in the Large Magellanic Cloud and Galaxy have been shown to differ significantly from the distribution of isolated Be stars in the Galaxy. Population synthesis models can explain this difference in spectral distributions through substantial angular momentum loss from the binary system. In this work we explore the spectral distribution of Be/X-ray binaries in the Small Magellanic Cloud (SMC) using high signal-to-noise spectroscopy of a sample of 37 optical counterparts to known X-ray pulsars. Our results show that the spectral distribution of Be/X-ray binaries in the SMC is consistent with that of the Galaxy, despite the lower metallicity environment of the SMC. This may indicate that, although the metallicity of the SMC is conducive to the formation of a large number of HMXBs, the spectral distribution of these systems is likely to be most strongly influenced by angular momentum losses during binary evolution, which are not particularly dependent on the local metallicity.

V. A. McBride; M. J. Coe; I. Negueruela; M. P. E. Schurch; K. E. McGowan

2008-04-30T23:59:59.000Z

62

Spitzer SAGE survey of the Large Magellanic Cloud II: Evolved Stars and Infrared Color Magnitude Diagrams  

E-Print Network (OSTI)

Color-magnitude diagrams (CMDs) are presented for the Spitzer SAGE (Surveying the Agents of a Galaxy's Evolution) survey of the Large Magellanic Cloud (LMC). IRAC and MIPS 24 um epoch one data are presented. These data represent the deepest, widest mid-infrared CMDs of their kind ever produced in the LMC. Combined with the 2MASS survey, the diagrams are used to delineate the evolved stellar populations in the Large Magellanic Cloud as well as Galactic foreground and extragalactic background populations. Some 32000 evolved stars brighter than the tip of the red giant branch are identified. Of these, approximately 17500 are classified as oxygen-rich, 7000 carbon-rich, and another 1200 as ``extreme'' asymptotic giant branch (AGB) stars. Brighter members of the latter group have been called ``obscured'' AGB stars in the literature owing to their dusty circumstellar envelopes. A large number (1200) of luminous oxygen--rich AGB stars/M supergiants are also identified. Finally, there is strong evidence from the 24 um MIPS channel that previously unexplored, lower luminosity oxygen-rich AGB stars contribute significantly to the mass loss budget of the LMC (1200 such sources are identified).

R. D. Blum; J. R. Mould; K. A. Olsen; J. A. Frogel; M. Werner; M. Meixner; F. Markwick-Kemper; R. Indebetouw; B. Whitney; M. Meade; B. Babler; E. B. Churchwell; K. Gordon; C. Engelbracht; B. -Q. For; K. Misselt; U. Vijh; C. Leitherer; K. Volk; S. Points; W. Reach; J. L. Hora; J. -P. Bernard; F. Boulanger; S. Bracker; M. Cohen; Y. Fukui; J. Gallagher; V. Gorjian; J. Harris; D. Kelly; A. Kawamura; W. B. Latter; S. Madden; A. Mizuno; N. Mizuno; A. Nota; M. S. Oey; T. Onishi; R. Paladini; N. Panagia; P. Perez-Gonzalez; H. Shibai; S. Sato; L. Smith; L. Staveley-Smith; A. G. G. M. Tielens; T. Ueta; S. Van Dyk; D. Zaritsky

2006-08-08T23:59:59.000Z

63

STAR FORMATION HISTORY IN TWO FIELDS OF THE SMALL MAGELLANIC CLOUD BAR  

SciTech Connect

The Bar is the most productive region of the Small Magellanic Cloud in terms of star formation but also the least studied one. In this paper, we investigate the star formation history of two fields located in the SW and in the NE portion of the Bar using two independent and well-tested procedures applied to the color-magnitude diagrams of their stellar populations resolved by means of deep Hubble Space Telescope photometry. We find that the Bar experienced a negligible star formation activity in the first few Gyr, followed by a dramatic enhancement from 6 to 4 Gyr ago and a nearly constant activity since then. The two examined fields differ both in the rate of star formation and in the ratio of recent over past activity, but share the very low level of initial activity and its sudden increase around 5 Gyr ago. The striking similarity between the timing of the enhancement and the timing of the major episode in the Large Magellanic Cloud is suggestive of a close encounter triggering star formation.

Cignoni, M. [Dipartimento di Astronomia, Universita degli Studi di Bologna, via Ranzani, I-40127 Bologna (Italy); Cole, A. A. [School of Mathematics and Physics, University of Tasmania, Private Bag 37, Hobart, Tasmania 7001 (Australia); Tosi, M. [Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Bologna, Via Ranzani 1, I-40127 Bologna (Italy); Gallagher, J. S. [Department of Astronomy, University of Wisconsin, 475 North Charter Street, Madison, WI 53706 (United States); Sabbi, E.; Anderson, J.; Nota, A. [STScI, Baltimore, MD 21218 (United States); Grebel, E. K., E-mail: michele.cignoni@unibo.it [Astronomisches Rechen-Institut, Zentrum fuer Astronomie der Universitaet Heidelberg, Moenchhofstr. 12-14, 69120 Heidelberg (Germany)

2012-08-01T23:59:59.000Z

64

MAGNETIC FIELD STRUCTURE OF THE LARGE MAGELLANIC CLOUD FROM FARADAY ROTATION MEASURES OF DIFFUSE POLARIZED EMISSION  

Science Conference Proceedings (OSTI)

We present a study of the magnetic field of the Large Magellanic Cloud (LMC), carried out using diffuse polarized synchrotron emission data at 1.4 GHz acquired at the Parkes Radio Telescope and the Australia Telescope Compact Array. The observed diffuse polarized emission is likely to originate above the LMC disk on the near side of the galaxy. Consistent negative rotation measures (RMs) derived from the diffuse emission indicate that the line-of-sight magnetic field in the LMC's near-side halo is directed coherently away from us. In combination with RMs of extragalactic sources that lie behind the galaxy, we show that the LMC's large-scale magnetic field is likely to be of quadrupolar geometry, consistent with the prediction of dynamo theory. On smaller scales, we identify two brightly polarized filaments southeast of the LMC, associated with neutral hydrogen arms. The filaments' magnetic field potentially aligns with the direction toward the Small Magellanic Cloud (SMC). We suggest that tidal interactions between the SMC and the LMC in the past 10{sup 9} years are likely to have shaped the magnetic field in these filaments.

Mao, S. A. [National Radio Astronomy Observatory, P.O. Box O, Socorro, NM 87801 (United States); McClure-Griffiths, N. M.; McConnell, D. [Australia Telescope National Facility, CSIRO Astronomy and Space Science, Epping, NSW 1710 (Australia); Gaensler, B. M. [Sydney Institute for Astronomy, School of Physics, University of Sydney, Sydney, NSW 2006 (Australia); Haverkorn, M. [Department of Astrophysics, Radboud University, P.O. Box 9010, 6500-GL Nijmegen (Netherlands); Beck, R. [Max-Planck-Institut fuer Radioastronomie, D-53121 Bonn (Germany); Wolleben, M. [Square Kilometre Array South Africa, The Park, Pinelands 7405 (South Africa); Stanimirovic, S. [Department of Astronomy, University of Wisconsin, Madison, WI 53706 (United States); Dickey, J. M. [Physics Department, University of Tasmania, Hobart, TAS 7001 (Australia); Staveley-Smith, L., E-mail: mao@astro.wisc.edu [International Centre for Radio Astronomy Research (ICRAR), The University of Western Australia, Crawley, WA 6009 (Australia)

2012-11-01T23:59:59.000Z

65

La perception et la production des sons relveraient de deux habilets distinctes. Ils empchent aussi l'altration  

E-Print Network (OSTI)

imbibés de concoctions douteuses. Les débuts sont diffici- les pour les ancêtres de Jean Coutu. Moins

Charette, André

66

Facult des arts et des sciences Dpartement de linguistique et de traduction  

E-Print Network (OSTI)

Faculté des arts et des sciences Département de linguistique et de traduction DEMANDE D'ADH?SION AU

Parrott, Lael

67

Facult des arts et des sciences Dpartement de linguistique et de traduction  

E-Print Network (OSTI)

Faculté des arts et des sciences Département de linguistique et de traduction GUIDE DE R?DACTION DU

Parrott, Lael

68

Facult des arts et des sciences Dpartement de linguistique et de traduction  

E-Print Network (OSTI)

Faculté des arts et des sciences Département de linguistique et de traduction Fiche d'évaluation de

Parrott, Lael

69

Facult des arts et des sciences Dpartement de linguistique et de traduction  

E-Print Network (OSTI)

Faculté des arts et des sciences Département de linguistique et de traduction BOURSES D ___________________________________________ Linguistique Traduction Code permanent __________________________________________ Adresse

Parrott, Lael

70

FACULT DES ARTS ET DES SCIENCES BUREAU DU SECRTAIRE  

E-Print Network (OSTI)

'une façon pratique la liste des membres ainsi que les principes de composition et le mandat des comités de Francis GINGRAS (adm. dél.) 2012-05-31 Littératures et langues modernes Georges L. BASTIN (LNG-TRA) 2013 bibliothéconomie et sciences de l'information 2014-05-31 BASTIN, Georges L. (LNG-TRA) 1 littératures et langues

Charette, André

71

NEW OPTICAL REDDENING MAPS OF THE LARGE AND SMALL MAGELLANIC CLOUDS  

SciTech Connect

We present new reddening maps of the Small Magellanic Cloud (SMC) and Large Magellanic Cloud (LMC) based on the data of the third phase of the Optical Gravitational Lensing Experiment (OGLE III). We have used two different methods to derive optical reddening maps. We adopt a theoretical mean unreddened color for the red clump (RC) in the SMC and LMC, respectively. We subdivide the photometric data for both Clouds into subfields and calculate the difference between the observed RC position and the theoretical value for each field, which provides us with the reddening value in (V - I). Furthermore, reddening values are obtained for 13490 LMC RR Lyrae ab and 1529 SMC RR Lyrae ab stars covering the whole OGLE III region of the Magellanic Clouds (MCs). The observed colors (V - I) of the RR Lyrae stars are compared with the color from the absolute magnitudes. The absolute magnitude of each RR Lyrae star is computed using its period and metallicity derived from Fourier decomposition of its light curve. In general, we find a low and uniform reddening distribution in both MCs. The RC method indicates a mean reddening of the LMC of E(V - I) = 0.09 {+-} 0.07 mag, while for the SMC E(V - I) = 0.04 {+-} 0.06 mag is obtained. With RR Lyrae stars a median value of E(V - I) = 0.11 {+-} 0.06 mag for the LMC and E(V - I) = 0.07 {+-} 0.06 mag for the SMC is found. The LMC shows very low reddening in the bar region, whereas the reddening in the star-forming leading edge and 30 Doradus is considerably higher. In the SMC, three pronounced regions with higher reddening are visible. Two are located along the bar, while the highest reddening is found in the star-forming wing of the SMC. In general, the regions with higher reddening are in good spatial agreement with infrared reddening maps as well as with reddening estimations of other studies. The position-dependent reddening values from the RC method are available via the German Astrophysical Virtual Observatory interface.

Haschke, Raoul; Grebel, Eva K.; Duffau, Sonia, E-mail: haschke@ari.uni-heidelberg.de [Astronomisches Rechen-Institut, Zentrum fuer Astronomie der Universitaet Heidelberg, Moenchhofstrasse 12-14, D-69120 Heidelberg (Germany)

2011-05-15T23:59:59.000Z

72

DISCOVERY AND ANALYSIS OF 21 {mu}m FEATURE SOURCES IN THE MAGELLANIC CLOUDS  

Science Conference Proceedings (OSTI)

Spitzer Space Telescope mid-infrared spectroscopy has been obtained for 15 carbon-rich protoplanetary nebulae (PPNe) in the Large Magellanic Cloud (LMC) and for two other such stars in the Small Magellanic Cloud (SMC). Of these 17 PPNe, the unidentified 21 {mu}m feature is strong in 7 spectra, weak in 2 spectra, and very weak or questionable in 4 spectra. Two of the four spectra without the 21 {mu}m feature have a very strong feature near 11 {mu}m, similar to a feature observed in some carbon-rich planetary nebulae (PNe) in the LMC. We attribute this feature to unusual SiC dust, although the feature-to-continuum ratio is much larger than for SiC features in Galactic or Magellanic Cloud carbon star spectra. The remaining two objects show typical carbon-rich PPNe spectra with no 21 {mu}m features. One of the LMC objects that lacks the 21 {mu}m feature and one SMC object with a questionable 21 {mu}m detection may have mixed dust chemistries based upon their spectral similarity to Galactic [WC] PNe. The 13 objects that either definitely or may show the 21 {mu}m feature have distinct dust shell properties compared to the Galactic 21 {mu}m objects-the 21 {mu}m features are weaker, the estimated dust temperatures are significantly higher, the unidentified infrared (UIR) bands are stronger, and the UIRs show more structure. Four of the 21 {mu}m objects appear to show normal SiC emission features in their spectra. Many of the PPNe show strong 30 {mu}m features, although this feature carries less of the total mid-infrared emission than is normally the case for the Galactic 21 {mu}m PPNe. The LMC objects are in the LMC halo rather than in the LMC bar. The estimated luminosities of these PPNe vary from 4700 to 12,500 L{sub sun}.

Volk, Kevin; Meixner, Margaret; Gordon, Karl D. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Hrivnak, Bruce J. [Department of Physics and Astronomy, Valparaiso University, Valparaiso, IN 46383 (United States); Matsuura, Mikako [Department of Physics and Astronomy, UCL-Institute of Origins, University College London, Gower Street, London WC1E 6BT (United Kingdom); Bernard-Salas, Jeronimo [Institut d Astrophysique Spatiale, CNRS/Universite Paris-Sud 11, 91405, Orsay (France); Szczerba, Ryszard [N. Copernicus Astronomical Center, Rabianska 8, 87-100 Torun (Poland); Sloan, G. C. [Department of Astronomy, Cornell University, Ithaca, NY 14853 (United States); Kraemer, Kathleen E. [Air Force Research Laboratory, AFRL/RVBYB, 29 Randolph Road, Hanscom AFB, MA 01731 (United States); Van Loon, Jacco Th. [Astrophysics Group, Lennard-Jones Laboratories, Keele University, Staffordshire ST5 5BG (United Kingdom); Kemper, F.; Woods, Paul M.; Zijlstra, Albert A. [Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL (United Kingdom); Sahai, Raghvendra [Jet Propulsion Laboratory, MS 183-900, California Institute of Technology, Pasadena, CA 91109 (United States); Gruendl, Robert A. [Astronomy Department, University of Illinois, 1002 West Green Street, Urbana, IL 61801 (United States); Tielens, Alexander G. G. M. [Leiden Observatory, P.O. Box 9513, NL-2300 RA Leiden (Netherlands); Indebetouw, Remy [Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22903 (United States); Marengo, Massimo, E-mail: volk@stsci.edu [Department of Physics and Astronomy, Iowa State University, A313E Zaffarano, Ames, IA 50011 (United States)

2011-07-10T23:59:59.000Z

73

Jenseits des Standard Modells  

NLE Websites -- All DOE Office Websites (Extended Search)

The Standard Model The Standard Model Unngelöste Rätsel Jenseits des Standard Modells Das Standard Modell gibt auf viele Fragen, über Struktur und Stabilität der Materie eine Antwort. Dazu braucht es nur die sechs Sorten von Quarks und Leptonen und die vier fundamentalen Kräfte. Aber das Standard Modell ist nicht vollständig; es gibt noch viele unbeantwortete Fragen. Eigentlich sollten wir aus Gründen der Symmetrie im Weltraum gleichviel Materie wie Antimaterie beobachten. Wir finden aber praktisch nur normale Materie! Warum? Woraus besteht die "Dunkle Materie", die wir nicht sehen können, die aber im Universum sichtbare Gravitationswirkungen zeigt? Warum kann das Standard Modell die Massen der Teilchen nicht vorhersagen? Sind Quarks and Leptonen wirklich fundamentae Teilchen, oder sind sie aus noch elementareren Partikeln aufgebaut?

74

IDENTIFICATION OF A NEW RELATIVELY OLD STAR CLUSTER IN THE SMALL MAGELLANIC CLOUD  

Science Conference Proceedings (OSTI)

We present results on the age and metallicity estimates of the astonishingly unstudied Small Magellanic Cloud (SMC) cluster (ESO 51-SC09), from CCD BVI photometry obtained at the ESO NTT with the EMMI attached. ESO 51-SC09 turns out to be a relatively small cluster (FWHM = 10 {+-} 1 pc) located {approx}4 Degree-Sign northward from the galaxy center. We report for the first time a mean cluster age of 7.0 {+-} 1.3 Gyr and a mean cluster metallicity of [Fe/H] = -1.00 {+-} 0.15 dex, concluding that ESO 51-SC09 belongs to the group of the oldest SMC clusters. We found that the cluster is projected onto an older (age {approx}10-13 Gyr) and more metal-poor ([Fe/H] = -1.3 {+-} 0.2 dex) dominant field stellar population, so that the cluster could have reached its current location because of its orbital motion.

Piatti, Andres E., E-mail: andres@iafe.uba.ar [Instituto de Astronomia y Fisica del Espacio, CC 67, Suc. 28, 1428 Ciudad de Buenos Aires (Argentina)

2012-09-10T23:59:59.000Z

75

Physical parameters of the Small Magellanic Cloud RR Lyrae stars and the distance scale  

E-Print Network (OSTI)

We present a careful and detailed light curve analysis of RR Lyrae stars in the Small Magellanic Cloud (SMC) discovered by the Optical Gravitational Lensing Experiment (OGLE) project. Out of 536 single mode RR Lyrae stars selected from the database, we have investigated the physical properties of 335 `normal looking' RRab stars and 17 RRc stars that have good quality photometric light curves. We have also been able to estimate the distance modulus of the cloud which is in good agreement with those determined from other independent methods. The Fourier decomposition method has been used to study the basic properties of these variables. Accurate Fourier decomposition parameters of 536 RR Lyrae stars in the OGLE-II database are computed. Empirical relations between the Fourier parameters and some physical parameters of these variables have been used to estimate the physical parameters for the stars from the Fourier analysis. Further, the Fourier decomposition of the light curves of the SMC RR Lyrae stars yields ...

Deb, Sukanta

2009-01-01T23:59:59.000Z

76

Are the Magellanic Clouds on their First Passage about the Milky Way?  

E-Print Network (OSTI)

Recent proper motion measurements of the Large and Small Magellanic Clouds (LMC and SMC, respectively) by Kallivayalil et al (2006a,b) suggest that the 3D velocities of the Clouds are substantially higher (~100 km/s) than previously estimated and now approach the escape velocity of the Milky Way (MW). Previous studies have also assumed that the Milky Way can be adequately modeled as an isothermal sphere to large distances. Here we re-examine the orbital history of the Clouds using the new velocities and a LCDM-motivated MW model with virial mass Mvir = 1e12 Msun (e.g. Klypin et al 2002). We conclude that the Clouds are either currently on their first passage about the MW or, if the MW can be accurately modeled by an isothermal sphere to distances >200 kpc (i.e., Mvir > 2e12 Msun), that their orbital period and apogalacticon distance must be a factor of two larger than previously estimated, increasing to 3 Gyr and 200 kpc, respectively. A first passage scenario is consistent with the fact that the LMC and SMC appear to be outliers when compared to other satellite galaxies of the MW: they are irregular in appearance and are moving faster. We discuss the implications of this orbital analysis for our understanding of the star formation history, the nature of the warp in the MW disk and the origin of the Magellanic Stream (MS), a band of HI gas trailing the LMC and SMC that extends roughly 100 degrees across the sky. Specifically, as a consequence of the new orbital history of the Clouds, the origin of the MS may not be explainable by current tidal and ram pressure stripping models.

Gurtina Besla; Nitya Kallivayalil; Lars Hernquist; Brant Robertson; T. J. Cox; Roeland P. van der Marel; Charles Alcock

2007-03-08T23:59:59.000Z

77

Facult des lettres Facult de psychologie  

E-Print Network (OSTI)

Faculté des lettres Faculté de psychologie et des sciences de l'éducation linguistique et'ac- ceptation suite à la procédure d'admission Maîtrise en linguistique (Faculté des lettres) Faculté des'université de genève, une forma- tion interfacultaire en linguistique et en psychologie est offerte aux

Halazonetis, Thanos

78

FACULT DES LETTRES Dpartement de linguistique  

E-Print Network (OSTI)

FACULT? DES LETTRES Département de linguistique Linguis'que et psychologie Baccalauréat universitaire #12;FACULT? DES LETTRES Département de linguistique La faculté de langage «La faculté DES LETTRES Département de linguistique Pourquoi un BA interfacultaire? CeVe forma

Halazonetis, Thanos

79

Histoire philosophique des deux Indes, 1770  

E-Print Network (OSTI)

enfans du bas-ge. Tout autour, on voyoit les cases de ceux de sa postrit qui toient maris. Ces cabanes avoient pour colonnes des pieux, du chaume pour tot; & pour meubles, des armes, des lits de coton sans art & sans travail, quelques corbeilles...

Raynal

2006-11-08T23:59:59.000Z

80

TRAITEMENT DES EFFLUENTS WASTE TREATMENT  

E-Print Network (OSTI)

TRAITEMENT DES EFFLUENTS WASTE TREATMENT Anaerobic digestion of pig manure B. DE LA FARGE Michèle properties of the methanized effluemt are preserved. A trial on anaerobic digestion of untreated pig manure technique du Porc, Station expérimentale, Les Cabrière.l, 12200 Villefranche-de-Rouer/(ue Frctnce Anaerobic

Recanati, Catherine

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


81

CANDIDATES OF H{alpha} EMITTING REGIONS IN THE MAGELLANIC STREAM IV CLOUD  

Science Conference Proceedings (OSTI)

From H{alpha} narrowband observations, we identified three H{alpha} emitting regions in the direction of Magellanic Stream IV (MS IV). They consist of three parallel filaments of 2 arcmin width and 6-30 arcmin length at 12 arcmin intervals. Their mean surface brightness (SB) is {approx}2 Multiplication-Sign 10{sup -18} erg s{sup -1} cm{sup -2} arcsec{sup -2}. Because of their low SB, the regions were not detected in previous H{alpha} surveys. In the H I map, the position of the filaments overlap MS, suggesting that they are parts of the MS, but there also exists a local H I structure. If the filaments are associated with the MS, the sizes are 30 pc Multiplication-Sign 100-500 pc. The filaments lie at the leading edge of a downstream cloud, which supports shock heating and its propagation (shock cascade) model for the ionizing source. If they are local objects, on the other hand, Fossil Stroemgren Trails of more than two stars is a possible interpretation, and the sizes would be 0.1 pc Multiplication-Sign 0.3-1.5 pc at 180 pc distance. The positional information of the H{alpha} filaments presented in this Letter enables future spectroscopic observations to clarify their nature.

Yagi, Masafumi; Komiyama, Yutaka [Optical and Infrared Astronomy Division, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Yoshida, Michitoshi, E-mail: YAGI.Masafumi@nao.ac.jp [Hiroshima Astrophysical Science Center, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526 (Japan)

2012-04-10T23:59:59.000Z

82

EXTENDED STAR FORMATION IN THE INTERMEDIATE-AGE LARGE MAGELLANIC CLOUD STAR CLUSTER NGC 2209  

SciTech Connect

We present observations of the 1 Gyr old star cluster NGC 2209 in the Large Magellanic Cloud made with the GMOS imager on the Gemini South Telescope. These observations show that the cluster exhibits a main-sequence turnoff that spans a broader range in luminosity than can be explained by a single-aged stellar population. This places NGC 2209 amongst a growing list of intermediate-age (1-3 Gyr) clusters that show evidence for extended or multiple epochs of star formation of between 50 and 460 Myr in extent. The extended main-sequence turnoff observed in NGC 2209 is a confirmation of the prediction in Keller et al. made on the basis of the cluster's large core radius. We propose that secondary star formation is a defining feature of the evolution of massive star clusters. Dissolution of lower mass clusters through evaporation results in only clusters that have experienced secondary star formation surviving for a Hubble time, thus providing a natural connection between the extended main-sequence turnoff phenomenon and the ubiquitous light-element abundance ranges seen in the ancient Galactic globular clusters.

Keller, Stefan C.; Mackey, A. Dougal; Da Costa, Gary S. [Research School of Astronomy and Astrophysics, Australian National University, Canberra (Australia)

2012-12-10T23:59:59.000Z

83

Observations of ground-state OH in the Large Magellanic Cloud  

E-Print Network (OSTI)

We have carried out a series of observations of the 1665- and 1667-MHz transitions of the 2Pi_3/2, J=3/2 OH ground state towards six selected HII regions in the Large Magellanic Cloud (IRAS 05011-6815 and MRC 0510-689, 0513-694B, 0539-691, 0540-696B, 0540-697A) using the Australia Telescope Compact Array. The study has provided the first accurate positions for known 1665- and 1667-MHz OH masers as well as detecting several new masers. The regions all contain H_2O or CH_3OH masers but OH masers were detected in only four. The 1.6-GHz continuum emission was also imaged to investigate its spatial relationship to the associated OH maser. Although some masers are close to compact continuum components, in other cases they are near the continuum distribution boundaries and perhaps have been created as a result of the HII region interacting with the surrounding interstellar medium.

K. J. Brooks; J. B. Whiteoak

1997-10-16T23:59:59.000Z

84

Chemical and structural analysis of the Large Magellanic Cloud using the fundamental mode RR Lyrae stars  

E-Print Network (OSTI)

We present a careful and detailed light curve analysis of publicly available $I$-band data on fundamental mode RR Lyrae (RRab) stars of the Large Magellanic Cloud (LMC) obtained by the Optical Gravitational Lensing Experiment (OGLE) phase-III project. Using the Fourier parameters of $13,095$ RRab stars, metallicities and absolute magnitudes of individual stars are obtained. The representation of stars on the $P-\\phi_{31}^{V}$ plane shows the existence of three significant metallicity groups with mean metallicities as $-1.20 \\pm 0.12$ dex, $-1.57 \\pm 0.10$ dex and $-1.89 \\pm 0.09$ dex. The corresponding absolute magnitudes of these three groups are obtained as $0.70\\pm 0.08$ mag, $0.59 \\pm 0.06$ mag and $0.49 \\pm 0.08$ mag, respectively. Distribution of these three groups as a function of vertical $|z|$ distance indicates that the formation of the LMC disk predates the formation of the inner halo. Issue of the existence of a metallicity gradient as a function of galactocentric distances has also been addressed...

Deb, Sukanta

2013-01-01T23:59:59.000Z

85

SUPERGIANT SHELLS AND MOLECULAR CLOUD FORMATION IN THE LARGE MAGELLANIC CLOUD  

Science Conference Proceedings (OSTI)

We investigate the influence of large-scale stellar feedback on the formation of molecular clouds in the Large Magellanic Cloud (LMC). Examining the relationship between H I and {sup 12}CO(J = 1-0) in supergiant shells (SGSs), we find that the molecular fraction in the total volume occupied by SGSs is not enhanced with respect to the rest of the LMC disk. However, the majority of objects ({approx}70% by mass) are more molecular than their local surroundings, implying that the presence of a supergiant shell does on average have a positive effect on the molecular gas fraction. Averaged over the full SGS sample, our results suggest that {approx}12%-25% of the molecular mass in supergiant shell systems was formed as a direct result of the stellar feedback that created the shells. This corresponds to {approx}4%-11% of the total molecular mass of the galaxy. These figures are an approximate lower limit to the total contribution of stellar feedback to molecular cloud formation in the LMC, and constitute one of the first quantitative measurements of feedback-triggered molecular cloud formation in a galactic system.

Dawson, J. R.; Dickey, John M. [School of Mathematics and Physics, University of Tasmania, Sandy Bay Campus, Churchill Avenue, Sandy Bay, TAS 7005 (Australia)] [School of Mathematics and Physics, University of Tasmania, Sandy Bay Campus, Churchill Avenue, Sandy Bay, TAS 7005 (Australia); McClure-Griffiths, N. M. [Australia Telescope National Facility, CSIRO Astronomy and Space Science, Marsfield NSW 2122 (Australia)] [Australia Telescope National Facility, CSIRO Astronomy and Space Science, Marsfield NSW 2122 (Australia); Wong, T. [Astronomy Department, University of Illinois, Urbana, IL 61801 (United States)] [Astronomy Department, University of Illinois, Urbana, IL 61801 (United States); Hughes, A. [Max-Planck-Institut fuer Astronomie, Koenigstuhl 17, D-69117, Heidelberg (Germany)] [Max-Planck-Institut fuer Astronomie, Koenigstuhl 17, D-69117, Heidelberg (Germany); Fukui, Y. [Department of Physics and Astrophysics, Nagoya University, Chikusa-ku, Nagoya (Japan)] [Department of Physics and Astrophysics, Nagoya University, Chikusa-ku, Nagoya (Japan); Kawamura, A., E-mail: joanne.dawson@utas.edu.au [National Astronomical Observatory of Japan, Tokyo 181-8588 (Japan)

2013-01-20T23:59:59.000Z

86

The Mass Distribution and Assembly of the Milky Way from the Properties of the Magellanic Clouds  

SciTech Connect

We present a new measurement of the mass of the Milky Way (MW) based on observed properties of its largest satellite galaxies, the Magellanic Clouds (MCs), and an assumed prior of a {Lambda}CDM universe. The large, high-resolution Bolshoi cosmological simulation of this universe provides a means to statistically sample the dynamical properties of bright satellite galaxies in a large population of dark matter halos. The observed properties of the MCs, including their circular velocity, distance from the center of the MW, and velocity within the MW halo, are used to evaluate the likelihood that a given halo would have each or all of these properties; the posterior probability distribution function (PDF) for any property of the MW system can thus be constructed. This method provides a constraint on the MW virial mass, 1.2{sup +0.7} - {sub 0.4}(stat.){sup +0.3} - {sub 0.3}(sys.) x 10{sup 12} M {circle_dot} (68% confidence), which is consistent with recent determinations that involve very different assumptions. In addition, we calculate the posterior PDF for the density profile of the MW and its satellite accretion history. Although typical satellites of 10{sup 12} M {circle_dot} halos are accreted over a wide range of epochs over the last 10 Gyr, we find a {approx}72% probability that the MCs were accreted within the last Gyr, and a 50% probability that they were accreted together.

Busha, Michael T.; /KIPAC, Menlo Park /Zurich U.; Marshall, Philip J.; /KIPAC, Menlo Park /Oxford U.; Wechsler, Risa H.; /KIPAC, Menlo Park /SLAC; Klypin, Anatoly; /New Mexico State U.; Primack, Joel; /UC, Santa Cruz, Phys. Dept.

2012-02-29T23:59:59.000Z

87

THE MASS DISTRIBUTION AND ASSEMBLY OF THE MILKY WAY FROM THE PROPERTIES OF THE MAGELLANIC CLOUDS  

SciTech Connect

We present a new measurement of the mass of the Milky Way (MW) based on observed properties of its largest satellite galaxies, the Magellanic Clouds (MCs), and an assumed prior of a {Lambda}CDM universe. The large, high-resolution Bolshoi cosmological simulation of this universe provides a means to statistically sample the dynamical properties of bright satellite galaxies in a large population of dark matter halos. The observed properties of the MCs, including their circular velocity, distance from the center of the MW, and velocity within the MW halo, are used to evaluate the likelihood that a given halo would have each or all of these properties; the posterior probability distribution function (PDF) for any property of the MW system can thus be constructed. This method provides a constraint on the MW virial mass, 1.2{sup +0.7}{sub -0.4} (stat.){sup +0.3}{sub -0.3} (sys.) Multiplication-Sign 10{sup 12} M{sub Sun} (68% confidence), which is consistent with recent determinations that involve very different assumptions. In addition, we calculate the posterior PDF for the density profile of the MW and its satellite accretion history. Although typical satellites of 10{sup 12} M{sub Sun} halos are accreted over a wide range of epochs over the last 10 Gyr, we find a {approx}72% probability that the MCs were accreted within the last Gyr, and a 50% probability that they were accreted together.

Busha, Michael T.; Marshall, Philip J.; Wechsler, Risa H. [Kavli Institute for Particle Astrophysics and Cosmology, Physics Department, Stanford University, Stanford, CA 94305 (United States); Klypin, Anatoly [Astronomy Department, New Mexico State University, Las Cruces, NM 88003 (United States); Primack, Joel, E-mail: mbusha@physik.uzh.ch, E-mail: pjm@slac.stanford.edu, E-mail: rwechsler@stanford.edu, E-mail: aklypin@nmsu.edu, E-mail: joel@ucsc.edu [Department of Physics, University of California, Santa Cruz, CA 95064 (United States)

2011-12-10T23:59:59.000Z

88

Variable Stars in Large Magellanic Cloud Globular Clusters I: NGC 1466  

E-Print Network (OSTI)

This is the first in a series of papers studying the variable stars in Large Magellanic Cloud globular clusters. The primary goal of this series is to better understand how the RR Lyrae stars in Oosterhoff-intermediate systems compare to those in Oosterhoff I/II systems. In this paper we present the results of our new time-series BV photometric study of NGC 1466. A total of 62 variables were identified in the cluster, of which 16 are new discoveries. The variables include 30 RRab stars, 11 RRc's, 8 RRd's, 1 candidate RR Lyrae, 2 long-period variables, 1 potential anomalous Cepheid, and 9 variables of undetermined classification. We present photometric parameters for these variables. For the RR Lyrae stars physical properties derived from Fourier analysis of their light curves are presented. The RR Lyrae stars were used to determine a reddening-corrected distance modulus of (m-M)0 = 18.43 +/- 0.15. We discuss several different indicators of Oosterhoff type and find NGC 1466 to be an Oosterhoff-intermediate obj...

Kuehn, Charles A; Catelan, Mrcio; Pritzl, Barton J; De Lee, Nathan; Borissova, Jura

2011-01-01T23:59:59.000Z

89

Variable Stars in Large Magellanic Cloud Globular Clusters II: NGC 1786  

E-Print Network (OSTI)

This is the second in a series of papers studying the variable stars in Large Magellanic Cloud globular clusters. The primary goal of this series is to study how RR Lyrae stars in Oosterhoff-intermediate systems compare to their counterparts in Oosterhoff I/II systems. In this paper, we present the results of our new time-series BV photometeric study of the globular cluster NGC 1786. A total of 65 variable stars were identified in our field of view. These variables include 53 RR Lyraes (27 RRab, 18 RRc, and 8 RRd), 3 classical Cepheids, 1 Type II Cepheid, 1 Anomalous Cepheid, 2 eclipsing binaries, 3 Delta Scuti/SX Phoenicis variables, and 2 variables of undetermined type. Photometeric parameters for these variables are presented. We present physical properties for some of the RR Lyrae stars, derived from Fourier analysis of their light curves. We discuss several different indicators of Oosterhoff type which indicate that the Oosterhoff classification of NGC 1786 is not as clear cut as what is scene in most gl...

Kuehn, Charles A; Catelan, Marcio; Pritzl, Barton J; De Lee, Nathan; Borissova, Jura

2012-01-01T23:59:59.000Z

90

Facult des arts et des sciences Dpartement de linguistique et de traduction  

E-Print Network (OSTI)

Faculté des arts et des sciences Département de linguistique et de traduction ?VALUATION DE LA vous remercions de votre précieuse collaboration au programme de stages du Département de linguistique

Parrott, Lael

91

Dpartement de linguistique et de traduction Facult des arts et des sciences  

E-Print Network (OSTI)

Département de linguistique et de traduction Faculté des arts et des sciences Poste de professeur(e) invité(e) en linguistique Le Département de linguistique et de traduction sollicite des candidatures pour occuper un poste de professeur(e) invité(e) en linguistique, avec une spécialisation en sémantique

Montréal, Université de

92

Conception et test intgr des dispositifs analogiques, mixtes et microsystmes.  

E-Print Network (OSTI)

??Cette Habilitation Diriger des Recherches dcrit les travaux de recherche du candidat sur la conception et le test intgr des dispositifs analogiques, mixtes et (more)

Mir, S.

93

THE DUST BUDGET OF THE SMALL MAGELLANIC CLOUD: ARE ASYMPTOTIC GIANT BRANCH STARS THE PRIMARY DUST SOURCE AT LOW METALLICITY?  

Science Conference Proceedings (OSTI)

We estimate the total dust input from the cool evolved stars in the Small Magellanic Cloud, using the 8 {mu}m excess emission as a proxy for the dust-production rate (DPR). We find that asymptotic giant branch (AGB) and red supergiant (RSG) stars produce (8.6-9.5) Multiplication-Sign 10{sup -7} M{sub Sun} yr{sup -1} of dust, depending on the fraction of far-infrared sources that belong to the evolved star population (with 10%-50% uncertainty in individual DPRs). RSGs contribute the least (budget, this suggests that dust must grow in the ISM or be formed by another unknown mechanism.

Boyer, M. L.; Gordon, K. D.; Meixner, M.; Sargent, B. A. [STScI, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Srinivasan, S. [UPMC-CNRS UMR7095, Institut d'Astrophysique de Paris, F-75014 Paris (France); Riebel, D. [Department of Physics and Astronomy, The Johns Hopkins University, Homewood Campus, Baltimore, MD 21218 (United States); McDonald, I. [Jodrell Bank Centre for Astrophysics, Alan Turing Building, University of Manchester, Manchester M13 9PL (United Kingdom); Van Loon, J. Th. [Astrophysics Group, Lennard-Jones Laboratories, Keele University, Staffordshire ST5 5BG (United Kingdom); Clayton, G. C. [Department of Physics and Astronomy, Louisiana State University, 233-A Nicholson Hall, Tower Dr., Baton Rouge, LA 70803-4001 (United States); Sloan, G. C., E-mail: mboyer@stsci.edu [Astronomy Department, Cornell University, Ithaca, NY 14853-6801 (United States)

2012-03-20T23:59:59.000Z

94

AGE AND MASS FOR 920 LARGE MAGELLANIC CLOUD CLUSTERS DERIVED FROM 100 MILLION MONTE CARLO SIMULATIONS  

SciTech Connect

We present new age and mass estimates for 920 stellar clusters in the Large Magellanic Cloud (LMC) based on previously published broadband photometry and the stellar cluster analysis package, MASSCLEANage. Expressed in the generic fitting formula, d{sup 2} N/dMdt{proportional_to}M{sup {alpha}} t{sup {beta}}, the distribution of observed clusters is described by {alpha} = -1.5 to -1.6 and {beta} = -2.1 to -2.2. For 288 of these clusters, ages have recently been determined based on stellar photometric color-magnitude diagrams, allowing us to gauge the confidence of our ages. The results look very promising, opening up the possibility that this sample of 920 clusters, with reliable and consistent age, mass, and photometric measures, might be used to constrain important characteristics about the stellar cluster population in the LMC. We also investigate a traditional age determination method that uses a {chi}{sup 2} minimization routine to fit observed cluster colors to standard infinite-mass limit simple stellar population models. This reveals serious defects in the derived cluster age distribution using this method. The traditional {chi}{sup 2} minimization method, due to the variation of U, B, V, R colors, will always produce an overdensity of younger and older clusters, with an underdensity of clusters in the log (age/yr) = [7.0, 7.5] range. Finally, we present a unique simulation aimed at illustrating and constraining the fading limit in observed cluster distributions that includes the complex effects of stochastic variations in the observed properties of stellar clusters.

Popescu, Bogdan; Hanson, M. M. [Department of Physics, University of Cincinnati, P.O. Box 210011, Cincinnati, OH 45221-0011 (United States); Elmegreen, Bruce G., E-mail: popescb@mail.uc.edu, E-mail: margaret.hanson@uc.edu, E-mail: bge@us.ibm.com [IBM Research Division, T. J. Watson Research Center, 1101 Kitchawan Road, Yorktown Heights, NY 10598 (United States)

2012-06-01T23:59:59.000Z

95

A RARE EARLY-TYPE STAR REVEALED IN THE WING OF THE SMALL MAGELLANIC CLOUD  

SciTech Connect

Sk 183 is the visually brightest star in the N90 nebula, a young star-forming region in the Wing of the Small Magellanic Cloud (SMC). We present new optical spectroscopy from the Very Large Telescope which reveals Sk 183 to be one of the most massive O-type stars in the SMC. Classified as an O3-type dwarf on the basis of its nitrogen spectrum, the star also displays broadened He I absorption, which suggests a later type. We propose that Sk 183 has a composite spectrum and that it is similar to another star in the SMC, MPG 324. This brings the number of rare O2- and O3-type stars known in the whole of the SMC to a mere four. We estimate physical parameters for Sk 183 from analysis of its spectrum. For a single-star model, we estimate an effective temperature of 46 {+-} 2 kK, a low mass-loss rate of {approx}10{sup -7} M{sub Sun} yr{sup -1}, and a spectroscopic mass of 46{sup +9}{sub -8} M{sub Sun} (for an adopted distance modulus of 18.7 mag to the young population in the SMC Wing). An illustrative binary model requires a slightly hotter temperature ({approx}47.5 kK) for the primary component. In either scenario, Sk 183 is the earliest-type star known in N90 and will therefore be the dominant source of hydrogen-ionizing photons. This suggests Sk 183 is the primary influence on the star formation along the inner edge of the nebula.

Evans, C. J. [UK Astronomy Technology Centre, Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Hainich, R.; Oskinova, L. M.; Hamann, W.-R.; Todt, H. [Institute for Physics and Astronomy, University of Potsdam, 14476 Potsdam (Germany); Gallagher III, J. S. [Department of Astronomy, University of Wisconsin-Madison, 5534 Sterling, 475 North Charter St., Madison, WI 53706 (United States); Chu, Y.-H.; Gruendl, R. A. [Astronomy Department, University of Illinois, 1002 W. Green Street, Urbana, IL 61801 (United States); Henault-Brunet, V. [Scottish Universities Physics Alliance (SUPA), Institute for Astronomy, University of Edinburgh, Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom)

2012-07-10T23:59:59.000Z

96

CCD photometric and mass function study of 9 young Large Magellanic Cloud star clusters  

E-Print Network (OSTI)

We present CCD photometric and mass function study of 9 young Large Magellanic Cloud star clusters namely NGC 1767, NGC 1994, NGC 2002, NGC 2003, NGC 2006, SL 538, NGC 2011, NGC 2098 and NGC 2136. The BVRI data reaching down to V ~ 21 mag, are collected from 3.5-meter NTT/EFOSC2 in sub-arcsec seeing conditions. For NGC 1767, NGC 1994, NGC 2002, NGC 2003, NGC 2011 and NGC 2136, broad band photometric CCD data are presented for the first time. Seven of the 9 clusters have ages between 16 to 25 Myr while remaining two clusters have ages $32\\pm4$ Myr (NGC 2098) and $90\\pm10$ Myr (NGC 2136). For 7 younger clusters, the age estimates based on a recent model and the integrated spectra are found to be systematically lower ($\\sim$ 10 Myr) from the present estimate. In the mass range of $\\sim 2 - 12$ $M_{\\odot}$, the MF slopes for 8 out of nine clusters were found to be similar with the value of $\\gamma$ ranging from $-1.90\\pm0.16$ to $-2.28\\pm0.21$. For NGC 1767 it is flatter with $\\gamma = -1.23\\pm0.27$. Mass segregation effects are observed for NGC 2002, NGC 2006, NGC 2136 and NGC 2098. This is consistent with the findings of Kontizas et al. for NGC 2098. Presence of mass segregation in these clusters could be an imprint of star formation process as their ages are significantly smaller than their dynamical evolution time. Mean MF slope of $\\gamma = -2.22\\pm0.16$ derived for a sample of 25 young ($\\le 100$ Myr) dynamically unevolved LMC stellar systems provide support for the universality of IMF in the intermediate mass range $\\sim 2-12 M_{\\odot}$.

B. Kumar; R. Sagar; J. Melnick

2008-01-07T23:59:59.000Z

97

YELLOW SUPERGIANTS IN THE SMALL MAGELLANIC CLOUD: PUTTING CURRENT EVOLUTIONARY THEORY TO THE TEST  

SciTech Connect

The yellow supergiant content of nearby galaxies provides a critical test of massive star evolutionary theory. While these stars are the brightest in a galaxy, they are difficult to identify because a large number of foreground Milky Way stars have similar colors and magnitudes. We previously conducted a census of yellow supergiants within M31 and found that the evolutionary tracks predict a yellow supergiant duration an order of magnitude longer than we observed. Here we turn our attention to the Small Magellanic Cloud (SMC), where the metallicity is 10x lower than that of M31, which is important as metallicity strongly affects massive star evolution. The SMC's large radial velocity ({approx}160 km s{sup -1}) allows us to separate members from foreground stars. Observations of {approx}500 candidates yielded 176 near-certain SMC supergiants, 16 possible SMC supergiants, along with 306 foreground stars, and provide good relative numbers of yellow supergiants down to 12 M {sub sun}. Of the 176 near-certain SMC supergiants, the kinematics predicted by the Besancon model of the Milky Way suggest a foreground contamination of {<=}4%. After placing the SMC supergiants on the Hertzsprung-Russell diagram (HRD) and comparing our results to the Geneva evolutionary tracks, we find results similar to those of the M31 study: while the locations of the stars on the HRD match the locations of evolutionary tracks well, the models overpredict the yellow supergiant lifetime by a factor of 10. Uncertainties about the mass-loss rates on the main sequence thus cannot be the primary problem with the models.

Neugent, Kathryn F.; Massey, Philip; Skiff, Brian [Lowell Observatory, 1400 W Mars Hill Road, Flagstaff, AZ 86001 (United States); Drout, Maria R. [Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52245 (United States); Meynet, Georges [Geneva Observatory, Geneva University, CH-1290 Versoix (Switzerland); Olsen, Knut A. G., E-mail: kneugent@lowell.ed, E-mail: phil.massey@lowell.ed, E-mail: bas@lowell.ed, E-mail: maria-drout@uiowa.ed, E-mail: georges.meynet@unige.c, E-mail: kolsen@noao.ed [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85748 (United States)

2010-08-20T23:59:59.000Z

98

Collation des grades de la Facult des arts et des sciences  

E-Print Network (OSTI)

'études cinématographiques Département de linguistique et de traduction Département de littérature comparée Département des'histoire de l'art et d'études cinématographiques Département de linguistique et de traduction Département de'art...........................................................................................44 #12;ix Département de linguistique et de traduction Majeure en linguistique et mineure

Montréal, Université de

99

Multilinguisme, variation, contact. Des pratiques langagires sur le terrain l'analyse de corpus htrognes.  

E-Print Network (OSTI)

??Ce mmoire de synthse prsente un premier chapitre de positionnements pistmologiques (pratiques langagires, construction des objets, des donnes et des corpus, linguistique de terrain implique, (more)

Lglise, Isabelle

2013-01-01T23:59:59.000Z

100

A WASHINGTON PHOTOMETRIC SURVEY OF THE LARGE MAGELLANIC CLOUD FIELD STAR POPULATION  

SciTech Connect

We present photometry for an unprecedented database of some 5.5 million stars distributed throughout the Large Magellanic Cloud main body, from 21 fields covering a total area of 7.6 deg{sup 2}, obtained from Washington CT{sub 1} T{sub 2} CTIO 4 m MOSAIC data. Extensive artificial star tests over the whole mosaic image data set and the observed behavior of the photometric errors with magnitude demonstrate the accuracy of the morphology and clearly delineate the position of the main features in the color-magnitude diagrams (CMDs). The representative T{sub 1}(MS TO) mags are on average {approx}0.5 mag brighter than the T{sub 1} mags for the 100% completeness level of the respective field, allowing us to derive an accurate age estimate. We have analyzed the CMD Hess diagrams and used the peaks in star counts at the main sequence turnoff and red clump (RC) locations to age date the most dominant sub-population (or 'representative' population) in the stellar population mix. The metallicity of this representative population is estimated from the locus of the most populous red giant branch track. We use these results to derive age and metallicity estimates for all of our fields. The analyzed fields span age and metallicity ranges covering most of the galaxy's lifetime and chemical enrichment, i.e., ages and metallicities between {approx}1 and 13 Gyr and {approx}-0.2 and -1.2 dex, respectively. We show that the dispersions associated with the mean ages and metallicities represent in general a satisfactory estimate of the age/metallicity spread ({approx}1-3 Gyr/0.2-0.3 dex), although a few subfields have a slightly larger age/metallicity spread. Finally, we revisit the study of the vertical structure (VS) phenomenon, a striking feature composed of stars that extend from the bottom, bluest end of the RC to {approx}0.45 mag fainter. We confirm that the VS phenomenon is not clearly seen in most of the studied fields and suggest that its occurrence is linked to some other condition(s) in addition to the appropriate age, metallicity, and the necessary red giant star density.

Piatti, Andres E. [Instituto de Astronomia y Fisica del Espacio, CC 67, Suc. 28, 1428, Ciudad de Buenos Aires (Argentina); Geisler, Doug; Mateluna, Renee, E-mail: andres@iafe.uba.ar [Departamento de Astronomia, Universidad de Concepcion, Casilla 160-C, Concepcion (Chile)

2012-10-01T23:59:59.000Z

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


101

SPITZER CHARACTERIZATION OF DUST IN THE IONIZED MEDIUM OF THE LARGE MAGELLANIC CLOUD  

SciTech Connect

A systematic investigation of dust emission associated with ionized gas has so far been performed only in our Galaxy and for wavelengths longer than 60 {mu}m. Newly available Spitzer data now offer the opportunity to carry out a similar analysis in the Large Magellanic Cloud (LMC). By cross-correlating Spitzer Surveying the Agents of a Galaxy's Evolution (SAGE) data with the Australia Telescope Compact Array/Parkes H I 21 cm data, the NANTEN {sup 12}CO (J = 1-0) data, and both the Southern H-Alpha Sky Survey Atlas H{alpha} and the Parkes 6 cm data, we investigate the physical properties of dust associated with the different phases of the gas (atomic, molecular, and ionized). In particular, we study the presence and nature of dust from 3.6 to 160 {mu}m and for various regimes of ionized gas, spanning emission measures from {approx}1 pc cm{sup -6} (diffuse component) to {approx}10{sup 3}pc cm{sup -6} (H II regions). Using a dust emission model and testing our results with several radiation field spectra, we show that dust in ionized gas is warmer than dust associated with other phases (atomic and molecular). We also find a decrease of the polycyclic aromatic hydrocarbon (PAH) relative abundance with respect to big grains, as well as an increase of the near-infrared (NIR) continuum. These three results (i.e., warmer temperature, decrease of PAH abundance, and increase of the NIR continuum) are found consistently for all regimes of ionized gas. On the contrary, the molecular phase appears to provide favorable conditions for the survival of PAHs. Furthermore, the very small grain relative abundance tends to increase in the ionized phase, especially in bright H II regions. Last but not least, our analysis shows that the emissivity of dust associated with ionized gas is lower in the LMC than in our Galaxy and that this difference is not accounted for by the lower metallicity of the LMC.

Paradis, Deborah; Paladini, Roberta; Noriega-Crespo, Alberto [Spitzer Science Center, California Institute of Technology, Pasadena, CA 91125 (United States); Lagache, Guilaine [Institut d'Astrophysique Spatiale, 91405 Orsay (France); Kawamura, Akiko; Fukui, Yasuo [Department of Astrophysics, Nagoya University, Chikusa-ku, Nagoya 464-8602 (Japan); Onishi, Toshikazu [Department of Physical Science, Osaka Prefecture University, Gakuen 1-1, Sakai, Osaka 599-8531 (Japan)

2011-07-01T23:59:59.000Z

102

The Stars Aligned Over the Cornfields: Tobacco Industry Political Influence and Tobacco Policy Making in Iowa 1897-2009  

E-Print Network (OSTI)

Banning Smoking in Restaurants. October 2, 2000. http://11, 2000. 8B. Lewis, R. Restaurant, bar owners pitch banlimits smoking in restaurants, bars. Des Moines Register. (

Epps-Johnson, BA, Tiana; Barnes, JD, Richard; Glantz, PhD, Stanton

2009-01-01T23:59:59.000Z

103

Business Plan for 1st Street Diner and Nightclub.  

E-Print Network (OSTI)

??A business plan was created for a diner and nightclub located in downtown Des Moines, Iowa, and the concept was found to be unique to (more)

Deets, Brian D.

2011-01-01T23:59:59.000Z

104

Dr. John L. Gross  

Science Conference Proceedings (OSTI)

... Des Moines Steel Company, where he worked on various projects including the analysis and design of an ocean-going LNG containment system ...

2013-05-06T23:59:59.000Z

105

CONTRIBUTION A L'ETUDE DES ELASTOMERES ET DES MEMBRANES SOUFFLEES.  

E-Print Network (OSTI)

??Dans le prsent travail, deux aspects complmentaires de la modlisation mcanique des lastomres sont abords. Le premier concerne le choix d'un modle de comportement adapt (more)

Marckmann, Gilles

2004-01-01T23:59:59.000Z

106

Towards a Theory of Proofs of Classical Logic Habilitation diriger des recherches  

E-Print Network (OSTI)

iii 0 Vers une thorie des preuves pour la logique classique v 0.1 Catgories des preuves.............................. vi

Universit Denis; Diderot Paris; Lutz Straburger; Gilles Dowek; Delia Kesner; Christian Retor

2013-01-01T23:59:59.000Z

107

THE DISCOVERY OF A RARE WO-TYPE WOLF-RAYET STAR IN THE LARGE MAGELLANIC CLOUD  

SciTech Connect

While observing OB stars within the most crowded regions of the Large Magellanic Cloud, we happened upon a new Wolf-Rayet (WR) star in Lucke-Hodge 41, the rich OB association that contains S Doradus and numerous other massive stars. At first glance the spectrum resembled that of a WC4 star, but closer examination showed strong O VI {lambda}{lambda}3811, 34 lines, leading us to classify it as a WO4. This is only the second known WO in the LMC, and the first known WO4 (the other being a WO3). This rarity is to be expected due to these stars' short lifespans as they represent the most advanced evolutionary stage in a massive star's lifetime before exploding as supernovae. This discovery shows that while the majority of WRs within the LMC have been discovered, there may be a few WRs left to be found.

Neugent, Kathryn F.; Massey, Philip [Lowell Observatory, 1400 W Mars Hill Road, Flagstaff, AZ 86001 (United States); Morrell, Nidia, E-mail: kneugent@lowell.edu, E-mail: phil.massey@lowell.edu, E-mail: nmorrell@lco.cl [Las Campanas Observatory, Carnegie Observatories, Casilla 601, La Serena (Chile)

2012-12-01T23:59:59.000Z

108

The Global Gas and Dust budge of the Large Magellanic Cloud --- Importance of Asymptotic Giant Branch stars  

E-Print Network (OSTI)

It is still an unresolved problem how much AGB stars can contribute to the overall gas and dust enrichment processes in the interstellar medium within galaxies. We start tackling this problem, by using our test case observational data from the Large Magellanic Cloud (LMC), from which we obtain the global gas and dust budget. The photometric data from the LMC is obtained with the Spitzer Space Telescope. We established an infrared colour classification scheme to select AGB stars, which are based on spectroscopically identified AGB stars. We further confirm a correlation between the Spitzer colour and mass-loss rate, which leads to a measurement of the total mass-loss rate from the entire AGB population in the LMC. Indeed, AGB stars are an important gas and dust source.

Matsuura, M

2010-01-01T23:59:59.000Z

109

CONSTRAINTS ON THE MAGELLANIC CLOUDS' INTERACTION FROM THE DISTRIBUTION OF OB STARS AND THE KINEMATICS OF GIANTS  

SciTech Connect

Young, OB-type candidates are identified in a {approx}7900 deg{sup 2} region encompassing the Large and Small Magellanic Clouds (LMC/SMC) periphery, the Bridge, part of the Magellanic Stream (MS), and Leading Arm (LA). Selection is based on UV, optical, and IR photometry from existing large-area surveys and proper motions from the Southern Proper Motion 4 (SPM4) catalog. The spatial distribution of these young star candidates shows (1) a well-populated SMC wing which continues westward with two branches partially surrounding the SMC, (2) a rather narrow path from the SMC wing eastward toward the LMC which is offset by 1 Degree-Sign -2 Degree-Sign from the high-density H I ridge in the Bridge, (3) a well-populated periphery of the LMC dominated by clumps of stars at the ends of the LMC bar, and (4) a few scattered candidates in the MS and two overdensities in the LA regions above and below the Galactic plane. Additionally, a proper-motion analysis is made of a radial-velocity-selected sample of red giants and supergiants in the LMC, previously shown to be a kinematically and chemically distinct subgroup, most likely captured from the SMC. SPM4 proper motions of these stars also indicate they are distinct from the LMC population. The observational results presented here, combined with the known orbits of the Clouds and other aspects of the LMC morphology, suggest an off-center, moderate to highly inclined collision between the SMC and the LMC's disk that took place between 100 and 200 Myr ago.

Casetti-Dinescu, Dana I.; Girard, Terrence M.; Van Altena, William F. [Astronomy Department, Yale University, P.O. Box 208101, New Haven, CT 06520-8101 (United States); Vieira, Katherine, E-mail: dana.casetti@yale.edu, E-mail: terry.girard@yale.edu, E-mail: william.vanaltena@yale.edu, E-mail: kvieira@cida.ve [Centro de Investigaciones de Astronomia, Apartado Postal 264, Merida 5101-A (Venezuela, Bolivarian Republic of)

2012-07-10T23:59:59.000Z

110

GLOBULAR CLUSTER ABUNDANCES FROM HIGH-RESOLUTION, INTEGRATED-LIGHT SPECTROSCOPY. III. THE LARGE MAGELLANIC CLOUD: Fe AND AGES  

Science Conference Proceedings (OSTI)

In this paper, we refine our method for the abundance analysis of high-resolution spectroscopy of the integrated light of unresolved globular clusters (GCs). This method was previously demonstrated for the analysis of old (>10 Gyr) Milky Way (MW) GCs. Here, we extend the technique to young clusters using a training set of nine GCs in the Large Magellanic Cloud. Depending on the signal-to-noise ratio of the data, we use 20-100 Fe lines per cluster to successfully constrain the ages of old clusters to within a {approx}5 Gyr range, the ages of {approx}2 Gyr clusters to a 1-2 Gyr range, and the ages of the youngest clusters (0.05-1 Gyr) to a {approx}200 Myr range. We also demonstrate that we can measure [Fe/H] in clusters with any age less than 12 Gyr with similar or only slightly larger uncertainties (0.1-0.25 dex) than those obtained for old MW GCs (0.1 dex); the slightly larger uncertainties are due to the rapid evolution in stellar populations at these ages. In this paper, we present only Fe abundances and ages. In the next paper in this series, we present our complete analysis of {approx}20 elements for which we are able to measure abundances. For several of the clusters in this sample, there are no high-resolution abundances in the literature from individual member stars; our results are the first detailed chemical abundances available. The spectra used in this paper were obtained at Las Campanas with the echelle on the du Pont Telescope and with the MIKE spectrograph on the Magellan Clay Telescope.

Colucci, Janet E.; Bernstein, Rebecca A. [Department of Astronomy and Astrophysics, 1156 High Street, UCO/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States); Cameron, Scott A. [Astronomy Department, 500 Church Street, University of Michigan, Ann Arbor, MI 48109-1090 (United States); McWilliam, Andrew, E-mail: jcolucci@ucolick.org, E-mail: rab@ucolick.org, E-mail: sacamero@umich.edu, E-mail: andy@ociw.edu [The Observatories of the Carnegie Institute of Washington, 813 Santa Barbara Street, Pasadena, CA 91101-1292 (United States)

2011-07-01T23:59:59.000Z

111

Service Recherche Bureau des Formations Doctorales  

E-Print Network (OSTI)

. Elle affirme nettement son caractère acadien, dans un paysage linguistique diversifié, consciente d de la linguistique variationniste et des recherches contemporaines en linguistique cognitive (rapport

Naud Frédéric

112

The Des Plaines River -- Part Two  

NLE Websites -- All DOE Office Websites (Extended Search)

a canal through the Chicago Portage, down the Des Plaines valley, and thence to LaSalle-Peru where the Illinois River became navigable in all seasons. The Northwest Territory...

113

Effets de deux procds de traitement des tours aro rfrigrantes vis--vis du dveloppement des biofilms : cas particulier des lgionnelles et des amibes.  

E-Print Network (OSTI)

??L'implication des tours aro-rfrigrantes dites ouvertes , dans les cas de lgionellose, demeure l'heure actuel un problme de sant public malgr la multitude (more)

Chaabna, Zineddine

2013-01-01T23:59:59.000Z

114

Facult des arts et des sciences Dpartement de linguistique et de traduction  

E-Print Network (OSTI)

Faculté des arts et des sciences Département de linguistique et de traduction Directives concernant'ont pas de service linguistique. Rapport de stage Au plus tard un mois après la fin du stage, l

Parrott, Lael

115

Congrs des innovations mcaniques CIM'08 28-29 avril 2008 Sousse Tunisie. Pilotage des processus collaboratifs dans les  

E-Print Network (OSTI)

1er Congrès des innovations mécaniques CIM'08 ­ 28-29 avril 2008 Sousse ­ Tunisie. Pilotage des Manuscrit auteur, publié dans "1er Congrès des innovations mécaniques CIM'08, Sousse : Tunisie (2008)" #12;CIM'08 ­ 28-29 avril 2008 Sousse ­ Tunisie. 2 1. Introduction Les systèmes PLM sont des systèmes d

Paris-Sud XI, Université de

116

U.S. DEPARTMENT OF I!NI!RGY EERE PROJECT MANAGEMENT CENTER NFPA DETTIUlIINATION  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

I!NI!RGY I!NI!RGY EERE PROJECT MANAGEMENT CENTER NFPA DETTIUlIINATION RECIPIENT:Magelian Midstream Partners. LP (SEP Sub-recipient of the Iowa Office of Energy STATE: IA Independence) PROJECf TITLE: Magellan Des Moines Biodiesel Terminal Project Page 10f3 Funding Opportunity Announcement Number Procurement Instrument Number NEPA Control Number CID Number DE FDA 000052 OE-EE-OOOO162 GFQ-OOOO162-016 EE162 Based on my review orlbe information concerning tbe proposed action, as NEPA Compliance Officer (authorl7.ed under DOE Order 451.JA), I have made the following determination: ex, EA, ~:IS APPI<:NDIX AND NUMBER: Description: 85.1 Actions to oonserve energy, demonstrate potential energy conservation, and promote energy-efficiency that do not increase the indoor concentrations of potentially harmful substances. These actions may involve financial and techmcal

117

THE AGE-METALLICITY RELATIONSHIP OF THE LARGE MAGELLANIC CLOUD FIELD STAR POPULATION FROM WIDE-FIELD WASHINGTON PHOTOMETRY  

SciTech Connect

We analyze age and metallicity estimates for an unprecedented database of some 5.5 million stars distributed throughout the Large Magellanic Cloud (LMC) main body, obtained from CCD Washington CT{sub 1} photometry, reported on in Piatti et al. We produce a comprehensive field star age-metallicity relationship (AMR) from the earliest epoch until {approx}1 Gyr ago. This AMR reveals that the LMC has not evolved chemically as either a closed-box or bursting system, exclusively, but as a combination of both scenarios that have varied in relative strength over the lifetime of the galaxy, although the bursting model falls closer to the data in general. Furthermore, while old and metal-poor field stars have been preferentially formed in the outer disk, younger and more metal-rich stars have mostly been formed in the inner disk, confirming an outside-in formation. We provide evidence for the formation of stars between 5 and 12 Gyr, during the cluster age gap, although chemical enrichment during this period was minimal. We find no significant metallicity gradient in the LMC. We also find that the range in the metallicity of an LMC field has varied during the lifetime of the LMC. In particular, we find only a small range of the metal abundance in the outer disk fields, whereas an average range of {Delta}[Fe/H] = +0.3 {+-} 0.1 dex appears in the inner disk fields. Finally, the cluster and field AMRs show a satisfactory match only for the last 3 Gyr, while for the oldest ages (>11 Gyr), the cluster AMR is a remarkable lower envelope to the field AMR. Such a difference may be due to the very rapid early chemical evolution and lack of observed field stars in this regime, whereas the globular clusters are easily studied. This large difference is not easy to explain as coming from stripped ancient Small Magellanic Cloud (SMC) clusters, although the field SMC AMR is on average {approx}0.4 dex more metal-poor at all ages than that of the LMC but otherwise very similar.

Piatti, Andres E. [Instituto de Astronomia y Fisica del Espacio, CC 67, Suc. 28, 1428 Ciudad de Buenos Aires (Argentina); Geisler, Doug, E-mail: andres@iafe.uba.ar [Departamento de Astronomia, Universidad de Concepcion, Casilla 160-C, Concepcion (Chile)

2013-01-01T23:59:59.000Z

118

Complexification des donnes et des techniques en linguistique : contributions du TAL aux solutions et aux problmes.  

E-Print Network (OSTI)

??Ce mmoire d'habilitation est l'occasion de faire le bilan de mon activit d'enseignant-chercheur en traitement automatique des langues (TAL) dans un laboratoire de linguistique (CLLE-ERSS) (more)

Tanguy, Ludovic

2012-01-01T23:59:59.000Z

119

ANALYSIS OF TWO SMALL MAGELLANIC CLOUD H II REGIONS CONSIDERING THERMAL INHOMOGENEITIES: IMPLICATIONS FOR THE DETERMINATIONS OF EXTRAGALACTIC CHEMICAL ABUNDANCES  

SciTech Connect

We present long-slit spectrophotometry considering the presence of thermal inhomogeneities (t{sup 2}) of two H II regions in the Small Magellanic Cloud (SMC): NGC 456 and NGC 460. Physical conditions and chemical abundances were determined for three positions in NGC 456 and one position in NGC 460, first under the assumption of uniform temperature and then allowing for the possibility of thermal inhomogeneities. We determined t{sup 2} values based on three different methods: (1) by comparing the temperature derived using oxygen forbidden lines with the temperature derived using helium recombination lines (RLs), (2) by comparing the abundances derived from oxygen forbidden lines with those derived from oxygen RLs, and (3) by comparing the abundances derived from ultraviolet carbon forbidden lines with those derived from optical carbon RLs. The first two methods averaged t{sup 2} = 0.067 {+-} 0.013 for NGC 456 and t{sup 2} = 0.036 {+-} 0.027 for NGC 460. These values of t{sup 2} imply that when gaseous abundances are determined with collisionally excited lines they are underestimated by a factor of nearly two. From these objects and others in the literature, we find that in order to account for thermal inhomogeneities and dust depletion, the O/H ratio in low-metallicity H II regions should be corrected by 0.25-0.45 dex depending on the thermal structure of the nebula or by 0.35 dex if such information is not available.

Pena-Guerrero, Maria A.; Peimbert, Antonio; Peimbert, Manuel [Instituto de Astronomia, Universidad Nacional Autonoma de Mexico, Apdo. Postal 70-264, Mexico 04510 D.F. (Mexico); Ruiz, Maria Teresa, E-mail: guerrero@astroscu.unam.mx, E-mail: antonio@astroscu.unam.mx, E-mail: peimbert@astroscu.unam.mx, E-mail: mtruiz@das.uchile.cl [Departamento de Astronomia, Universidad de Chile, Casilla Postal 36D, Santiago de Chile (Chile)

2012-02-20T23:59:59.000Z

120

A MAGELLAN-IMACS-IFU SEARCH FOR DYNAMICAL DRIVERS OF NUCLEAR ACTIVITY. I. REDUCTION PIPELINE AND GALAXY CATALOG  

Science Conference Proceedings (OSTI)

Using the IMACS integral-field unit (IFU) on the 6.5 m Magellan telescope, we have designed the first statistically significant investigation of the two-dimensional distribution and kinematics of ionized gas and stars in the central kiloparsec regions of a well-matched sample of Seyfert and inactive control galaxies selected from the Sloan Digital Sky Survey. The goals of the project are to use the fine spatial sampling (0.2 arcsec pixel{sup -1}) and large wavelength coverage (4000-7000 A) of the IMACS-IFU to search for dynamical triggers of nuclear activity in the central region where active galactic nucleus (AGN) activity and dynamical timescales become comparable, to identify and assess the impact of AGN-driven outflows on the host galaxy and to provide a definitive sample of local galaxy kinematics for comparison with future three-dimensional kinematic studies of high-redshift systems. In this paper, we provide the first detailed description of the procedure to reduce and calibrate data from the IMACS-IFU in 'long mode' to obtain two-dimensional maps of the distribution and kinematics of ionized gas and stars. The sample selection criteria are presented, the observing strategy is described, and resulting maps of the sample galaxies are presented along with a description of the observed properties of each galaxy and the overall observed properties of the sample.

Westoby, P. B.; Mundell, C. G.; Maciejewski, W.; Baldry, I. K. [Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD (United Kingdom); Nagar, N. M. [Astronomy Group, Departamento de Fisica, Universidad de Concepcion, Casilla 160-C, Concepcion (Chile); Emsellem, E. [European Southern Observatory, Karl-Schwarzschild-Str 2, 85748 Garching (Germany); Roth, M. M.; Gerssen, J. [Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam (Germany)

2012-03-01T23:59:59.000Z

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


121

HIGH-RESOLUTION H I DISTRIBUTIONS AND MULTI-WAVELENGTH ANALYSES OF MAGELLANIC SPIRALS NGC 4618 AND NGC 4625  

Science Conference Proceedings (OSTI)

We present a detailed analysis of high-resolution H I observations of the Magellanic spiral galaxies NGC 4618 and NGC 4625. While the H I disk of NGC 4625 is remarkably quiescent with a nearly uniform velocity dispersion and no evidence of H I holes, there is a dynamic interplay between star formation and the distribution of neutral hydrogen in NGC 4618. We calculate the critical density for widespread star formation in each galaxy and find that star formation proceeds even where the surface density of the atomic gas is well below the critical density necessary for global star formation. There are strong spatial correlations in NGC 4618 between UV emission, 1.4 GHz radio continuum emission, and peaks in the H I column density. Despite the apparent overlap of the outer disks of the two galaxies, we find that they are kinematically distinct, indicating that NGC 4618 and NGC 4625 are not interacting. The structure of NGC 4618 and, in particular, the nature of its outer ring are highly suggestive of an interaction, but the timing and nature of such an interaction remain unclear.

Kaczmarek, Jane F. [Now at Sydney Institute for Astronomy, School of Physics A29, The University of Sydney, NSW 2006 (Australia); Wilcots, Eric M., E-mail: jane@astro.wisc.edu, E-mail: ewilcots@astro.wisc.edu [Department of Astronomy, University of Wisconsin Madison, 475 N. Charter Street, Madison, WI 53706 (United States)

2012-08-15T23:59:59.000Z

122

Spitzer Infrared Spectrograph Observations of Magellanic Cloud Planetary Nebulae: the nature of dust in low metallicity circumstellar ejecta  

E-Print Network (OSTI)

We present 5 - 40 micron spectroscopy of 41 planetary nebulae (PNe) in the Magellanic Clouds, observed with the Infrared Spectrograph on board the Spitzer Space Telescope. The spectra show the presence of a combination of nebular emission lines and solid-state features from dust, superimposed on the thermal IR continuum. By analyzing the 25 LMC and 16 SMC PNe in our sample we found that the IR spectra of 14 LMC and 4 SMC PNe are dominated by nebular emission lines, while the other spectra show solid-state features. We observed that the solid-state features are compatible with carbon-rich dust grains (SiC, polycyclic aromatic hydrocarbons (PAHs), etc.) in most cases, except in three PNe showing oxygen-rich dust features. The frequency of carbonaceous dust features is generally higher in LMC than in SMC PNe. The spectral analysis allowed the correlations of the dust characteristics with the gas composition and morphology, and the properties of the central stars. We found that: 1) all PNe with carbonaceous dust features have C/O>1, none of these being bipolar or otherwise highly asymmetric; 2) all PNe with oxygen-rich dust features have C/Oproduction efficiency depends on metallicity, with low metallicity environments not favoring dust production.

L. Stanghellini; P. Garcia-Lario; D. A. Garcia-Hernandez; J. V. Perea-Calderon; J. E. Davies; A. Manchado; E. Villaver; R. A. Shaw

2007-09-04T23:59:59.000Z

123

Energy Efficiency and Conservation Block Grant Program  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

U.S. Department of Energy Categorical Exclusion Determination Form Program or Field Office: Energy Efficiency and Conservation Block Grant Program Project Title IA-City-West Des Moines Location: City West Des Moines IA American Recovery and Reinvestment Act: Proposed Action or Project Description: 1) Fund energy audits (benchmarking) and educational outreach and marketing campaign, 2) create

124

Master Linguistique, apprentissage des langues, informatique  

E-Print Network (OSTI)

Master Linguistique, apprentissage des langues, informatique Formation dispensée par l'UFR Lettres > Formation continue Lieu de formation : Site Gergovia (Clermont-Ferrand) #12;Master Linguistique linguistique générale (syntaxe, sémantique, pragmatique). Dans la partie linguistique appliquée, elle s

Sart, Remi

125

Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results  

E-Print Network (OSTI)

We are performing a uniform and unbiased, ~7x7 degrees imaging survey of the Large Magellanic Cloud (LMC), using the IRAC and MIPS instruments on board the Spitzer Space Telescope in order to survey the agents of a galaxy's evolution (SAGE), the interstellar medium (ISM) and stars in the LMC. The detection of diffuse ISM with column densities >1.2x10^21 H cm^-2 permits detailed studies of dust processes in the ISM. SAGE's point source sensitivity enables a complete census of newly formed stars with masses >3 solar masses that will determine the current star formation rate in the LMC. SAGE's detection of evolved stars with mass loss rates >1x10^-8 solar masses per year will quantify the rate at which evolved stars inject mass into the ISM of the LMC. The observing strategy includes two epochs in 2005, separated by three months, that both mitigate instrumental artifacts and constrain source variability. The SAGE data are non-proprietary. The data processing includes IRAC and MIPS pipelines and a database for mining the point source catalogs, which will be released to the community in support of Spitzer proposal cycles 4 and 5. We present initial results on the epoch 1 data with a special focus on the N79 and N83 region. The SAGE epoch 1 point source catalog has ~4 million sources. The point source counts are highest for the IRAC 3.6 microns band and decrease dramatically towards longer wavelengths consistent with the fact that stars dominate the point source catalogs and that the dusty objects, e.g. young stellar objects and dusty evolved stars that detected at the longer wavelengths, are rare in comparison. We outline a strategy for identifying foreground MW stars, that may comprise as much as 18% of the source list, and background galaxies, that may comprise ~12% of the source list.

Margaret Meixner; Karl D. Gordon; Remy Indebetouw; Joseph L. Hora; Barbara Whitney; Robert Blum; William Reach; Jean-Philippe Bernard; Marilyn Meade; Brian Babler; Charles W. Engelbracht; Bi-Qing For; Karl Misselt; Uma Vijh; Claus Leitherer; Martin Cohen; Ed B. Churchwell; Francois Boulanger; Jay A. Frogel; Yasuo Fukui; Jay Gallagher; Varoujan Gorjian; Jason Harris; Douglas Kelly; Akiko Kawamura; SoYoung Kim; William B. Latter; Suzanne Madden; Ciska Markwick-Kemper; Akira Mizuno; Norikazu Mizuno; Jeremy Mould; Antonella Nota; M. S. Oey; Knut Olsen; Toshikazu Onishi; Roberta Paladini; Nino Panagia; Pablo Perez-Gonzalez; Hiroshi Shibai; Sato Shuji; Linda Smith; Lister Staveley-Smith; A. G. G. M. Tielens; Toshiya Ueta; Schuyler Van Dyk; Kevin Volk; Michael Werner; Dennis Zaritsky

2006-06-14T23:59:59.000Z

126

PROBING THE STRUCTURE AND KINEMATICS OF THE TRANSITION LAYER BETWEEN THE MAGELLANIC STREAM AND THE HALO IN H I  

Science Conference Proceedings (OSTI)

The Magellanic Stream (MS) is a nearby laboratory for studying the fate of cool gas streams injected into a gaseous galactic halo. We investigate properties of the boundary layer between the cool MS gas and the hot Milky Way halo with 21 cm H I observations of a relatively isolated cloud having circular projection in the northern MS. Through averaging and modeling techniques, our observations, obtained with the Robert C. Byrd Green Bank Telescope, reach unprecedented 3{sigma} sensitivity of {approx}1 Multiplication-Sign 10{sup 17} cm{sup -2}, while retaining the telescope's 9.'1 resolution in the essential radial dimension. We find an envelope of diffuse neutral gas with FWHM of 60 km s{sup -1}, associated in velocity with the cloud core having FWHM of 20 km s{sup -1}, extending to 3.5 times the core radius with a neutral mass seven times that of the core. We show that the envelope is too extended to represent a conduction-dominated layer between the core and the halo. Its observed properties are better explained by a turbulent mixing layer driven by hydrodynamic instabilities. The fortuitous alignment of the NGC 7469 background source near the cloud center allows us to combine UV absorption and H I emission data to determine a core temperature of 8350 {+-} 350 K. We show that the H I column density and size of the core can be reproduced when a slightly larger cloud is exposed to Galactic and extragalactic background ionizing radiation. Cooling in the large diffuse turbulent mixing layer envelope extends the cloud lifetime by at least a factor of two relative to a simple hydrodynamic ablation case, suggesting that the cloud is likely to reach the Milky Way disk.

Nigra, Lou; Stanimirovic, Snezana; Gallagher, John S. III [Department of Astronomy, University of Wisconsin, 475 North Charter Street, Madison, WI 53706 (United States); Wood, Kenneth [School of Physics and Astronomy, University of St. Andrews, North Haugh, St. Andrews KY16 9SS (United Kingdom); Nidever, David; Majewski, Steven, E-mail: lou@zooniverse.org, E-mail: sstanimi@astro.wisc.edu, E-mail: jsg@astro.wisc.edu, E-mail: kw25@st-andrews.ac.uk, E-mail: dnidever@virginia.edu, E-mail: srm4n@virginia.edu [Department of Astronomy, University of Virginia, Charlottesville, VA 22904-4325 (United States)

2012-11-20T23:59:59.000Z

127

Interpretation of the Spatial Power Spectra of Neutral Hydrogen in the Galaxy and in the Small Magellanic Cloud  

E-Print Network (OSTI)

Recent 21 cm radio observations of H$_I$ regions in the Small Magellanic Cloud, have revealed spatial power spectra of the intensity, which are quite similar in shape to those previously deduced for the Galaxy. The similarity, in spite the differences in the physical parameters between the Galaxy and the SMC, suggests that the shape of the power spectra reflects some underlying mechanism which is not too sensitive to the environmental specifics. In this paper we present an interpretation for the observational power spectra in terms of a large scale turbulence in the interstellar medium, in which the emitting H$_I$ regions are embedded. The turbulence gives rise to density fluctuations which lead to the observed intensity fluctuations, in the H$_I$ regions. The observational power spectra are used to deduce the turbulence spectral function. In the SMC, the turbulence largest eddies are comparable in scale to the SMC itself. This implies that turbulent mixing should have smoothed out any large scale abundance gradients. Indeed, this seems to be the case, observationally. The turbulence is also expected to amplify and shape up the large scale magnetic field. Indeed, the observational data indicate the existence of a large scale disordered field of the strength expected from energy equilibrium with the turbulent velocity field. The large scale turbulence is most probably generated by instabilities in the large scale flows induced by the tidal close encounter with the LMC $ \\sim 2\\times 10^8{\\rm yr}$ ago. The life-time of the largest eddies is $\\sim 4\\times 10^8{\\rm yr}$ so the turbulence had not yet enough time to decay and persists even though the energy source is no longer there.

Itzhak Goldman

2000-05-01T23:59:59.000Z

128

Diagnostic du colmatage des gnrateurs de vapeur l'aide de modles physiques et statistiques.  

E-Print Network (OSTI)

??Les gnrateurs de vapeur sont d'imposants changeurs de chaleur qui alimentent les turbines des centrales nuclaires eau pressurise. Au cours de leur exploitation, des (more)

Girard, Sylvain

129

Contrle de combustion en transitoires des moteurs combustion interne.  

E-Print Network (OSTI)

??Cette thse traite le problme du contrle de combustion des moteurs automobiles combustion interne. On propose une mthode compltant les stratgies de contrle existantes (more)

Hillion, Mathieu

2009-01-01T23:59:59.000Z

130

prsente au Conservatoire national des arts et mtiers  

E-Print Network (OSTI)

diodes électroluminescentes (LED : Light Emitting Diode). D'une technologie datant des années 60, les LED

Paris-Sud XI, Université de

131

L'inscurit linguistique des professeurs de langues trangres non natifs : le cas des professeurs grecs de franais.  

E-Print Network (OSTI)

??La notion d'inscurit linguistique a t rgulirement explore depuis les annes 1960: les recherches ont t initialement centres autour des questions de prononciation dans diffrents (more)

Roussi, Maria

2009-01-01T23:59:59.000Z

132

The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. VII. Classical Cepheids in the Small Magellanic Cloud  

E-Print Network (OSTI)

The seventh part of the OGLE-III Catalog of Variable Stars (OIII-CVS) consists of 4630 classical Cepheids in the Small Magellanic Cloud (SMC). The sample includes 2626 fundamental-mode (F), 1644 first-overtone (1O), 83 second-overtone (2O), 59 double-mode F/1O, 215 double-mode 1O/2O, and 3 triple-mode classical Cepheids. For each object basic parameters, multi-epoch VI photometry collected within 8 or 13 years of observations, and finding charts are provided in the OGLE Internet archive. We present objects of particular interest: exceptionally numerous sample of single-mode second-overtone pulsators, five double Cepheids, two Cepheids with eclipsing variations superimposed on the pulsation light curves. At least 139 first-overtone Cepheids exhibit low-amplitude secondary variations with periods in the range 0.60-0.65 of the primary ones. These stars populate three distinct sequences in the Petersen diagram. The origin of this secondary modulation is still unknown. Contrary to the Large Magellanic Cloud (LMC) ...

Soszynski, I; Udalski, A; Szymanski, M K; Kubiak, M; Pietrzynski, G; Wyrzykowski, L; Szewczyk, O; Ulaczyk, K

2010-01-01T23:59:59.000Z

133

Facult des arts et des sciences Service d'appui la formation interdisciplinaire  

E-Print Network (OSTI)

.desi.umontreal.ca/ 117573 Administration des systèmes informatiques 117574 Multimédia LINGUISTIQUE ET TRADUCTION 118010 Bac. en linguistique 4 juin à 10h00 3200 Jean Brillant B4325 www.ling.umontreal.ca/ 118020 Majeure en linguistique 118040 Mineure en linguistique 114715 Bac. litt. langue françaiselinguistique

Charette, André

134

Des apprentis pour le traitement automatique des langues Mmoire prsent pour l'obtention de l'  

E-Print Network (OSTI)

2.1.2 L'analogie en linguistique . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57 2'analyse linguistique 133 A.0.6 Segmentation et prétraitements ; ­ frontière entre analyse linguistique d'une part et analyse de données linguistiques, qui recouvrent des

Yvon, François

135

COMPARAISON DU RAYONNEMENT DES ISOTOPES RADIOACTIFS DES TERRES RARES FORMS DANS L'URANIUM ET LE THORIUM  

E-Print Network (OSTI)

COMPARAISON DU RAYONNEMENT DES ISOTOPES RADIOACTIFS DES TERRES RARES FORM?S DANS L'URANIUM ET LE semblables au lanthane, extraits de l'uranium ou du thorium irradié par les neutrons. Dans les limites dV. On sait que les noyaux d'uranium et de thorium irradiés par les neutrons peuvent subir une explosion qui

Paris-Sud XI, Université de

136

SURVEYING THE AGENTS OF GALAXY EVOLUTION IN THE TIDALLY STRIPPED, LOW METALLICITY SMALL MAGELLANIC CLOUD (SAGE-SMC). II. COOL EVOLVED STARS  

SciTech Connect

We investigate the infrared (IR) properties of cool, evolved stars in the Small Magellanic Cloud (SMC), including the red giant branch (RGB) stars and the dust-producing red supergiant (RSG) and asymptotic giant branch (AGB) stars using observations from the Spitzer Space Telescope Legacy program entitled 'Surveying the Agents of Galaxy Evolution in the Tidally Stripped, Low Metallicity SMC', or SAGE-SMC. The survey includes, for the first time, full spatial coverage of the SMC bar, wing, and tail regions at IR wavelengths (3.6-160 {mu}m). We identify evolved stars using a combination of near-IR and mid-IR photometry and point out a new feature in the mid-IR color-magnitude diagram that may be due to particularly dusty O-rich AGB stars. We find that the RSG and AGB stars each contribute {approx}20% of the global SMC flux (extended + point-source) at 3.6 {mu}m, which emphasizes the importance of both stellar types to the integrated flux of distant metal-poor galaxies. The equivalent SAGE survey of the higher-metallicity Large Magellanic Cloud (SAGE-LMC) allows us to explore the influence of metallicity on dust production. We find that the SMC RSG stars are less likely to produce a large amount of dust (as indicated by the [3.6] - [8] color). There is a higher fraction of carbon-rich stars in the SMC, and these stars appear to reach colors as red as their LMC counterparts, indicating that C-rich dust forms efficiently in both galaxies. A preliminary estimate of the dust production in AGB and RSG stars reveals that the extreme C-rich AGB stars dominate the dust input in both galaxies, and that the O-rich stars may play a larger role in the LMC than in the SMC.

Boyer, Martha L.; Meixner, Margaret; Gordon, Karl D.; Shiao, Bernie [STScI, Baltimore, MD 21218 (United States); Srinivasan, Sundar [Institut d'Astrophysique de Paris, CNRS UPR 341, Paris F-75014 (France); Van Loon, Jacco Th. [Astrophysics Group, Lennard-Jones Laboratories, Keele University, Staffordshire ST5 5BG (United Kingdom); McDonald, Iain; Kemper, F. [Jodrell Bank Centre for Astrophysics, University of Manchester, M13 9PL (United Kingdom); Zaritsky, Dennis; Block, Miwa; Engelbracht, Charles W.; Misselt, Karl [Steward Observatory, University of Arizona, Tucson, AZ 85721 (United States); Babler, Brian; Bracker, Steve; Meade, Marilyn; Whitney, Barbara [Department of Astronomy, University of Wisconsin, Madison, Madison, WI 53706-1582 (United States); Hora, Joe; Robitaille, Thomas [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138-1516 (United States); Indebetouw, Remy [Department of Astronomy, University of Virginia, Charlottesville, VA 22903-0818 (United States); Sewilo, Marta, E-mail: mboyer@stsci.edu [Department of Physics and Astronomy, The Johns Hopkins University, Homewood Campus, Baltimore, MD 21218 (United States)

2011-10-15T23:59:59.000Z

137

tude des Vitesses Fondamentales des Flammes Laminaires Prmlanges: Application aux Mlanges Mthane/Air et Syngas (H2/CO)/Air.  

E-Print Network (OSTI)

??Cette tude est consacre l'laboration d'une mthodologie de dtermination des vitesses fondamentales des flammes laminaires, en utilisant un diagnostic de Vlocimtrie par Imagerie de (more)

Bouvet, Nicolas

2009-01-01T23:59:59.000Z

138

Facult des arts et des sciences Service d'appui la formation interdisciplinaire  

E-Print Network (OSTI)

.desi.umontreal.ca/1-175-7-3 Administration des systèmes informatiques 1-175-7-4 Multimédia LINGUISTIQUE ET TRADUCTION 1-180-1-0 Bac. en linguistique 5 juin à 10h00 3200 Jean- Brillant B-3280 www.ling.umontreal.ca/ 1-180-2-0 Majeure en linguistique 1-180-4-0 Mineure en linguistique 1-147-1-5 Bac. litt. langue française-linguistique

Parrott, Lael

139

Fermilab Today | Experiment Profiles Archive | DES & DECam  

NLE Websites -- All DOE Office Websites (Extended Search)

DES and DECam DES and DECam photo FACT SHEET: Click here to download PDF. NAME: The Dark Energy Survey, or DES, which uses the Dark Energy Camera, called DECam WHAT WILL THIS TELL US? Because gravity causes mass to attract other mass, over time, this gravitational pull should slow the universe's expansion. Instead, the universe is accelerating: Galaxies are speeding away from each other faster and faster. DES aims to help pin down the cause of this acceleration. Theorists offer two possibilities: Either three-quarters of the universe is dark energy, which causes a type of anti-gravity, or gravity itself behaves differently on cosmic scales than Einstein thought it did. The answer will determine the fate of the universe. If Einstein was correct, the expansion of the universe will continue to speed up, and in

140

Modlisation, simulation et contrle des installations cryogniques du CERN  

E-Print Network (OSTI)

Cette thse prsente le dveloppement d'un simulateur de processus cryogniques de grande taille appliqu aux installations cryogniques de l'acclrateur de particules LHC (Large Hadron Collider) au CERN (Organisation Europenne pour la Recherche Nuclaire). Ce simulateur est bas sur une approche de modlisation oriente objet o chaque quipement (changeur, turbine, compresseur, etc.) est reprsent partir d'un ensemble d'quations physiques algbro-diffrentielles. L'architecture de contrle du CERN est galement simule en intgrant le contrle ralis par des automates programmables (PLC) avec le systme de supervision. Ce simulateur t dvelopp pour servir diffrents desseins comme l'entranement des oprateurs, la vrification des programmes automates (virtual commissioning) et l'optimisation des stratgies de contrle. Le systme cryognique d'un dtecteur de particules (CMS) a d'abord t simul pour valider les modles, puis un liqufacteur d'...

Bradu, Benjamin; Gayet, P

2010-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


141

Einfhrungsveranstaltung des Instituts fr Chemie zum Wintersemester 2013/2014  

E-Print Network (OSTI)

Einführungsveranstaltung des Instituts für Chemie zum Wintersemester 2013/2014 Donnerstag, 10.10.2013 Albert-Einstein-Str. 3a, August Michaelis Hörsaal 09.00 Uhr Hörsaalgebäude Chemie, Albert Einstein-Str. 3a/ Hörsaal 101 Begrü?ung der Studenten des Bachelor-Studienganges Chemie und der Lehramtskandidaten

Wolkenhauer, Olaf

142

Einfhrungsveranstaltung des Instituts fr Chemie zum Wintersemester 2012/2013  

E-Print Network (OSTI)

Einführungsveranstaltung des Instituts für Chemie zum Wintersemester 2012/2013 Donnerstag, 11.10.2012 Albert-Einstein-Str. 3a, August Michaelis Hörsaal 09.00 Uhr Hörsaalgebäude Chemie, Albert Einstein-Str. 3a/ Hörsaal 101 Begrü?ung der Studenten des Bachelor-Studienganges Chemie und der Lehramtskandidaten

Wolkenhauer, Olaf

143

es recherches sur les capacits linguistiques des nourrissons ont  

E-Print Network (OSTI)

Médecine & enfance L es recherches sur les capacités linguistiques des nourrissons ont été lancées linguistiques pré- coces [1]. Ces auteurs ont ainsi constaté que les nourrissons de un et trois mois étaient'identification correcte, en fonction de l'âge et de l'expérience linguistique des sujets, de deux contrastes phonémiques

Dehaene-Lambertz, Ghislaine

144

DES modelling and control vs. problem solving methods  

Science Conference Proceedings (OSTI)

Modelling and control of a kind of Discrete-Event Systems (DES) having a character of Flexible Manufacturing Systems (FMS) are examined by means of methods used in applied artificial intelligence. While assembly and/or disassembly ... Keywords: DES modelling, FMS control, PNs, Petri nets, agent-based systems, artificial intelligence, control agents, decision making, discrete event systems, flexible manufacturing systems, intelligent information, multi-agent systems, ontology, problem solving, reachability graphs, vehicle crossroads

Frantisek Capkovic

2007-04-01T23:59:59.000Z

145

Tables des principaux minerais d'uranium et de thorium  

E-Print Network (OSTI)

233 Tables des principaux minerais d'uranium et de thorium Par B. SZILARD [Faculté des Sciences de minerais d'uranium et de thorium avec leurs données les plus importantes, telles que la com- position, la teneur en uranium et en thorium, la provenance et quelques indications générales. La liste ne prétend pas

Paris-Sud XI, Université de

146

The Des Plaines River -- Part One  

NLE Websites -- All DOE Office Websites (Extended Search)

One One Nature Bulletin No. 606 May 28, 1960 Forest Preserve District of Cook County Daniel Ryan, President Roberts Mann, Conservation Editor David H. Thompson, Senior Naturalist THE DES PLAINES RIVER -- PART ONE: DESCRIPTION Chicago was incorporated as a village in 1833 and in less than 100 years it had become one of the world's great cities. Four unique natural features have contributed to its phenomenal growth. The first is Lake Michigan. Chicago is strategically located at the south end of it, deep in the heart of the continent and the vast central lowland -- bread-basket of our nation. The lake provides an inexhaustible supply of fresh water and a highway for water-borne commerce. Since the completion of the St. Lawrence Seaway, Chicago has also become a port for ocean going ships.

147

Refroidissement seculaire de la Terre solide, emergence des continents, et evolution des enveloppes externes de la Terre.  

E-Print Network (OSTI)

??Le refroidissement seculaire du manteau terrestre et de la lithosphere continentale se traduit par l'augmentation de la surface de terres emergees. L'augmentation corollaire des processus (more)

Flament, Nicolas

2009-01-01T23:59:59.000Z

148

PROPAGATION DES ONDES LASTIQUES DE SURFACE Atlas des configurations calcules pour le quartz, le tantalate de lithium,  

E-Print Network (OSTI)

, le tantalate de lithium, le niobate de lithium et le vanado-sulfure de thallium en ce qui concerne'ensemble des configurations possibles des matériaux classiques (quartz, niobate de lithium et tantalate de lithium) ainsi que d'un matériau récemment signalé le vanado-sulfure de thallium (Tl3VS4). La propagation

Paris-Sud XI, Université de

149

Guide l'intention des tudiants internationaux dition 2011-2012  

E-Print Network (OSTI)

3200, rue Jean-Brillant) ainsi que dans certains comptoirs-satellites (pavillon Jean-Coutu, pavillon Postes Canada 2122, chemin de la Côte-des-Neiges 6605, chemin de la Côte-des-Neiges Jean Coutu

Charette, André

150

Nano-antennes optiques pour l'inspection des structures photoniques.  

E-Print Network (OSTI)

??L'objectif de cette thse est de concevoir et laborer des outils innovants, baptiss nano-antennes (NAs), pour sonder le champ lectromagntique optique au voisinage des structures (more)

Abdoulkader Ibrahim, Idriss

2010-01-01T23:59:59.000Z

151

THE MASS LOSS RETURN FROM EVOLVED STARS TO THE LARGE MAGELLANIC CLOUD: EMPIRICAL RELATIONS FOR EXCESS EMISSION AT 8 AND 24 {mu}m  

SciTech Connect

We present empirical relations describing excess emission from evolved stars in the Large Magellanic Cloud (LMC) using data from the Spitzer Space Telescope Surveying the Agents of a Galaxy's Evolution (SAGE) survey which includes the Infrared Array Camera (IRAC) 3.6, 4.5, 5.8, and 8.0 {mu}m and Multiband Imaging Photometer (MIPS) 24, 70, and 160 {mu}m bands. We combine the SAGE data with the Two Micron All Sky Survey (2MASS; J, H, and K {sub s}) and the optical Magellanic Cloud Photometric Survey (MCPS; U, B, V, and I) point source catalogs in order to create complete spectral energy distributions (SEDs) of the asymptotic giant branch (AGB) star candidates in the LMC. AGB star outflows are among the main producers of dust in a galaxy, and this mass loss results in an excess in the fluxes observed in the 8 and 24 {mu}m bands. The aim of this work is to investigate the mass loss return by AGB stars to the interstellar medium of the LMC by studying the dependence of the infrared excess flux on the total luminosity. We identify oxygen-rich, carbon-rich, and extreme AGB star populations in our sample based on their 2MASS and IRAC colors. The SEDs of oxygen- and carbon-rich AGB stars are compared with appropriate stellar photosphere models to obtain the excess flux in all the IRAC bands and the MIPS 24 {mu}m band. Extreme AGB stars are dominated by circumstellar emission at 8 and 24 {mu}m; thus we approximate their excesses with the flux observed in these bands. We find about 16,000 O-rich, 6300 C-rich, and 1000 extreme sources with reliable 8 {mu}m excesses, and about 4500 O-rich, 5300 C-rich, and 960 extreme sources with reliable 24 {mu}m excesses. The excesses are in the range 0.1 mJy to 5 Jy. The 8 and 24 {mu}m excesses for all three types of AGB candidates show a general increasing trend with luminosity. The color temperature of the circumstellar dust derived from the ratio of the 8 and 24 {mu}m excesses decreases with an increase in excess, while the 24 {mu}m optical depth increases with excess. The extreme AGB candidates are the major contributors to the mass loss, and we estimate the total AGB mass loss return to the LMC to be (5.9-13) x 10{sup -3} M {sub sun} yr{sup -1}.

Srinivasan, Sundar [Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218 (United States); Meixner, Margaret; Leitherer, Claus; Vijh, Uma; Gordon, Karl D.; Sewilo, Marta [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Volk, Kevin [Gemini Observatory, 670 North A'ohoku Place, Hilo, HI 96720 (United States); Blum, Robert D.; Harris, Jason [National Optical Astronomy Observatory, P.O. Box 26732, Tucson, AZ 85726-6732 (United States); Babler, Brian L.; Bracker, Steve; Meade, Marilyn [Department of Astronomy, University of Wisconsin, 475 North Charter Street, Madison, WI 53706 (United States); Block, Miwa; Engelbracht, Charles W.; For, Bi-Qing; Misselt, Karl A. [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Cohen, Martin [Radio Astronomy Laboratory, 601 Campbell Hall, University of California, Berkeley, CA 94720 (United States); Hora, Joseph L. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Indebetouw, Remy [Astronomy Department, University of Virginia, P.O. Box 3818, Charlottesville, VA 22903-0818 (United States); Markwick-Kemper, Francisca [Jodrell Bank Centre of Astrophysics, School of Physics and Astronomy, University of Manchester, Manchester M13 9PL (United Kingdom)], E-mail: sundar@pha.jhu.edu (and others)

2009-06-15T23:59:59.000Z

152

Animation de mod`eles UML -Application dans le contexte des Smartgrids  

E-Print Network (OSTI)

Animation de mod`eles UML - Application dans le contexte des Smartgrids Rachida Seghiri T'arriv´ee des Smartgrids dans le domaine ´electrique apporte de profonds changements au sein des Syst`emes d, nous ´etayons cet ´etat de l'art par la simulation d'un cas m´etier illustratif des Smartgrids en

153

Le CLV, c'est...... L'intgration linguistique et culturelle des tu-  

E-Print Network (OSTI)

Le CLV, c'est...... L'intégration linguistique et culturelle des étu- diants et chercheurs non Vivantes organise des for- mations linguistiques à l'attention du personnel de l'université Ateliers'allemand. Le CLV, c'est...... La certification des connaissances linguistiques ! Le Centre de Langues Vivantes

Glineur, François

154

Mise en correspondance par correlation avec prise en compte des occultations  

E-Print Network (OSTI)

Mise en correspondance par corr´elation avec prise en compte des occultations Occlusions handling cours de l'appariement, provient des occultations. C'est pourquoi le second objectif est de pr compte le probl`eme des occultations. Les r´esultats mettent en ´evidence la meilleure m´ethode qui

Chambon, Sylvie

155

UTILISATION D'UNE EXPRIENCE DE RSONANCE LECTRIQUE. RADIOFRQUENCE SUR DES NIVEAUX EXCITS DANS UN FAISCEAU  

E-Print Network (OSTI)

structures fines ou hyperfines des atomes hydro- génoïdes légers car les séparations entre niveaux sont alors détection optique d'une résonance électrique entre niveaux hydro- génoïdes sur un faisceau d'ions excités

Lombardi, Maurice

156

The effect of metallicity on the Cepheid Period-Luminosity relation from a Baade-Wesselink analysis of Cepheids in the Galaxy and in the Small Magellanic Cloud  

E-Print Network (OSTI)

(ABRIDGED) We have applied the near-IR Barnes-Evans realization of the Baade-Wesselink method as calibrated by Fouque & Gieren (1997) to five metal-poor Cepheids with periods between 13 and 17 days in the Small Magellanic Cloud as well as to a sample of 34 Galactic Cepheids to determine the effect of metallicity on the period-luminosity (P-L) relation. For ten of the Galactic Cepheids we present new accurate and well sampled radial-velocity curves. The Baade-Wesselink analysis provides accurate individual distances and luminosities to the Cepheids in the two samples, allowing us to constrain directly, in a purely differential way, the metallicity effect on the Cepheid P-L relation. For the Galactic Cepheids we provide a new set of P-L relations which have zero-points in excellent agreement with astrometric and interferometric determinations. These relations can be used directly for the determination of distances to solar-metallicity samples of Cepheids in distant galaxies, circumventing any corrections for metallicity effects on the zero-point and slope of the P-L relation. We find evidence for both such metallicity effects in our data. Comparing our two samples of Cepheids at a mean period of about 15 days, we find a weak effect of metallicity on the luminosity similar to that adopted by the HST Key Project on the Extragalactic Distance Scale.

Jesper Storm; Bruce W. Carney; Wolfgang P. Gieren; Pascal Fouque; David W. Latham; Anne M. Fry

2004-01-12T23:59:59.000Z

157

The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. III. RR Lyrae Stars in the Large Magellanic Cloud  

E-Print Network (OSTI)

The third part of the OGLE-III Catalog of Variable Stars comprises 24906 RR Lyr stars in the Large Magellanic Cloud (LMC). This sample consist of 17693 fundamental-mode (RRab), 4958 first-overtone (RRc), 986 double-mode (RRd) and 1269 suspected second-overtone (RRe) pulsators. 66 objects are foreground Galactic RR Lyr stars. The catalog data include basic photometric and astrometric properties of the RR Lyr stars, multi-epoch VI photometry and finding charts. We detected one new RR Lyr star with additional eclipsing variations. The spatial distribution of RR Lyr stars in the LMC is distinctly non-spherical and it is elongated in the same direction as the LMC bar. The basic statistical features of RR Lyr stars in the LMC are provided. The apparent V-band magnitudes for RRab stars have the modal value at 19.36 mag, and for overtone RR Lyr stars it is about 19.32 mag. The mean periods for RRab, RRc and RRe stars are 0.576, 0.337 and 0.270 days, respectively.

Soszynski, I; Szymanski, M K; Kubiak, M; Pietrzynski, G; Wyrzykowski, L; Szewczyk, O; Ulaczyk, K; Poleski, R

2009-01-01T23:59:59.000Z

158

The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. IX. RR Lyrae Stars in the Small Magellanic Cloud  

E-Print Network (OSTI)

The ninth part of the OGLE-III Catalog of Variable Stars (OIII-CVS) comprises RR Lyrae stars in the Small Magellanic Cloud (SMC). Our sample consists of 2475 variables, of which 1933 pulsate in the fundamental mode (RRab), 175 are the first overtone pulsators (RRc), 258 oscillate simultaneously in both modes (RRd) and 109 stars are suspected second-overtone pulsators (RRe). 30 objects are Galactic RR Lyr stars seen in the foreground of the SMC. We discuss some statistical features of the sample. Period distributions show distinct differences between SMC and LMC populations of RR Lyr variables, with the SMC stars having on average longer periods. The mean periods for RRab, RRc and RRe stars are 0.596, 0.366 and 0.293 days, respectively. The mean apparent magnitudes of RRab stars are equal to 19.70 mag in the V band and 19.12 mag in the I band. Spatial distribution of RR Lyr stars shows that the halo of the SMC is roughly round in the sky, however the density map reveals two maxima near the center of the SMC. F...

Soszynski, I; Szymanski, M K; Kubiak, M; Pietrzynski, G; Wyrzykowski, L; Ulaczyk, K; Poleski, R

2010-01-01T23:59:59.000Z

159

Ocean Energy Company LLC | Open Energy Information  

Open Energy Info (EERE)

Ocean Energy Company LLC Address 505 Fifth Ave 800 Place Des Moines Zip 50309-2426 Sector Marine and Hydrokinetic Year founded 2011 Phone number (515) 246-1500 Region United States...

160

IOWA ARMY EPA Region 7 04/02/2012 City: Middletown  

E-Print Network (OSTI)

IOWA ARMY EPA Region 7 04/02/2012 City: Middletown AMMUNITION PLANT County: Des Moines County IOWA, and pack a variety of conventional ammunition and fusing systems for the Department of Defense. The Atomic

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


161

Forum des Jeuns du Gabon | Open Energy Information  

Open Energy Info (EERE)

des Jeuns du Gabon des Jeuns du Gabon Jump to: navigation, search Name Forum des Jeuns du Gabon Address Libreville-GABON, derrirère la Cité Damas Place Gabon Coordinates 0.390841°, 9.453644° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":0.390841,"lon":9.453644,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

162

Des Plaines, Illinois: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Des Plaines, Illinois: Energy Resources Des Plaines, Illinois: Energy Resources (Redirected from Des Plaines, IL) Jump to: navigation, search Equivalent URI DBpedia Coordinates 42.0333623°, -87.8833991° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":42.0333623,"lon":-87.8833991,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

163

Ein Modell der Produktionsspitze des Erdols: Stephen Keeling*  

E-Print Network (OSTI)

Ein Modell der Produktionsspitze des Erd¨ols: Peak Oil Stephen Keeling* 1 Die Problemstellung Die man einen Peak von Erd¨olentdeckung im Jahr 1965 und einen Peak von Erd¨olf¨orderung im Jahr 2006. W

Keeling, Stephen L.

164

XMM-Newton observations of the Small Magellanic Cloud: X-ray outburst of the 6.85 s pulsar XTE J0103-728  

E-Print Network (OSTI)

A bright X-ray transient was seen during an XMM-Newton observation in the direction of the Small Magellanic Cloud (SMC) in October 2006. The EPIC data allow us to accurately locate the source and to investigate its temporal and spectral behaviour. X-ray spectra covering 0.2-10 keV and pulse profiles in different energy bands were extracted from the EPIC data. The detection of 6.85 s pulsations in the EPIC-PN data unambiguously identifies the transient with XTE J0103-728, discovered as 6.85 s pulsar by RXTE. The X-ray light curve during the XMM-Newton observation shows flaring activity of the source with intensity changes by a factor of two within 10 minutes. Modelling of pulse-phase averaged spectra with a simple absorbed power-law indicates systematic residuals which can be accounted for by a second emission component. For models implying blackbody emission, thermal plasma emission or emission from the accretion disk (disk-blackbody), the latter yields physically sensible parameters. The photon index of the power-law of ~0.4 indicates a relatively hard spectrum. The 0.2-10 keV luminosity was 2x10^{37} with a contribution of ~3% from the disk-blackbody component. A likely origin for the excess emission is reprocessing of hard X-rays from the neutron star by optically thick material near the inner edge of an accretion disk. From a timing analysis we determine the pulse period to 6.85401(1) s indicating an average spin-down of ~0.0017 s per year since the discovery of XTE J0103-728 in May 2003. The X-ray properties and the identification with a Be star confirm XTE J0103-728 as Be/X-ray binary transient in the SMC.

F. Haberl; W. Pietsch

2008-01-30T23:59:59.000Z

165

Congrs des innovations mcaniques CIM'08 28-29 avril 2008 Sousse Tunisie. Dmarche d'intgration des connaissances  

E-Print Network (OSTI)

1er Congrès des innovations mécaniques CIM'08 ­ 28-29 avril 2008 Sousse ­ Tunisie. Démarche d2009 Author manuscript, published in "CIM'08, Sousse : Tunisia (2008)" #12;CIM'08 ­ 28-29 avril 2008

Paris-Sud XI, Université de

166

Ensembles de niveaux robustes au speckle et recalage B-spline: application la segmentation et l'analyse du mouvement cardiaque par des images ultrasons.  

E-Print Network (OSTI)

??L'analyse du mouvement local des parois du cur dans des images ultrasonores est souvent utilise pour diagnostiquer certaines malformations cardiaques. Malheureusement, cette modalit produit des (more)

Mora Cofre, Marco Antonio

2008-01-01T23:59:59.000Z

167

Nano-antennes optiques pour l'exaltation et le contrle de la fluorescence molculaire dans des volumes sub-longueur d'onde.  

E-Print Network (OSTI)

??Les nano-antennes optiques permettent la manipulation, le confinement et l'exaltation des champs lectromagntiques dans des volumes sub-longueur d'onde. Les applications de ces nano-objets concernent des (more)

Aouani, Heykel

2011-01-01T23:59:59.000Z

168

Effet chez le porcelet dune exposition un rgime co-contamin en mycotoxines, et apprciation des stratgies de lutte.  

E-Print Network (OSTI)

??Les mycotoxines sont des mtabolites secondaires des moisissures qui peuvent naturellement contaminer de nombreuses denres alimentaires, notamment les crales. Dans les travaux de thse, nous (more)

Grenier, Bertrand

2011-01-01T23:59:59.000Z

169

Ce dernier potentiel d'ionisation peut servir au calcul des moments magntiques nuclaires du plutonium,  

E-Print Network (OSTI)

plutonium, mais nous avons constaté par la suite, qu'un facteur 2 a été omis dans notre calcul du nombre valeurs probables des moments magnétiques nucléaires sont : y(239Pu) = 0,175 + 0,040 magnétons nucléaires y(241Pu) = 0,62 ± 0,15 » » L'incertitude des résultats provient principalemenl des mesures de la

Paris-Sud XI, Université de

170

La temporalit linguistique : circonscrire un objet d'analyse ainsi que des finalits cette analyse.  

E-Print Network (OSTI)

??De quoi parle-t-on quand on propose de traiter (de) la temporalit dans les textes ? Dans le paradigme applicatif du Traitement Automatique des Langues, on (more)

Battistelli, Delphine

2009-01-01T23:59:59.000Z

171

Politique linguistique du franais relev des sites de promotion enjeux traductifs.  

E-Print Network (OSTI)

??Ce travail dresse un relev des sites francophones d'appui la terminologie et la traduction et inscrit cette problmatique dans le contexte plus vaste (more)

Barros, Cristina Pinto de

2011-01-01T23:59:59.000Z

172

Steigerung des Wirkungsgrads und der Ausnutzung von Norm-Asynchronmotoren mit Kurzschlusskfig.  

E-Print Network (OSTI)

??Die allgemeine Energiesituation am Ende des 20. Jahrhunderts zwingt die Menschheit zum bewussteren Umgang mit der Energie. Weiterhin sorgt ein weltweites Umdenken in der Umweltpolitik (more)

Knopik, Thomas

2012-01-01T23:59:59.000Z

173

Comportement au jeune ge des matriaux cimentaires Caractrisation et modlisation chimio-hydro-mcanique du retrait.  

E-Print Network (OSTI)

??Le comportement au jeune ge des matriaux matrice cimentaire est un phnomne complexe qui met en opposition une structure volutive, mais encore faible mcaniquement (more)

Haouas, Adnan

2007-01-01T23:59:59.000Z

174

Publications et confrences invites Articles dans des revues avec comit de lecture  

E-Print Network (OSTI)

Drouilhet a été riche et singulier. Je me dois de remercier l'ensemble des personnes qui m'ont permis de

Habegger, Nathan

175

Th'eorie des nombres/Number Theory AN ESTIMATE FOR THE MULTIPLICITY OF BINARY RECURRENCES  

E-Print Network (OSTI)

'eg'ee Dans l'article [7] H.-P. Schlickewei donne une majoration, indep'endante du c* *orps des nom- bres, de

176

UNIVERSITE D'ANGERS Anne 2005 ESTIMATION DES LOIS DE FIABILITE EN MECANIQUE  

E-Print Network (OSTI)

], [EIREDA, 1998], [MIL-HDBK-217 F, 1995] etc.) A partir des retours garanties. Cette méthode permet d

Paris-Sud XI, Université de

177

Synthse et ractivit des disilanes : applications vers la synthse de la 10-silatestostrone.  

E-Print Network (OSTI)

??Les travaux rapports dans ce mmoire concernent la synthse et la ractivit des disilanes, en vue de leur application vers la synthse de la 10-silatestostrone. (more)

Giros, Audrey

2012-01-01T23:59:59.000Z

178

GLOBULAR CLUSTER ABUNDANCES FROM HIGH-RESOLUTION, INTEGRATED-LIGHT SPECTROSCOPY. IV. THE LARGE MAGELLANIC CLOUD: {alpha}, Fe-PEAK, LIGHT, AND HEAVY ELEMENTS  

SciTech Connect

We present detailed chemical abundances in eight clusters in the Large Magellanic Cloud (LMC). We measure abundances of 22 elements for clusters spanning a range in age of 0.05-12 Gyr, providing a comprehensive picture of the chemical enrichment and star formation history of the LMC. The abundances were obtained from individual absorption lines using a new method for analysis of high-resolution (R {approx} 25,000), integrated-light (IL) spectra of star clusters. This method was developed and presented in Papers I, II, and III of this series. In this paper, we develop an additional IL {chi}{sup 2}-minimization spectral synthesis technique to facilitate measurement of weak ({approx}15 mA) spectral lines and abundances in low signal-to-noise ratio data (S/N {approx} 30). Additionally, we supplement the IL abundance measurements with detailed abundances that we measure for individual stars in the youngest clusters (age < 2 Gyr) in our sample. In both the IL and stellar abundances we find evolution of [{alpha}/Fe] with [Fe/H] and age. Fe-peak abundance ratios are similar to those in the Milky Way (MW), with the exception of [Cu/Fe] and [Mn/Fe], which are sub-solar at high metallicities. The heavy elements Ba, La, Nd, Sm, and Eu are significantly enhanced in the youngest clusters. Also, the heavy to light s-process ratio is elevated relative to the MW ([Ba/Y] >+0.5) and increases with decreasing age, indicating a strong contribution of low-metallicity asymptotic giant branch star ejecta to the interstellar medium throughout the later history of the LMC. We also find a correlation of IL Na and Al abundances with cluster mass in the sense that more massive, older clusters are enriched in the light elements Na and Al with respect to Fe, which implies that these clusters harbor star-to-star abundance variations as is common in the MW. Lower mass, intermediate-age, and young clusters have Na and Al abundances that are lower and more consistent with LMC field stars. Our results can be used to constrain both future chemical evolution models for the LMC and theories of globular cluster formation.

Colucci, Janet E.; Bernstein, Rebecca A. [Department of Astronomy and Astrophysics, UCO/Lick Observatory, University of California, 1156 High Street, Santa Cruz, CA 95064 (United States); Cameron, Scott A. [Science Department, 3000 College Heights Blvd., Cerro Coso Community College, Ridgecrest, CA 93555 (United States); McWilliam, Andrew, E-mail: jcolucci@ucolick.org, E-mail: rab@ucolick.org, E-mail: scameron@cerrocoso.edu, E-mail: andy@ociw.edu [The Observatories of the Carnegie Institute of Washington, 813 Santa Barbara Street, Pasadena, CA 91101-1292 (United States)

2012-02-10T23:59:59.000Z

179

pour obtenir le diplme d'Habilitation Diriger des Recherches  

E-Print Network (OSTI)

, 81, 93 BR Breeding Ratio, taux de régénération : 47, 110 CANDU CANada Deuterium Uranium, réacteur oxyde de thorium . . . . . . . . . 15 1.2.2 Guides utiles à l'étude du cycle thorium en CANDU et en REP et modélisation des réacteurs étudiés . . . . . . . . . . . . . . . . . . . . 29 2.2.1 Le CANDU-6

180

La problmatique des dchets nuclaires Mmoire prsent au BAPE dans le cadre du projet de modification des  

E-Print Network (OSTI)

les réacteurs au Canada sont de type CANDU-PHWR modérés à l'eau lourde, alors que la majorité des'eau lourde, les réacteurs CANDU peuvent utiliser l'uranium naturel comme combustible. L'uranium naturel CANDU 15 GW 7,5 1760 t 1760 t LWR 335 GW 35 8400 t 58100 t* Total 350 GW - 10169 t 59820 t * incluant 50

Meunier, Michel

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


181

Recherche du boson de Higgs du Modle Standard dans le canal de dsintgration ZH->nu nu bb sur le collisionneur Tevatron dans l'exprience D0. Dveloppement d'une mthode d'tiquetage des jets de quark b avec des muons de basses impulsions transverses.  

E-Print Network (OSTI)

??Dans le Modle Standard de la physiques des particules, le boson de Higgs permet de gnrer la masse des particules lmentaires. Les contraintes thoriques et (more)

Jamin, D.

2010-01-01T23:59:59.000Z

182

Laboratoire Langues, Littratures, Linguistique des Universits d'Angers et du Maine (3L.AM) -  

E-Print Network (OSTI)

Laboratoire Langues, Littératures, Linguistique des Universités d'Angers et du Maine (3L.AM) - EA n Laboratoire Langues, Littératures, Linguistique des universités d'Angers et du Maine (Labo 3L.AM), ?quipe d

Di Girolami, Cristina

183

Universit d'Avignon et des Pays de Vaucluse Institut National de la Recherche Agronomique  

E-Print Network (OSTI)

'objet et un champ incident connu dont la direction de propagation et la fréquence peuvent varier. La the interaction between the unknown object and a known incident field whose propagation direction and frequency position r, de l'incidence inc et de la fréquence. Pour des raisons de lisibilité des équations, on les

Paris-Sud XI, Université de

184

Diffusion des rsultats de la recherche : une nouvelle donne numrique ? GOOGLE SCHOLAR, GOOGLE PRINT...  

E-Print Network (OSTI)

Diffusion des résultats de la recherche : une nouvelle donne numérique ? GOOGLE SCHOLAR, GOOGLE.» (GAR 05) 72 % des universitaires utilisent le moteur Google pour leurs recherches d'articles scientifiques (SWA 05). L'INIST, premier fournisseur français de documents de recherche a fait de Google Scholar

Paris-Sud XI, Université de

185

Cycle thorium et racteurs sel fondu. Exploration du champ des paramtres et des contraintes dfinissant le "Thorium Molten Salt Reactor".  

E-Print Network (OSTI)

??Le recours l'nergie lectronuclaire pour diminuer les missions anthropiques de CO2 ncessite des avances technologiques majeures. Les racteurs nuclaires de IVe gnration doivent rpondre (more)

Mathieu, Ludovic

186

Intgration du comportement thermomcanique des pices dans l'analyse des spcifications gomtriques : application une turbine de moteur d'hlicoptre.  

E-Print Network (OSTI)

??La performance d'un moteur d'hlicoptre est fortement corrle la performance de la turbine haute pression, et plus particulirement l'influence des diffrents composants constitutifs. (more)

Pierre, Laurent

187

Modlisation du comportement des neutrons dans un racteur avanc canadien ACR en utilisant les logiciels dvelopps  

E-Print Network (OSTI)

Limited (AECL), portant sur la mise au point de logiciels et de schémas de calcul pour le Advanced Candu des ACR est différente de celle des réacteurs CANDU actuels. La présence simultanée d'eau légère et d des réacteurs CANDU actuels devra être modifiée et améliorée avant de s'adapter au ACR. Nous devrons

Meunier, Michel

188

des vnements 2013-2014 de l'universit de rennes 1  

E-Print Network (OSTI)

Aire française (foire du diY et du bidouillage) à l'occasion des 20 ans de l'iut de saint-malo Vendredi 11 et

Rennes, Université de

189

Comptences linguistiques et cognitives des enfants bilingues en situation linguistique minoritaire.  

E-Print Network (OSTI)

??Au Canada, lvaluation langagire des enfants franco-ontariens savre une tche complexe pour les orthophonistes en raison dune carence doutils et de normes rgionales. Le problme (more)

Mayer-Crittenden, Chantal E.

2013-01-01T23:59:59.000Z

190

How to Protect DES Against Exhaustive Key Search (an Analysis of ...  

Science Conference Proceedings (OSTI)

Jan 1, 2001 ... The block cipher \\DESX is defined by \\DESX k.k1.k2 (x) = k2\\xor \\DES k (k1\\xor x) , where \\xor denotes bitwise exclusive-or. This construction...

191

UNIVERSIT TOULOUSE III -PAUL SABATIER ECOLE DOCTORALE DES SCIENCES DE L'UNIVERS,  

E-Print Network (OSTI)

constructifs avec Jean Pailleux, Florence Rabier, Gérald Desroziers, Loïk Berre et Bernard Chapnik, qui m'ont Belo-Pereira et Simona ¸Stefanescu concernant la construction des statistiques et Radmila Brozkova pour

192

Verbesserung der medizinischen Versorgung und des Outcomes sehr kleiner und leichter Frhgeborener durch klinisches Benchmarking.  

E-Print Network (OSTI)

??In der vorliegenden Arbeit wurde anhand der im Rahmen des Vermont-Oxford-Neonatal-Networks erhobenen Daten an der Berliner Klinik fr Neonatologie der Charit Campus Mitte und der (more)

Btzel, Carolin

2006-01-01T23:59:59.000Z

193

Etude de la distillation ractive dans une colonne avec un bac intermdiaire avec des ractions conscutives.  

E-Print Network (OSTI)

??La distillation ractive est lun des procds chimiques intensifis les plus reconnus, qui intgre la sparation et la raction au sein dun mme appareil. Les (more)

Lukacs, Timea

2009-01-01T23:59:59.000Z

194

Une g en eralisation des r esultats de Kreweras sur le polyn ... - CECM  

E-Print Network (OSTI)

Nous obtenons des g en eralisations de plusieurs r esultats de Kreweras [9]. ... notamment une r ecurrence v eri ee par ce polyn^ome et nous montrons que son ...

195

Une g en eralisation des r esultats de Kreweras sur le polyn ... - CECM  

E-Print Network (OSTI)

Nous obtenons des g en eralisations de plusieurs r esultats de. Kreweras [9]. Nous d emontrons notamment une r ecurrence v eri ee par ces polyn^omes et.

196

Mtrologie des supernovae de type Ia pour la cosmologie : instrumentation et analyse calorimtrique.  

E-Print Network (OSTI)

??L'utilisation des supernovae de type Ia comme indicateurs de distance est un pilier du modle de concordance actuel en cosmologie. Le travail d'instrumentation prsent dans (more)

Juramy, Claire

2006-01-01T23:59:59.000Z

197

Attraction d'ondes pour des systmes rsonance d'ondes contra-propagatives.  

E-Print Network (OSTI)

??L'attraction d'ondes dans des systmes contra-propagatifs est un phnomne gnral, tabli initialement en Physique dans le contexte de l'attraction de polarisation entre deux ondes contra-propagatives (more)

Grenier, Muriel

2011-01-01T23:59:59.000Z

198

Les micro-nanotechnologies pour les systmes hyperfrquences: au-del des conventions.  

E-Print Network (OSTI)

??L'volution de notre socit est spectaculaire. Les nouvelles technologies apportent sans cesse des bouleversements dans nos vies, dont nous n'avons d'ailleurs pas toujours conscience tellement (more)

Grenier, Katia

2010-01-01T23:59:59.000Z

199

LE SPECTRE POLLINIQUE DES MIELS DU QUBEC Marie-Jos FELLER-DEMALSY  

E-Print Network (OSTI)

, 1979, 10 (4), 313-340, La comparaison des deux séries d'analyses montre : - une augmentation de la suite à la publication « Analyse pollinique des miels du Québec (FELLER-DEMALSY et LAMONTAGNE 1979). Ce récoltés pour un tiers en 1977 et les deux tiers en 1978, pour la plupart par les services d'inspection du

Recanati, Catherine

200

Le TCL pour des produits alatoires d'automorphismes du tore, exemples dans le cas stationnaire.  

E-Print Network (OSTI)

Le TCL pour des produits aléatoires d'automorphismes du tore, exemples dans le cas stationnaire la mesure m vers N(0, 1). Nous présentons des situations où un TCL quenched peut être obtenu, en Introduction, la question du TCL quenched pour un système bré 3 2 Cas indépendant 4 2.1 Trou spectral

Frénod, Emmanuel

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


201

Un modle de commande pour le contrle des instabilits de combustion  

E-Print Network (OSTI)

Un modèle de commande pour le contrôle des instabilités de combustion Landau Ioan-Doré Bouziani pour l'instabilité de combustion. Ce système est analysé en utilisant la méthode de Krylov'analyse sont comparés avec des tests en simulation. Mots-clésmodélisation, instabilité de combustion, systèmes

Paris-Sud XI, Université de

202

A/s DES PONTS ET CHAUSSEES  

E-Print Network (OSTI)

HYDRAULIQUES DE MASSIFS ROCHEUX SIMULES PAR DES ASSEMBLAGES DE BLOCS RIGIDES. INTRODUCTION D'UN COUPLAGE HYDRO mécanique, hydraulique ou hydro-mécanique d'un massif rocheux, une importance particulière est accordée aux caractérisations de ses discontinuités car elles constituent, toujours, des zones de faiblesse du massif. L

Paris-Sud XI, Université de

203

niversit vire de fruxelles enne dmique pult des ienes eppliques PHHSEPHHT  

E-Print Network (OSTI)

plus trdD en IWUVD le premier stellite envoyé dns l9espeF in IWWRD le dernier stellite à devoir être de les dérypterF Principe ve système q est omposé de PR stellites en rottion utour de l terre de Fig. QFQ ! yrites des stellites du système qF PS : Sur cette gure, la représentation des orbites n

Libre de Bruxelles, Université

204

Diffusion thermique de l'uranium dans le zirconium. Application au stockage des gaines de combustible  

E-Print Network (OSTI)

Diffusion thermique de l'uranium dans le zirconium. Application au stockage des gaines de. De plus le dépôt d'énergie des produits de fission entraîne la pulvérisation de l'uranium et, au fur refroidis 5 ans, montrent que l'uranium et les actinides sont répartis uniformément dans la gaine. Nous

Paris-Sud XI, Université de

205

Sur le parcours des rayons 03B1 de l'uranium Par Lon BLOCH,  

E-Print Network (OSTI)

Sur le parcours des rayons 03B1 de l'uranium Par Léon BLOCH, Agrégé de l'Université de Paris parcours des rayons x de l'uranium a été dé- terminé par Bragg1 au moyen d'une méthode indirecte. Bragg a mesuré l'ionisatiol totale due au rayonnement de l'uranium lorsque la substance est recouverte d

Paris-Sud XI, Université de

206

Valorisation nergtique des dchets issus de la biomasse Dupuit Estellea, Dchomets Rolanda, Massiani Catherineb, Bourgois Jacquesa  

E-Print Network (OSTI)

Valorisation énergétique des déchets issus de la biomasse Dupuit Estellea, Déchomets Rolanda la biomasse et de ses déchets a été envisagée. Elle implique la sélection d'une aire géographique et'emplacement des sites de valorisation énergétique : ­ l'estimation de la quantité théorique disponible de biomasse

Paris-Sud XI, Université de

207

Le rle de la presse dans la constitution du littraire au Bas-Canada et au Brsil au cours du premier XIXe sicle : vers la formation d'une culture nationale dans les collectivits neuves des Amriques.  

E-Print Network (OSTI)

??Cette thse envisage la formation des cultures nationales au sein de deux collectivits neuves des Amriques, alors que s'enclenche, au toumant du XIXe sicle, un (more)

Doyon, Nova

2008-01-01T23:59:59.000Z

208

Le franais langue trangre dans la formation linguistique des apprentis guides touristiques vnzuliens : pistes pdagogiques partir de l'analyse du discours.  

E-Print Network (OSTI)

??Notre tude s'inscrit dans les recherches en didactique des langues. Elle vise faire des propositions pdagogiques pour l'enseignement du franais langue trangre dans la (more)

Machado key, Yolibeth

2012-01-01T23:59:59.000Z

209

Modlisation des hydroliennes axe vertical libres ou carnes : dveloppement d'un moyen exprimental et d'un moyen numrique pour l'tude de la cavitation.  

E-Print Network (OSTI)

??Cette thse s'inscrit dans le cadre des nergies renouvelables au sein du programme HARVEST centr sur le dveloppement d'un concept d'hydrolienne driv des turbines Darrieus (more)

Aumelas, Vivien

2011-01-01T23:59:59.000Z

210

tude des machines frigorifiques absorption et absorption-diffusion utilisant un mlange d'alcanes : tude systmique et modlisation rigoureuse de l'absorbeur.  

E-Print Network (OSTI)

??Le prsent travail est consacr en premier lieu l'investigation des limites de fonctionnement et de performances des machines frigorifiques absorption et absorption-diffusion utilisant (more)

Dardour, Houda

2012-01-01T23:59:59.000Z

211

Energy Efficiency and Conservation Block Grant Program  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

IA-City-Des Moines IA-City-Des Moines Location: City Des Moines IA American Recovery and Reinvestment Act: Proposed Action or Project Description 1) Reimbursement for the cost of preparing the energy efficiency and conservation strategy, 2) perform energy audits to benchmark the energy performance of municipal buildings and fund public education/outreach campaign, 3) revolving loan program for energy efficiency retrofits and incremental costs for purchasing hybrid vehicles, 4) energy efficiency window retrofits at City Hall and the Police Station, 5) fund program to increase cycling and walking opportunities in the city including safety training and bicycle rodeo, 6) technical consultant services to develop long-term energy plan, 7) technical services to assist with building energy audits, and 8) replace high pressure sodium lighting with light-emitting diode

212

Page not found | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

51 - 25260 of 26,764 results. 51 - 25260 of 26,764 results. Article DOE Announces Additional Steps in Developing Sustainable Biofuels Industry Releases Results from Preliminary Intermediate Blends Report, Continues Commitment of Commercial Scale Biorefinery, Announces $7 Million for New Biofuels Projects http://energy.gov/articles/doe-announces-additional-steps-developing-sustainable-biofuels-industry Article A Touch of Green for Des Moines' Sherman Hill Des Moines' Green & Main intends to intends to renovate an abandoned 1930s grocery store into a mixed-use facility with LEED Platinum certification - a prestigious badge of energy efficiency and sustainable building practices. http://energy.gov/articles/touch-green-des-moines-sherman-hill Download Chapter 13- Simplified Acquisition Procedures

213

JEP-TALN-RECITAL 2012, Atelier TALAf 2012: Traitement Automatique des Langues Africaines, pages 6374, Grenoble, 4 au 8 juin 2012. c 2012 ATALA & AFCP  

E-Print Network (OSTI)

'opposition phonologique au niveau vocalique est observable dans des mots comme : karoo vs kaaroo ; kishii vs kiishii

214

UN SYSTEME MULTI-AGENTS GOUVERNE PAR DES LOIS LINGUISTIQUES POUR LE TRAITEMENT DE LA LANGUE NATUREI,LE  

E-Print Network (OSTI)

TALISMAN UN SYSTEME MULTI-AGENTS GOUVERNE PAR DES LOIS LINGUISTIQUES POUR LE TRAITEMENT DE LA de Linguistique Frangaise 1700 Univcrsit6 de FRIBOURG. SUISSE ABSTRACT Natural language processinggration d'outils linguistiques o0 les diff6rents agents du sysl~me peuvent mettre en oeuvre des m6thodes

215

Im Botanischen Garten des Instituts fr Biologie und Umweltwissenschaften der Fakultt fr Mathematik und Naturwissenschaften ist zum  

E-Print Network (OSTI)

Im Botanischen Garten des Instituts für Biologie und Umweltwissenschaften der Fakultät für Leiters (E 10 TV-L) unbefristet zu besetzen. Der Botanische Garten umfasst eine Fläche von ca. 5 ha. Zentrale Aufgaben des Gartens sind die Unterstützung bei Forschung und Lehre verschiedener, biologisch

Oldenburg, Carl von Ossietzky Universität

216

rencontre du non-lin aire 2000 257 Dynamiques des cristaux liquides sous r tro-injection optique  

E-Print Network (OSTI)

des quations d'optiques caract risant la r tro injection, de d river un mod le simple permettant l proposons de d river de ces qua- tions un mod le plus simple nous permettant de se ramener des r sultats th.C.L.V. pour Liquid Crystal Light Valve se compose essentiellement d'un miroir di lectrique qui est interpos

Gavilan, Marcel G. Clerc

217

Une note sur l'origine du concept des huit categories d'esprits  

E-Print Network (OSTI)

avec le systme social des castesdans les textes consacrs au culte des klu. On y trouve rje rigs, les seigneursdes klu, bram ze rigs, les brahmanes, et gdol bai rigs, les intouchables. dri et btsanDeux catgorie de dri (ou dri bo, l. 363) sont... ) donne la date 823 ainsi que Stein (1983 : 215) citant Z. Yamagu-chi, mais les critres qui ont servi cette datation ne sont pas clairs pour moi.25 Macdonald, Imaeda, 1978 : Pl. 10 (28a, l.4): ...byang chub sems dpa chen po brgyaddang/ khro bo gnyis...

Karmay, Samten G

2003-01-01T23:59:59.000Z

218

EXPOS ET MISE AU POINT BIBLIOGRAPHIQUE LA FORMATION DES PARTICULES DE CARBONE DANS LES FLAMMES  

E-Print Network (OSTI)

des fours, qu'ils soient aciéristes, verriers, ou cimentiers. On sait que le rayonnement des flammes d'hydro cristaux de noir d'acéty- lène peut être due à la présence d'atomes interstitiels d'hydrogène, car on trouve généralement 1 % d'hydro- gène dans les dépôts de carbone-suie. Pour certains auteurs la structure

Paris-Sud XI, Université de

219

Ce sont des réactions de fusion qui libèrent l'éner  

NLE Websites -- All DOE Office Websites (Extended Search)

Ce sont des réactions de fusion qui libèrent l'éner- Ce sont des réactions de fusion qui libèrent l'éner- gie qui alimente le soleil et les étoiles. Pour produire cette énergie, des plasmas de haute température doivent être confinés suffisamment longtemps. Les résultats de la recherche en physique des plasmas permettent de recréer sur terre les conditions requises pour la fusion thermonucléaire contrôlée. Leur objectif à long terme est l'approvisionnement énergétique, en complément d'autres sources, pour faire face aux besoins futurs. Sur un fond représentant le Soleil et la Terre, la présente affiche explore les différents thèmes concernés par la fusion: ses rapports avec d'autres formes d'énergie, la physique des réactions de fusion, le confinement et le chauffage des plasmas ainsi que l'avancement des

220

400 Jahre Chemie als Wissenschaft in Hamburg Von der Grndung des Akademischen Gymnasiums bis zu aktuellen  

E-Print Network (OSTI)

6 REIHE 1 400 Jahre Chemie als Wissenschaft in Hamburg Von der Gründung des Akademischen Gymnasiums bis zu aktuellen Forschungsthemen am Fachbereich Chemie der Universität Hamburg ZEIT UND ORT 08 als Wissenschaft in Hamburg zurückbli- cken. Der heutige Fachbereich Chemie der Universität Hamburg

Hamburg,.Universität

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


221

Inhalt des Studiums Das Studium der Chemie ist breit angelegt mit Schwerpunkten in den  

E-Print Network (OSTI)

Inhalt des Studiums Das Studium der Chemie ist breit angelegt mit Schwerpunkten in den Kernfächern der Chemie. Es werden gründliche theoretische und methodische Fachkenntnisse in allen wichtigen Studierenden ein ?berblick über die Zusammenhänge in der Chemie und ihren benachbarten Disiplinen verschafft

Fiebig, Peter

222

a) Conservation de la vorticit potentielle b) Description Heuristique des ondes de Rossby  

E-Print Network (OSTI)

a) Conservation de la vorticité potentielle b) Description Heuristique des ondes de Rossby c, flott@lmd.ens.fr 4) Les ondes de Rossby 57 #12;a) Conservation de la vorticité potentielle Approximation;a) Conservation de la vorticité potentielle Rappel de la méthode générale En formant l

Lott, Francois

223

Sur la radioactivit des sels de potassium Par j. C. Mc. LENNAN  

E-Print Network (OSTI)

rayons émis sont des rayions 8 de vitesse plus faible fi ne ceux de l'uranium . Durant ces derniers mois les expériences d'Elster et Geitel dans une mine, semblent montrer qu'il existe dans l

Paris-Sud XI, Université de

224

PROBLMES POSS POUR L'APPLICATION DES ALLIAGES DE NIOBIUM AUX AUBES DE TURBINE  

E-Print Network (OSTI)

the hottest sections of gas turbine engines features an interesting answer to problems introduced513 PROBL?MES POS?S POUR L'APPLICATION DES ALLIAGES DE NIOBIUM AUX AUBES DE TURBINE par G. GAUJE et refroidissement interne par convection s'applique en général aux aubes fixes et mobiles de 1 er étage de turbine

Paris-Sud XI, Université de

225

Ecole doctorale n 432 : Sciences des Mtiers de l'Ingnieur Doctorat ParisTech  

E-Print Network (OSTI)

FONCTIONNANT AVEC DES MELANGES ALTERNATIFS ZEOTROPES DE FLUIDES FRIGORIGENES............................... 77 (différence moyenne de température) ODP Ozone Depletion Potential (PAOS) ORC Organic Rankine Cycle PAC Pompe à compression mécanique de vapeur (CMV), cycles de Rankine organiques (ORC) ou à basse pression de vapeur d

Paris-Sud XI, Université de

226

Apport en acides gras insaturs et risque de cancer du sein : revue des tudes pidmiologiques  

E-Print Network (OSTI)

on the contributing food : neutral or beneficial for vegetable oil, rather deleterious for animal products. Contrary questionnaires alimentaires ou des marqueurs (plasma, érythrocytes, tissu adipeux). La relation entre apport en, erythrocytes, adipose tissue). The relationship between MUFA intake and breast cancer risk seems to depend

Paris-Sud XI, Université de

227

Article de synthse L'amplification des squences de nuclotides par PCR  

E-Print Network (OSTI)

Article de synthèse L'amplification des séquences de nucléotides par PCR et les nouvelles'?tude de la Fertilité; Paris, 19-21 octobre 1989) Résumé ― La PCR (polymerase chain reaction) est en plus grande dans les approches diagnostiques. PCR amplification / ADN / ARN / diagnostic

Recanati, Catherine

228

ErgEbnisbEricht 2001 2008 des Biotechnologisch-Biomedizinischen Zentrums  

E-Print Network (OSTI)

ErgEbnisbEricht 2001 ­ 2008 des Biotechnologisch-Biomedizinischen Zentrums #12;2 der Fokussierung-Offensive Personalentwicklung 14 Finanzierung 14 Eingeworbene Drittmittel und Drittmittelprojekte 17 Wissenschaftliche 99 Ausgründung c-LEcta ­ tuning enzymes 102 Anhang Wissenschaftliche Veröffentlichungen 106

Schüler, Axel

229

Facteurs linguistiques et sociolinguistiques de l'intgration en milieu multilingue : le cas des immigrants Montral.  

E-Print Network (OSTI)

??Cette recherche a pour but de dfinir et de dcrire les facteurs linguistiques et sociolinguistiques de lintgration des immigrants dans le contexte multilingue quest Montral. (more)

Calinon, Anne-Sophie A.-S.

2009-01-01T23:59:59.000Z

230

La vengeance du consommateur insatisfait sur Internet et l'effet sur les attitudes des autres consommateurs.  

E-Print Network (OSTI)

??Ce travail doctoral s'intresse au phnomne de vengeance du consommateur insatisfait sur Internet et l'effet de cette action sur les attitudes des autres consommateurs. Deux (more)

Passos, Gisle

2013-01-01T23:59:59.000Z

231

tude thorique et numrique de l'endommagement thermo-hydro-mcanique des milieux poreux non saturs.  

E-Print Network (OSTI)

??Les dchets radioactifs sont stocks dans des milieux poreux multi-phasiques. Un nouveau modle d'endommagement, formul en variable indpendantes (contrainte nette, succion et contrainte thermique) est (more)

Arson, Chlo

2009-01-01T23:59:59.000Z

232

Prvision d'ensemble locale des brouillard et nuages bas l'aroport international de Roissy Charles de Gaulle.  

E-Print Network (OSTI)

??Un systme de prvision d'ensemble locale (LEPS-Local Ensemble Prediction System) ciblant la prvision des brouillards et nuages bas sur l'aroport international de Paris Charles de (more)

Roquelaure, Stevie

2007-01-01T23:59:59.000Z

233

Impact de l'environnement sur l'endommagement laser des optiques de silice du Laser MgaJoule.  

E-Print Network (OSTI)

??Cette thse vise connatre et expliquer l'impact de la contamination molculaire sur l'endommagement laser des optiques en silice d'un laser de puissance tel que (more)

Bien-Aim, Karell

2009-01-01T23:59:59.000Z

234

Sur la propagation des ondes laser avec couplage l'hydrodynamique pour l'interaction laser plasma.  

E-Print Network (OSTI)

??On s'intresse la propagation des ondes laser dans le cadre de l'interaction laser plasma. On utilise une stratgie base sur une mthode de dcomposition (more)

Desroziers, Sylvain

2006-01-01T23:59:59.000Z

235

Linguistique et volution Anne Reboul, L2C2, CNRS UMR-5230, Institut des Sciences Cognitives, 67 bd Pinel,  

E-Print Network (OSTI)

Linguistique et évolution Anne Reboul, L2C2, CNRS UMR-5230, Institut des Sciences Cognitives, 67 bd Pinel, 69675 Bron cedex 1. Introduction En linguistique, la question de lévolution est, bien évidemment responsabilité des éventuelles erreurs restantes. 1 Le 8 mars 1868, la Société de Linguistique de Paris interdit

Institut des Sciences Cognitives, CNRS

236

LA REVUE DE L'EPI N 96 LE SITE DU MUSE DES ARTS ET MTIERS LE SITE WEB DU MUSE NATIONAL  

E-Print Network (OSTI)

: Musica Mecanica, PenWeb, TNC Network, L'?cho des Régions, Archives Photo CNAM. #12;158 Michelle ELARDJA

Paris-Sud XI, Université de

237

PCFB Repowering Project 80 MW plant description  

Science Conference Proceedings (OSTI)

This report documents the design of a 80 MW Pressurized Circulating Fluidized Bed (PCFB) boiler for the repowering of Unit 1 at the Des Moines Energy Center. Objective is to demonstrate that PCFB combined-cycle technology is cost effective and environmentally superior compared to traditional pulverized coal burning facilities.

Not Available

1994-05-01T23:59:59.000Z

238

2006 EPRI Cooling Tower Technology Conference Proceedings  

Science Conference Proceedings (OSTI)

Cooling towers and associated systems cause significant loss of availability and heat rate degradation in both nuclear and fossil-fired power plants. Fifteen papers presented at a 2006 Conference in Des Moines, Iowa discussed industrial experience and provided case histories of cooling tower problems and solutions.

2006-08-01T23:59:59.000Z

239

RECLAMATION  

NLE Websites -- All DOE Office Websites (Extended Search)

t a N o r t h N o r t h D a k o t a D a k o t a Boise Austin Topeka Pierre Helena Phoenix Lincoln Olympia Santa Fe Cheyenne Sacramento Des Moines Carson City Salt Lake City AE Comm...

240

Syst`eme de prevention du risque de renversement lateral pour des vehicules  

E-Print Network (OSTI)

de Charge Lat´eral (TCL), repr´esentatif des instabilit´es dynamiques lat´erales. Le TCL est calcul´eger Tout Terrain (VLTT), Transfert de Charge Lat´eral (TCL), observateur, pente lat´erale, quad, syst renversement Peters (2009), le TCL a ´et´e choisi car il n´ecessite seulement une mod´elisation simple du v

Paris-Sud XI, Université de

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


241

INTERPRTATION DES FAUTES D'EMPILEMENT DANS L'ANTIFERROMAGNTIQUE K2NiF4  

E-Print Network (OSTI)

859. INTERPR?TATION DES FAUTES D'EMPILEMENT DANS L'ANTIFERROMAGN?TIQUE K2NiF4 Par R. PLUMIER. 2014 Nous montrons qu'une légère déformation orthorhombique de la maille de K2NiF4 entraîne parNiF4 cell leads to a decrease of the free energy of the crystal through an exchange striction

Paris-Sud XI, Université de

242

IMITATION, PAR LES COURANTS LIQUIDES OU GAZEUX, DES PHNOMNES D'LECTRICIT ET DE MAGNTISME ;  

E-Print Network (OSTI)

être exposé succinctement. I. - Effets mécaniques. . Hydro-aimant. - Après avoir adapté à un tuyau d'au contact, car le liquide s'écoule au pourtour avec une faible vitesse; mais, si l'onveut soulever le tube'on puisse produire, avec ces deux sortes d'ajutages, des hydro-aimants à deux pôles contraires, l' un

Paris-Sud XI, Université de

243

Gnration de second harmonique dans des guides enterrs sur niobate de lithium.  

E-Print Network (OSTI)

Génération de second harmonique dans des guides enterrés sur niobate de lithium. Oleksandr niobate de lithium. Mots-clés : Optique non linéaire, Optique Intégrée, Niobate de lithium, Echange protonique sur niobate de lithium1 ,2 de nombreux progrès ont été réalisés. Grâce à la technique d

244

EFFETS DES FAIBLES IRRADIATIONS SUR L'URANIUM Par Y. QUR,  

E-Print Network (OSTI)

489. EFFETS DES FAIBLES IRRADIATIONS SUR L'URANIUM Par Y. QU?R?, Centre d'?tudes Nucléaires de fragments de fission dans l'uranium, on présente quelques résultats de mesure de longueur et de résistivité modifiés. Abstract. 2014 After recalling Brinkman's model for the action of fission fragments on uranium

Paris-Sud XI, Université de

245

Sur la radioactivit des solutions de sels d'uranium Par L. MICHIELS  

E-Print Network (OSTI)

432 Sur la radioactivité des solutions de sels d'uranium Par L. MICHIELS [Laboratoire de'une substanceradioactive ne produisant pas d'émanation, telle que l'uranium. D'une première série d'expériences effectuées au moyen de solutions de sulfate uranico-potassique K(UO)SO4+H2O dont la teneur, exprimée en uranium

Paris-Sud XI, Université de

246

DPARTEMENT DE PHYSIQUE DE L'COLE NORMALE SUPRIEURE  

E-Print Network (OSTI)

lortoireD en onférenes ou en éoles d9étéD de hulin à portlezD en pssnt pr des destintions moins exotiques ixhustivité et spéi(ité sur SQpre pour les liens de CexempleF F F F F F F F F F F F WR RFT yurrene des termes

Paris-Sud XI, Université de

247

The Magellan Final Report on Cloud Computing  

E-Print Network (OSTI)

10.5.1 Standard Hadoop Benchmarks . . . . . . . .10.5.2 Data Intensive Benchmarks . . . . . . . . . . 10.5.3workload analysis and benchmark selection process. Technical

Coghlan, Susan

2013-01-01T23:59:59.000Z

248

The Magellan Final Report on Cloud Computing  

E-Print Network (OSTI)

Theory High Energy Physics - High Energy Physics Theory NuclearTheory High Energy Physics - High Energy Physics Theory B2 Nuclear

Coghlan, Susan

2013-01-01T23:59:59.000Z

249

Magellan Tackles the Mysterious Proton Spin  

NLE Websites -- All DOE Office Websites (Extended Search)

image and with little tweaks have a bunch of sites run it." Aside from the real-time W event analysis, the STAR collaboration also processed a large sample of gold-gold events...

250

The Magellan Final Report on Cloud Computing  

E-Print Network (OSTI)

In order to meet DOE requirements, these features would needthrough the lens of DOE security requirements and report onscience? Can DOE cyber security requirements be met within a

Coghlan, Susan

2013-01-01T23:59:59.000Z

251

The Magellan Final Report on Cloud Computing  

E-Print Network (OSTI)

at the Argonne Leadership Computing Facility (ALCF) and theat the Argonne Leadership Computing Facility (ALCF) and theat the Argonne Leadership Computing Facility (ALCF) and the

Coghlan, Susan

2013-01-01T23:59:59.000Z

252

Magellan: experiences from a science cloud  

Science Conference Proceedings (OSTI)

Cloud resources promise to be an avenue to address new categories of scientific applications including data-intensive science applications, on-demand/surge computing, and applications that require customized software environments. However, there is a ... Keywords: cloud computing, mapreduce, programming model, science, virtual machines

Lavanya Ramakrishnan; Piotr T. Zbiegel; Scott Campbell; Rick Bradshaw; Richard Shane Canon; Susan Coghlan; Iwona Sakrejda; Narayan Desai; Tina Declerck; Anping Liu

2011-06-01T23:59:59.000Z

253

Magellan: experiences from a Science Cloud  

E-Print Network (OSTI)

at the Argonne Leadership Computing Facility (ALCF) and theArgonne Leadership Com- puting Facility (ALCF) and the National Energy Research Scientific Computing Facility (

Ramakrishnan, Lavanya

2013-01-01T23:59:59.000Z

254

Magellan: experiences from a Science Cloud  

E-Print Network (OSTI)

Leadership Computing Facility (ALCF) and the National EnergyCom- puting Facility (ALCF) and the National Energy Research

Ramakrishnan, Lavanya

2013-01-01T23:59:59.000Z

255

The Magellan Final Report on Cloud Computing  

E-Print Network (OSTI)

of the Argonne Leadership Computing Facility at Argonneof the Argonne Leadership Computing Facility at Argonneat the Argonne Leadership Computing Facility (ALCF) and the

Coghlan, Susan

2013-01-01T23:59:59.000Z

256

Magellan: experiences from a Science Cloud  

E-Print Network (OSTI)

at the Argonne Leadership Computing Facility (ALCF) and thescience at the Argonne Leadership Computing Facility and theof the Argonne Leadership Computing Facility at Argonne

Ramakrishnan, Lavanya

2013-01-01T23:59:59.000Z

257

The Magellan Final Report on Cloud Computing  

E-Print Network (OSTI)

resources. 1. Finding Tropical Cyclones on a Cloud Computing2010 2. Finding Tropical Cyclones on Clouds, D. Hasenkamp

Coghlan, Susan

2013-01-01T23:59:59.000Z

258

The Magellan Final Report on Cloud Computing  

E-Print Network (OSTI)

research used resources of the Argonne Leadership ComputingFacility at Argonne National Laboratory, which is supportedused resources of the Argonne Leadership Computing Facility

Coghlan, Susan

2013-01-01T23:59:59.000Z

259

Magellan: experiences from a Science Cloud  

E-Print Network (OSTI)

computing for science at the Argonne Leadership Computinghow the cloud computing business Argonne NationalLab Argonne, IL model can be used to serve the needs of mid-

Ramakrishnan, Lavanya

2013-01-01T23:59:59.000Z

260

The Magellan Final Report on Cloud Computing  

E-Print Network (OSTI)

NERSC partnered with ESnet and was able to provisionWestin Center Building ESnet provided ALU 7750-SR w/ 10Managed by SCinet 100G ESnet 100G 2x10 4x10 ESnet Internet2

Coghlan, Susan

2013-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


261

Magellan: experiences from a Science Cloud  

E-Print Network (OSTI)

desai)@mcs.anl.gov NERSC, Lawrence Berkeley National LabComputing Facility (NERSC). In this paper, we detail theComputing Facility (NERSC). The testbed con- sists of IBM

Ramakrishnan, Lavanya

2013-01-01T23:59:59.000Z

262

The Magellan Final Report on Cloud Computing  

E-Print Network (OSTI)

J. M. Shalf, and H. Wasserman. NERSC-6 workload analysis andand E. Strohmaier. The NERSC Sustained System Performance (of 2009. Resources and research at NERSC were funded by the

Coghlan, Susan

2013-01-01T23:59:59.000Z

263

The Magellan Final Report on Cloud Computing  

E-Print Network (OSTI)

Office of Advanced Scientific Computing Research (ASCR)Office of Advanced Scientific Computing Research (ASCR)Office of Advanced Scientific Computing Research (ASCR), was

Coghlan, Susan

2013-01-01T23:59:59.000Z

264

UniReport Satzungen und Ordnungen vom 03.09.2010 1 Ordnung des Fachbereichs Biochemie, Chemie, Pharmazie der Johann Wolfgang Goe-  

E-Print Network (OSTI)

UniReport Satzungen und Ordnungen vom 03.09.2010 1 Ordnung des Fachbereichs Biochemie, Chemie Biochemie, Chemie und Pharmazie am 07.06.2010 aufgrund des § 44 Abs.1 i.V. mit § 20 Abs.1 HHG beschlossene, Chemie und Pharmazie der Johann Wolfgang Goethe-Universität Frankfurt am Main den akademischen Grad

Mester, Rudolf

265

UniReport Satzungen und Ordnungen vom 25.09.2012 1 Ordnung des Fachbereichs Biochemie, Chemie und Pharmazie der Johann  

E-Print Network (OSTI)

UniReport Satzungen und Ordnungen vom 25.09.2012 1 Ordnung des Fachbereichs Biochemie, Chemie und) Die vom Fachbereich Biochemie, Chemie und Pharmazie am 12.03.2012 aufgrund des § 44 Abs.1 i.V. mit, Chemie und Pharmazie der Johann Wolfgang Goethe-Universität Frankfurt am Main den akademischen Grad

Mester, Rudolf

266

Contribution aux nombrables de la tradition Bon po : l'Appendive de bsTan 'dzin Rin chen rgyal mtshan a la Sphere de Cristal des Dieux et des Demons de Shar rdza rin po che  

E-Print Network (OSTI)

lettre Ha) ; 2. lessence fminine manifeste sous la forme du a shad etlocalise lextrmit infrieure du canal central ; et 3. le thig le indestructi-ble (mi shig pai thig le) localise dans le cur et exprime en fonction duneEssence vide (ngo bo... familiarisation avec les principes de lapratique, lors de la fusion des essences conscutive au Brasier et lEcoulement (bar dzag)44, il entre alors dans des expriences contemplativesde Dlice (bde ba), de Clart (gsal ba) et de Non-discursivit (mi rtog pa...

Achard, Jean-Luc

2003-01-01T23:59:59.000Z

267

Bifurcation vers l'etat d'Abrikosov et diagramme des phases  

E-Print Network (OSTI)

Nous \\'etudions dans cette th\\`ese la fonctionnelle de Ginzburg-Landau dans $\\R^3$ sur des couples de fonctions $(\\phi, \\overrightarrow{A})$ qui v\\'erifient des conditions de p\\'eriodicit\\'e de jauge en $x_3$ et selon un r\\'eseau discret de $(x_1,x_2)$. Nous montrons que le probl\\`eme variationnel est \\'equivalent au probl\\`eme de la minimisation d'une autre fonctionnelle sur un tore. Dans le cadre de la d\\'emonstration, un fibr\\'e vectoriel non trivial appara\\^it. On se limite alors pour la suite \\`a une quantification de 1. On montre ensuite que la fonctionnelle admet un minimum sur l'espace fonctionnel $H^{1}$ qui v\\'erifie un syst\\`eme d'\\'equations aux d\\'eriv\\'ees partielles appel\\'e syst\\`eme de Ginzburg-Landau. Le minimum est $C^{\\infty}$ par l'ellipticit\\'e du syst\\`eme d'\\'equations de Ginzburg-Landau. On montre qu'il y a une bifurcation du couple $(0,0)$ pour le champ critique $H_{ext}=k$ o\\`u $k$ est un param\\`etre caract\\'eristique du syst\\`eme. On \\'etudie alors la stabilit\\'e de la solution bifurqu\\'ee. On \\'etudie la d\\'ependance de l'\\'energie minimale \\`a l'\\'egard de la g\\'eom\\'etrie du tore. Enfin nous d\\'ecrivons toutes les solutions du syst\\`eme d'\\'equations de Ginzburg-Landau dans la limite $k$ tend vers l'infini. Dans le dernier chapitre, nous donnons pour notre mod\\`ele la structure du diagramme des phases en pr\\'ecisant quelles r\\'egions sont normales, supraconductrices pure, mixte.

Mathieu Dutour

1999-12-15T23:59:59.000Z

268

Etude ptrologique, gochimique et structurale des terrains cristallins de Belledonne entre l'Arc et l'Isre (Alpes franaises).  

E-Print Network (OSTI)

??La chaine de Belledonne est l'un des massifs cristallins,comme le Mont Blanc, l'Aar-Gothard au Nord-Est, les grandes Rousses , les Ecrins-Pelvoux, l'Argentera-Mercantour au Sud-Est. Ces (more)

Simeon, Yves

269

A propos d'un premier inventaire des monasteres bon po du Tibet et de l'Himalaya. Notes de lecture  

E-Print Network (OSTI)

bon po au Gansu (p. 504 et 506) et 10 au Qinghai (p.497-500, de faon plus dtaille). Revue dEtudes Tibtaines44 Bon po, la grande statue de Buddha du Bingling si (Gansu) est celle degShen rab mi bo. Il cite galement des relevs chinois des annes... 'dition de 1982 (Lanzhou,Kan su'u mi rigs dpe skrun khang), le numro de ligne est celui o apparat lenom du monastre ; sa dfinition ou localisation sommaire telle qu'elle peut tredduite des brves mentions du texte ou du contexte ; ventuellement...

Chayet, Anne

2004-01-01T23:59:59.000Z

270

Politique linguistique ducative l'gard de l'amazighe (berbre) au Maroc : des choix sociolinguistiques et didactiques leur mise en pratique.  

E-Print Network (OSTI)

??Ce travail de thse s'inscrit l'intersection des champs de la sociolinguistique et de la didactique dans un contexte de minoration linguistique. Il cherche (more)

Abouzaid, Myriam

2001-01-01T23:59:59.000Z

271

Comportement hydro-thermique d'un coulement de fluide dans une fracture rugueuse: Modlisation et application des massifs fracturs.  

E-Print Network (OSTI)

??Dans de nombreux rservoirs gothermiques profonds, l'changeur thermique est un massif de roches chaudes fractures. Comment la morphologie des fractures influence-t-elle le flux hydraulique et (more)

Neuville, Amlie

2010-01-01T23:59:59.000Z

272

Le dveloppement de LiDAR satellitaire multifonctions. Analyse exploratoire du potentiel de capteurs LiDAR pour le suivi altimtrique et bathymtrique des surfaces en eau continentales et ctires.  

E-Print Network (OSTI)

??Disposer de donnes prcises, spatialises et actualises sur les niveaux et les profondeurs des eaux ctires ou continentales est ncessaire pour assurer et anticiper une (more)

Abdallah, H.

2012-01-01T23:59:59.000Z

273

Annexe au projet de nouveau plan d'tudes de linguistique, soumis la commission des tudes le 9 fvrier 2010  

E-Print Network (OSTI)

Annexe au projet de nouveau plan d'études de linguistique, soumis à la commission des études le 9 février 2010 Dispositions transitoires - BA Les étudiants ayant commencé leur BA de linguistique avant l Les étudiants ayant commencé leur MA de linguistique avant l'entrée en vigueur du nouveau plan d

Genève, Université de

274

Le contenu de cet annuaire est sujet changement sans pravis et est bas sur des renseignements disponibles au  

E-Print Network (OSTI)

-25Jul2011 #12;4. ETUDE ET SEGMENTATION DE LA METHODE DU MPPT 115 4.1 La méthode du MPPT simple capteur de tension 115 4.2 Simulation des sous-blocs de la méthode du MPPT 117 5. SIMULATIONS GLOBALES 118 5 Logique 143 3.5 Fonctionnement global du filtre de puissance 144 4. LE BLOC POUR LA METHODE DU MPPT 145 4

Québec, Université du

275

MOUVEMENT D'UNE BULLE DANS UN LIQUIDE APPLICATIONS DE L'EFFET FUSE (FONCTIONNEMENT DES POMPES  

E-Print Network (OSTI)

dans l'écoulement d'une émulsion à l'intérieur d'une pompe centrifuge, dans l'érosion de cavitation électroérosion, dans la formation des aérosols et dans quelques autres cas possibles. Abstract. 2014 A gas relative to the flow of emulsions in centrifugal pumps, to cavitation erosion, to some problems

Paris-Sud XI, Université de

276

Modlisation et valuation du comportement dynamique d'une structure de machine outil UGV pour la prdiction des dfauts gomtriques  

E-Print Network (OSTI)

To achieve better performances in term of productivity, High Speed Machining centers have increasing kinematical characteristics. High accelerations caused by the trajectory execution dynamically load mechanical structure, axes and joints. Such deformations of mechanical components a ect the actual position of the tool in the machining frame. Hence, these gemetrical deviations make the machined geometry of the part vary from the expected one. Within the context of managing the HSM process, this study develops a framework and choice of nite element model to evaluate the structure dynamical behavior of a HSM center. Based on the proposed model, a calculation method is detailed to evaluate the geometrical deviations induced by the trajectory execution. The presented works can thus be used as a tool for the structure design of machine, the adjustment and the optimization of kinematical parameters for machining. --- Pour atteindre des performances accrues en terme de productivit\\'e, les centres d'Usinage Grande Vitesse poss\\`edent des caract\\'eristiques cin\\'ematiques \\'elev\\'ees. Les fortes acc\\'el\\'erations mises en jeu lors de l'ex\\'ecution des trajectoires sollicitent dynamiquement la structure et les liaisons. Les d\\'eformations engendr\\'ees peuvent alors se r\\'epercuter sur la position effective de l'outil par rapport \\`a la pi\\`ece cr\\'eant des \\'ecarts g\\'eom\\'etriques par rapport \\`a la g\\'eom\\'etrie attendue. Dans un contexte de ma\\^itrise du processus de r\\'ealisation de pi\\`eces en UGV, les travaux d\\'evelopp\\'es pr\\'esentent une d\\'emarche et un choix de mod\\'elisation \\'el\\'ements finis pour \\'evaluer le comportement dynamique d'une structure de centre UGV. Bas\\'e sur ce mod\\`ele, une m\\'ethodologie de calcul est propos\\'ee pour \\'evaluer les \\'ecarts g\\'eom\\'etriques g\\'en\\'er\\'es lors de l'ex\\'ecution de trajectoires types. Ces travaux constituent ainsi une voie pour le dimensionnement de structure, le r\\'eglage et l'optimisation des param\\`etres cin\\'ematiques pour l'usinage.

David Prvost; Sylvain Lavernhe; Franois Louf; Philippe Rouch

2011-11-03T23:59:59.000Z

277

CX-003913: Categorical Exclusion Determination | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

13: Categorical Exclusion Determination 13: Categorical Exclusion Determination CX-003913: Categorical Exclusion Determination Iowa-City-Des Moines CX(s) Applied: A1, A9, A11, B1.32, B5.1 Date: 09/17/2010 Location(s): Des Moines, Iowa Office(s): Energy Efficiency and Renewable Energy Energy Efficiency and Conservation Block Grant Program. 1) Reimbursement for the cost of preparing the energy efficiency and conservation strategy, 2) perform energy audits to benchmark the energy performance of municipal buildings and fund public education/outreach campaign, 3) revolving loan program for energy efficiency retrofits and incremental costs for purchasing hybrid vehicles, 4) energy efficiency window retrofits at City Hall and the Police Station, 5) fund program to increase cycling and walking opportunities in the city including safety training and bicycle

278

CX-000081: Categorical Exclusion Determination | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

81: Categorical Exclusion Determination 81: Categorical Exclusion Determination CX-000081: Categorical Exclusion Determination Des Moines' Energy Efficiency Retrofits and Programs CX(s) Applied: B1.32, B5.1, A1, A9, A11 Date: 11/17/2009 Location(s): Des Moines, Iowa Office(s): Energy Efficiency and Renewable Energy Energy Efficiency and Conservation Block Grant Program. 1) Reimbursement for the cost of preparing the energy efficiency and conservation strategy; 2) Perform energy audits to benchmark the energy performance of municipal buildings and fund public education/outreach campaign; 3) Revolving loan program for energy efficiency retrofits and incremental costs for purchasing hybrid vehicles; 4) Establish a mortgage buy-down program for residential buildings; 5) Energy efficiency window retrofits at City Hall

279

Iowa Community College Campuses Reduce Energy Use | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Iowa Community College Campuses Reduce Energy Use Iowa Community College Campuses Reduce Energy Use Iowa Community College Campuses Reduce Energy Use August 27, 2010 - 1:05pm Addthis DMACC will be installing nearly 1,500 occupancy sensors in the college's classrooms to help conserve energy.| Photo Courtesy of DMACC DMACC will be installing nearly 1,500 occupancy sensors in the college's classrooms to help conserve energy.| Photo Courtesy of DMACC Kevin Craft What are the key facts? Energy retrofit projects estimated to reduce annual energy use by 16 percent Des Moines Area Community College projects annual savings of $280,000 Project funded by nearly $640,000 in Recovery Act funding Des Moines Area Community College (DMACC) serves more than 65,000 Iowans on six campuses, making it the largest two-year college in the state of Iowa.

280

Categorical Exclusion Determinations: A1 | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

17, 2010 17, 2010 CX-003913: Categorical Exclusion Determination Iowa-City-Des Moines CX(s) Applied: A1, A9, A11, B1.32, B5.1 Date: 09/17/2010 Location(s): Des Moines, Iowa Office(s): Energy Efficiency and Renewable Energy September 17, 2010 CX-003745: Categorical Exclusion Determination Renewable Microgrid Scanning Transmission Electron Microscopy Education and Colonias Outreach Program CX(s) Applied: A1, A9 Date: 09/17/2010 Location(s): Texas Office(s): Electricity Delivery and Energy Reliability, National Energy Technology Laboratory September 17, 2010 CX-003739: Categorical Exclusion Determination National Electric Sector Cybersecurity Organization CX(s) Applied: A1, A9, A11 Date: 09/17/2010 Location(s): Clackamas, Oregon Office(s): Electricity Delivery and Energy Reliability, National Energy

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


281

Iowa's Clean Energy Economy is Working | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Iowa's Clean Energy Economy is Working Iowa's Clean Energy Economy is Working Iowa's Clean Energy Economy is Working July 30, 2012 - 1:52pm Addthis Under Secretary Sandalow tours Keystone Electrical Manufacturing Company with employees at the plant. | Photo courtesy of Keystone Manufacturing Co. Under Secretary Sandalow tours Keystone Electrical Manufacturing Company with employees at the plant. | Photo courtesy of Keystone Manufacturing Co. David Sandalow David Sandalow Former Under Secretary of Energy (Acting) and Assistant Secretary for Policy & International Affairs Extending the production tax credit means lower taxes and more jobs for Americans. David Sandalow EDITOR'S NOTE: This article was originally published in the Des Moines Register on July 28, 2012. This week, I visited Keystone Electrical Manufacturing Co. in Des Moines

282

CX-006016: Categorical Exclusion Determination | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

6: Categorical Exclusion Determination 6: Categorical Exclusion Determination CX-006016: Categorical Exclusion Determination Energy Efficiency and Conservation Block Grant Program - Iowa-City-West Des Moines CX(s) Applied: A1, A9, B2.5, B5.1 Date: 05/27/2011 Location(s): Des Moines, Iowa Office(s): Energy Efficiency and Renewable Energy Energy Efficiency and Conservation Block Grant Program. 1) Fund energy audits (benchmarking) and educational outreach and marketing campaign, 2) create revolving loan fund for energy efficiency projects, 3) develop and present training workshop for building green in the residential sector, 4) energy efficiency retrofits including window replacement, roof replacement, heating, ventilation and air conditioning (HVAC), ductwork, insulation, chiller replacement, pumps and lighting retrofits, 5) purchase and install

283

AgraGate Carbon Credits Corporation | Open Energy Information  

Open Energy Info (EERE)

AgraGate Carbon Credits Corporation AgraGate Carbon Credits Corporation Jump to: navigation, search Name AgraGate Carbon Credits Corporation Place Des Moines, Iowa Zip 50266 Product Offset aggregators that work with American farmers, ranchers, and private forest owners, providing clients with cash flows produced by the sale of credits. Offsets are sold on the Chicago Climate Exchange References AgraGate Carbon Credits Corporation[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. AgraGate Carbon Credits Corporation is a company located in Des Moines, Iowa . References ↑ "AgraGate Carbon Credits Corporation" Retrieved from "http://en.openei.org/w/index.php?title=AgraGate_Carbon_Credits_Corporation&oldid=341882"

284

Iowa Office of Energy Independence | Open Energy Information  

Open Energy Info (EERE)

Iowa Office of Energy Independence Iowa Office of Energy Independence Jump to: navigation, search Name Iowa Office of Energy Independence Place Des Moines, Iowa Zip IA 50319 Product In 2007, Governor Culver and the Iowa State Legislature created the Office of Energy Independence and the Iowa Power Fund to accelerate Iowaâ€(tm)s leadership in energy for the 21st Century. References Iowa Office of Energy Independence[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Iowa Office of Energy Independence is a company located in Des Moines, Iowa . References ↑ "Iowa Office of Energy Independence" Retrieved from "http://en.openei.org/w/index.php?title=Iowa_Office_of_Energy_Independence&oldid=347104

285

Categorical Exclusion Determinations: Office of Energy Efficiency and  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

7, 2010 7, 2010 CX-003993: Categorical Exclusion Determination Closed Loop Short Rotation Woody Biomass Energy Crops, Pending Renewable of Grant Award CX(s) Applied: B3.6, B3.8, B5.1 Date: 09/17/2010 Location(s): New York Office(s): Energy Efficiency and Renewable Energy, Golden Field Office September 17, 2010 CX-003913: Categorical Exclusion Determination Iowa-City-Des Moines CX(s) Applied: A1, A9, A11, B1.32, B5.1 Date: 09/17/2010 Location(s): Des Moines, Iowa Office(s): Energy Efficiency and Renewable Energy September 17, 2010 CX-003797: Categorical Exclusion Determination Recovery Act: San Bernardino Associated Government Natural Gas Truck Project - Alternative Fueling Station in Rancho Cucamonga, California CX(s) Applied: B5.1 Date: 09/17/2010 Location(s): Rancho Cucamonga, California

286

Revue transatlantique d'tudes suisses  

E-Print Network (OSTI)

. Perspectives dialectologiques Yan GREUB, « La genèse de l'espace linguistique francoprovençal: le témoignage'une des langues distinctes du groupe linguistique galloroman, il présente certains traits communs avec le linguistique de génération en génération et hésitent moins à parler l'idiome local à leurs enfants, à l

Parrott, Lael

287

Batrice David, La dynamique de l'ethnicit rurale et urbaine dans le kalidoscope des identits hongkongaises , in L. Augustin-Jean & F. Padovani (dir.), Hong Kong. Economie,  

E-Print Network (OSTI)

, de nature territoriale et sociale, qui séparent 7 Cf. J. Lagerwey, 1992, p. 367. Sur les jiao* dans les villages des Nouveaux Territoires, voir notamment D. Faure, 1986, p. 80-86. 8 Cf. Choi Chi, 1946, He Ge'en, 1955, Zhang Shouqi, 1991. 14 Cf. B. David, op. cit., p. 18-59. Formatted: Indent: First

Peyré, Gabriel

288

ITPA Joint Meeting on Control, St. Petersburg, Russia, 14/07/2003 R. A. Pitts, Centre de Recherches en Physique des Plasmas Some requirements and possibilities for the  

E-Print Network (OSTI)

ITPA Joint Meeting on Control, St. Petersburg, Russia, 14/07/2003 R. A. Pitts, Centre de Recherches de Recherches en Physique des Plasmas #12;ITPA Joint Meeting on Control, St. Petersburg, Russia, 14 factors, pumping Materials · Erosion and redeposition, tritium inventory #12;ITPA Joint Meeting on Control

289

INTERNATIONAL CONFERENCE ON ENGINEERING DESIGN, ICED'07 28 -31 AUGUST 2007, CITE DES SCIENCES ET DE L'INDUSTRIE, PARIS, FRANCE  

E-Print Network (OSTI)

and the solution evolve parallel. Then, we explain that the complexity of the medical devices needs specificINTERNATIONAL CONFERENCE ON ENGINEERING DESIGN, ICED'07 28 - 31 AUGUST 2007, CITE DES SCIENCES ET, there is such a difficulty of medical terms routinely employed by the surgeon to explain his need, which causes to reduction

Paris-Sud XI, Université de

290

Enseignement-apprentissage d'une discipline linguistique et non-linguistique l'cole primaire : analyse de l'action conjointe professeurs-lves dans des classes primaires bilingues en Thalande.  

E-Print Network (OSTI)

??Notre thse vise tudier et caractriser les situations didactiques mises en oeuvre pour l'enseignement de l'anglais, une discipline linguistique, et des sciences, une discipline (more)

Kewara, Punwalai

2012-01-01T23:59:59.000Z

291

Comparaison des discours publics de Theobald Wolfe Tone (Irlande) et de Louis-Joseph Papineau (Bas-Canada) sur le lien la Grande-Bretagne et sur la constitution.  

E-Print Network (OSTI)

??L'objectif de ce mmoire est de rendre compte, en les comparant, des discours publics respectifs de Theobald Wolfe Tone, pour l'Irlande, et de Louis-Joseph Papineau (more)

Guyot, Julie

2009-01-01T23:59:59.000Z

292

tude de l'effet d'inhibition du gel induit par les sulfates dans les nuages arctiques l'aide des mesures satellitaires de CloudSat et CALIPSO.  

E-Print Network (OSTI)

??Les sulfates issus de la pollution industrielle d'Eurasie et transports travers la basse troposphre arctique durant l'hiver sont souponns d'altrer les proprits des nuages (more)

Grenier, Patrick

2010-01-01T23:59:59.000Z

293

The Magellan Project: Building High-Performance Clouds | Argonne...  

NLE Websites -- All DOE Office Websites (Extended Search)

our network interfaces were the limiting factor was excellent; that demonstrates the low overhead virtualization can have, while leaving room for improved node performance. Even...

294

Magellan at NERSC Progress Report for June 2010  

E-Print Network (OSTI)

DOE clouds (at NERSC and ALCF) provide high availability byLeadership Computing Facility (ALCF) and the National Energy

Broughton, Richard Canon, Lavanya Ramakrishnan, Brent Draney, Jeff

2011-01-01T23:59:59.000Z

295

Magellan at NERSC Progress Report for June 2010  

E-Print Network (OSTI)

33] R. Masud, High Performance Computing with Clouds. [framework for high-performance computing systems. In IEEEConference for High Performance Computing, Networking,

Broughton, Richard Canon, Lavanya Ramakrishnan, Brent Draney, Jeff

2011-01-01T23:59:59.000Z

296

Magellan additional information | U.S. DOE Office of Science...  

Office of Science (SC) Website

for Teachers and Scientists Small Business Innovation Research and Small Business Technology Transfer Project Assessment Laboratories Ames Laboratory Argonne National...

297

Magellan at NERSC Progress Report for June 2010  

E-Print Network (OSTI)

Antypas and H. Wasserman. Nersc-6 workload analysis andand E. Strohmaier, The NERSC Sustained System Performance (M. Shalf, and H. Wasserman, NERSC-6 workload analysis and

Broughton, Richard Canon, Lavanya Ramakrishnan, Brent Draney, Jeff

2011-01-01T23:59:59.000Z

298

JEP-TALN-RECITAL 2012, Atelier DEGELS 2012: Dfi GEste Langue des Signes, pages 5772, Grenoble, 4 au 8 juin 2012. c 2012 ATALA & AFCP  

E-Print Network (OSTI)

nature linguistique ou non de leur statut sous les 5 pistes suivantes : Français ; Onomatopées'une part, quant au statut linguistique ou non de l'unité formelle, et, d'autre part, quant à l'une manière générale les tentatives de la linguistique structurale de s'abstraire des questions de sens

299

Gestion des auto-occultations pour l'augmentation d'une surface deformable V. Gay-Bellile1,2  

E-Print Network (OSTI)

Gestion des auto-occultations pour l'augmentation d'une surface d´eformable V. Gay-Bellile1,2 A peu. La surface est habituellement suppos´ee ne pas s'auto-occulter. En effet, l'estimation d'une fonction de d´eformation en pr´esence d'auto-occultations s'av`ere complexe. Cette article propose un

Bartoli, Adrien

300

Sehr geehrte Damen und Herren, liebe Freunde der bildenden Kunst, wir mchten Sie herzlich zum 20. Jubilum des Kunstpfades der Ulmer Universitt einladen.  

E-Print Network (OSTI)

Garten. B Am Musischen Zentrum spielt die Bigband der Universität Ulm und wandert anschlie?end als NewOrleansZug zum Botanischen Garten. Snacks&Getränke am Atelier. C Vor den Gewächshäusern des Botanischen Gartens Holzskulpturen, die sich am Abend zu Feuerskulpturen verwandeln. Um 17:00 Uhr wird im Botanischen Garten auf der

Ulm, Universität

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


301

Particularits d'adoption des compteurs intelligents au Royaume-Uni et en Allemagne : entre marchs de comptage libralis et rgles mettre en place pour un rel smart grid intgr.  

E-Print Network (OSTI)

marchés de comptage libéralisé et règles à mettre en place pour un réel smart grid intégré. Association maximiser les bénéfices d'un réel smart grid intégré dans lequel les compteurs sont un élément déterminant'une des composantes majeures des réseaux électriques intelligents ou smart grids. Selon la Directive

Paris-Sud XI, Université de

302

La Liste Des Tantras Du rNying Ma'i Rgyud 'bum Selon L'edition Et Ablie Par Kun Mkhyen 'Jigs Med Gling Pa  

E-Print Network (OSTI)

gro bai rgyud lnga) qui sontcommuns lAnuyoga24 et dont la liste concerne les nos. 229, 224, 169, 166 etun Ri bo brtsegs pai rgyud qui est non-identifi dans la liste de Jigs med glingpa),xvi. le Recueillement Concentr (Ting dzin rtse gcig, non... on pourrait leur en trouver une, ainsi quon la fait dans cette prsentation. Il faudrait galement appliquer ce schma celui des clas- sification complexes du Klong sde en Abme blanc (klong dkar po), noir (klong nag po), diapr (klong khra bo) et infini...

Achard, Jean-Luc

2002-01-01T23:59:59.000Z

303

"1. Walter Scott Energy Center","Coal","MidAmerican Energy Co",1660  

U.S. Energy Information Administration (EIA) Indexed Site

Iowa" Iowa" "1. Walter Scott Energy Center","Coal","MidAmerican Energy Co",1660 "2. George Neal North","Coal","MidAmerican Energy Co",957 "3. Louisa","Coal","MidAmerican Energy Co",746 "4. Ottumwa","Coal","Interstate Power and Light Co",696 "5. George Neal South","Coal","MidAmerican Energy Co",645 "6. Duane Arnold Energy Center","Nuclear","NextEra Energy Duane Arnold LLC",601 "7. Emery Station","Gas","Interstate Power and Light Co",518 "8. Greater Des Moines","Gas","MidAmerican Energy Co",496 "9. Pioneer Prairie Wind Farm","Other Renewables","Pioneer Prairie Wind Farm I, LLC",300

304

EPRI Biomass Interest Group Meeting 3 Results--2005  

Science Conference Proceedings (OSTI)

The EPRI Biomass Interest Group meets three times per year to exchange information on projects, explore new technologies, and to set the research agenda for the group. In 2005, the first meeting was held in March in Washington, DC, the second meeting was a tour of biomass facilities in Europe, and the third meeting was December 6, 2005 in Des Moines, Iowa. This report summarizes the results of that meeting, including a tour of the switchgrass cofiring facility at the nearby Ottumwa Generating Station.

2006-03-21T23:59:59.000Z

305

LINGUISTIQUE Facult des arts  

E-Print Network (OSTI)

'immersion linguistique rencontrent un succès grandissant. D'après les chiffres publiés lors du colloque `immersion linguistique et bilinguisme précoce' qui s'est tenu à l'Université de liège le 21 avril 2012, la communauté. Il comportera plusieurs volets : un encadrement linguistique en allemand et en français (basé surtout

Petriu, Emil M.

306

Gliederung des Wirtschaftsrechts - Springer  

Science Conference Proceedings (OSTI)

Not logged in Google [Search Crawler] (3000811494) 66.249.75.182. Springer for Research & Development. UA-26408784-1. JavaScript is currently disabled,...

307

Pondration des phrases  

Science Conference Proceedings (OSTI)

... P = (dr1 + + dri + + drm) / (dq1 + + drj + + dqn) with: dri: specificity degree of a lemma from the question found in the sentence, dqj ...

2003-02-13T23:59:59.000Z

308

Rechtliche Aspekte des Finanzratings  

Science Conference Proceedings (OSTI)

Bankenaufsicht am 26. Juni 2004 beschlossene Reform der Baseler Eigenkapitalvorschriften. (Basel II) bevorstehenden Vernderungen im Aufsichtsrecht vor.

309

Test des Systmes hybrides.  

E-Print Network (OSTI)

??Les systmes hybrides, systmes combinant la fois une dynamique continue et discrte, s'avrent tre un modle mathmatique utile pour diffrents phnomnes physiques, technologiques, biologiques (more)

Nahhal, Tarik

310

DES Validation List  

Science Conference Proceedings (OSTI)

... d) "The HIPP 7855 security processors packaged as part ... have it all in a single high-performance package." ... XXX" in P/N indicates plastic case colour ...

311

Triple DES Validation List  

Science Conference Proceedings (OSTI)

... 1506, Aviat Networks 5200 Great America Parkway Santa ... 350MHz; Intel Woodcrest 2.13GHz; Power-PC 405 ... 604 (32-bit) w/ Wind River VxWorks ...

312

Methoden des Erfindens - Springer  

Science Conference Proceedings (OSTI)

eben auch eine wissenschaftlich technische Erfindung. Hypothesen, Ideen .... Technologicus beobachten eines Menschen, der eine wissenschaftliche Metho -.

313

PARCOURS DES ALPHA DE 4,5 MeV DANS L'URANIUM, L'OR, LE ZIRCONIUM ET LE SILICIUM. Par Mmes A. GARIN et H. FARAGGI,  

E-Print Network (OSTI)

76. PARCOURS DES ALPHA DE 4,5 MeV DANS L'URANIUM, L'OR, LE ZIRCONIUM ET LE SILICIUM. Par Mmes A uranium alloys of known concentration in uranium it is possible to measure the range of 4,5 MeV 03B1 mesurant l'émission oc d'alliages d'uranium de différentes concentrations. Nous avons pu disposer d

Paris-Sud XI, Université de

314

Page not found | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

21 - 2730 of 28,905 results. 21 - 2730 of 28,905 results. Download CX-004138: Categorical Exclusion Determination Oklahoma-Tribe-Osage Nation CX(s) Applied: A9, A11, B5.1 Date: 10/01/2010 Location(s): Oklahoma Office(s): Energy Efficiency and Renewable Energy http://energy.gov/nepa/downloads/cx-004138-categorical-exclusion-determination Download CX-003913: Categorical Exclusion Determination Iowa-City-Des Moines CX(s) Applied: A1, A9, A11, B1.32, B5.1 Date: 09/17/2010 Location(s): Des Moines, Iowa Office(s): Energy Efficiency and Renewable Energy http://energy.gov/nepa/downloads/cx-003913-categorical-exclusion-determination Download CX-003911: Categorical Exclusion Determination California-City-Diamond Bar CX(s) Applied: A1, A9, A11, B1.32, B3.6, B5.1 Date: 09/15/2010 Location(s): Diamond Bar, California

315

Iowa Gasoline Price Data  

NLE Websites -- All DOE Office Websites (Extended Search)

Iowa Iowa Exit Fueleconomy.gov The links below are to pages that are not part of the fueleconomy.gov. We offer these external links for your convenience in accessing additional information that may be useful or interesting to you. Selected Cities Ames AmesGasPrices.com Automotive.com MapQuest.com Cedar Rapids CedarRapidsGasPrices.com Automotive.com MapQuest.com Council Bluffs CouncilBluffsGasPrices.com Automotive.com MapQuest.com Des Moines DesMoinesGasPrices.com Automotive.com MapQuest.com Dubuque DubuqueGasPrices.com Automotive.com MapQuest.com Iowa City IowaCityGasPrices.com Automotive.com MapQuest.com Quad Cities QuadCitiesGasPrices.com Sioux City SiouxCityGasPrices.com Automotive.com MapQuest.com Waterloo WaterlooGasPrices.com Automotive.com MapQuest.com Other Iowa Cities

316

Iowa Datos del Precio de la Gasolina  

NLE Websites -- All DOE Office Websites (Extended Search)

Iowa Iowa Salga de Ahorremosgasolina.org Los enlaces a continuación llevan a páginas que no son la parte del Sitio Web de ahorremosgasolina.org. Ofrecemos estos enlaces externos para su conveniencia y para ofrecerle acceso a información adicional que puede serle útil o interesante. Ciudades Selectas Ames AmesGasPrices.com Automotive.com MapQuest.com Cedar Rapids CedarRapidsGasPrices.com Automotive.com MapQuest.com Council Bluffs CouncilBluffsGasPrices.com Automotive.com MapQuest.com Des Moines DesMoinesGasPrices.com Automotive.com MapQuest.com Dubuque DubuqueGasPrices.com Automotive.com MapQuest.com Iowa City IowaCityGasPrices.com Automotive.com MapQuest.com Quad Cities QuadCitiesGasPrices.com Sioux City SiouxCityGasPrices.com Automotive.com MapQuest.com Waterloo WaterlooGasPrices.com Automotive.com MapQuest.com

317

Obtaining the optimal fuel conserving investment mix: a linear programming hedonic technique approach  

SciTech Connect

The objectives of this study were to: (1) determine how energy efficiency affects the resale value of homes; (2) use this information concerning the implicit price of energy efficiency to estimate the resale value of fuel saving investments; and (3) incorporate these resale values into the investment decision process and determine the efficient investment mix for a household planning to own a given home for three alternative time periods. Two models were used to accomplish these objectives. A hedonic price model was used to determine the impact of energy efficiency on housing prices. The hedonic technique is a method used to attach implicit prices to characteristics that are not themselves bought and sold in markets, but are components of market goods. The hedonic model in this study provided an estimate of the implicit price paid for an increase in energy efficiency in homes on the Des-Moines housing market. In order to determine how the length of time the home is to be owned affects the optimal investment mix, a linear programming model was used to determine the cost minimizing investment mix for a baseline house under the assumption that it would be owned for 6, 20, and 50 years, alternatively. The results of the hedonic technique revealed that a premium is paid for energy efficient homes in Des Moines. The results of the linear programming model reveal that the optimal fuel saving investment mix for a home is sensitive to the time the home is to be owned.

Dinan, T.M.

1984-01-01T23:59:59.000Z

318

Faszination Chemie: Keine unter allen Wissenschaften bietet dem Menschen eine grssere Flle von Gegenstnden des Denkens, der berlegung und von frischer, sich stets erneuender Erkenntnis dar als die Chemie. F O T O : S C H U E R P F , Z R I C H  

E-Print Network (OSTI)

Faszination Chemie: «Keine unter allen Wissenschaften bietet dem Menschen eine grössere Fülle von Gegenständen des Denkens, der ?berlegung und von frischer, sich stets erneuender Erkenntnis dar als die Chemie Gesellschaft Deutscher Chemi- ker beschrieben wurde, erregt nicht alle Forscher gleich. Oft stösst sie auf

Giger, Christine

319

Eros variable stars A catalog of Cepheids in the Magellanic Clouds  

E-Print Network (OSTI)

We present a catalog containing 290 LMC and 590 SMC Cepheids which have been obtained using the two 4k $\\times$ 8k CCD cameras of the EROS~2 microlensing survey. The Cepheids were selected from 1,134,000 and 504,000 stars in the central regions of the LMC and SMC respectively, that were monitored over 150 nights between October 1996 and February 1997, at a rate of one measurement every night. For each Cepheid the light curves, period, magnitudes in the EROS~2 filter system, Fourier coefficients, J2000 coordinates and cross-identifications with objects referenced in the CDS Simbad database are presented. Finding charts of identified Cepheids in clusters NGC 1943, NGC 1958 and Bruck 56 are presented. The catalogue and the individual light--curves will be electronically available through the CDS (Strasbourg).

Afonso, C; Alard, C; Amadon, A; Andersen, J; Ansari, R; Aubourg, E; Bauer, F; Bareyre, P; Beaulieu, J P; Blanc, G; Bouquet, A; Char, S; Charlot, X; Couchot, F; Coutures, C; Derue, F; Ferlet, R; Gaucherel, C; Glicenstein, J F; Goldman, B; Gould, A; Graff, D S; Gros, M H; Hassinski, J; Hamilton, J C; Hardin, D P; De Kat, J; Kim, A; Lasserre, T; Lesquoy, E; Loup, C; Magneville, C; Mansoux, B; Marquette, J B; Maurice, E; Milshtein, A I; Moniez, M; Palanque-Delabrouille, Nathalie; Perdereau, O; Prvt, L; Renault, C; Regnault, N; Rich, J; Spiro, Michel; Vidal-Madjar, A; Vigroux, L; Zylberajch, S

1999-01-01T23:59:59.000Z

320

The Magellanic System: Stars, Gas, and Galaxies Proceedings IAU Symposium No. 256, 2008  

E-Print Network (OSTI)

Gamma Ray Bursts progenitors foresee possible LGRBs progenitors at the SMC's metallicity. We confront parameters, gamma rays: theory 1. Introduction, observations This document deals with the determination

Recanati, Catherine

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


321

Submillimeter studies of cold gas and dust in the Magellanic Clouds .  

E-Print Network (OSTI)

??Presentamos datos a 870 mu obtenidos con el telescopio APEX en la SMC, LMC y puente Magallanico, obteniendo imagenes con 22 .4'' de resolucion para (more)

Verdugo Salgado, Celia Anahi

2012-01-01T23:59:59.000Z

322

Dpartement de chimie Facult des arts et des sciences  

E-Print Network (OSTI)

linguistique de l'Université de Montréal L'Université de Montréal est une université québécoise de langue à la Politique linguistique de l'Université de Montréal [http://www.direction.umontreal.ca/secgen/recueil/politique_linguistique

Montréal, Université de

323

Dpartement de chimie Facult des arts et des sciences  

E-Print Network (OSTI)

'adresse suivante : http://www.chimie.umontreal.ca/. Politique linguistique de l'Université de Montréal L spécialistes dans le monde et s'assure par ailleurs que, conformément à la Politique linguistique de l'Université de Montréal [http://www.direction.umontreal.ca/secgen/recueil/politique_linguistique.html], les

Charette, André

324

Dpartement de chimie Facult des arts et des sciences  

E-Print Network (OSTI)

://www.chimie.umontreal.ca/. Politique linguistique de l'Université de Montréal L'Université de Montréal est une université québécoise de, conformément à la Politique linguistique de l'Université de Montréal [http://www.direction.umontreal.ca/secgen/recueil/politique_linguistique

Charette, André

325

Dpartement de physique Facult des arts et des sciences  

E-Print Network (OSTI)

en consultant le site Web à l'adresse suivante : www.phys.umontreal.ca. #12;* Politique linguistique à la Politique linguistique de l'Université de Montréal (http://www.direction.umontreal.ca/secgen/recueil/politique_linguistique

Montréal, Université de

326

INSTITUT DE MECANIQUE DES FLUIDES ET DES SOLIDES  

E-Print Network (OSTI)

power density (HPD) solid oxide fuel cell (SOFC) is a geometry based on a tubular type SOFC increased power density, but still maintains the beneficial feature of secure sealing for a tubular SOFC. In this paper, the electric performance of a flat-tube HPD SOFC is studied. This paper also investigates

Genaud, Stéphane

327

Facult des arts et des sciences Dpartement de chimie  

E-Print Network (OSTI)

of Manchester "Conformational Control; New Organolithium Reactivity" Salle S1-111, Pavillon Jean-Coutu 15 Light Harvesting" Salle S1-111, Pavillon Jean-Coutu #12;Février February 22 PROFESSEUR DAVID VOCADLO1-111, Pavillon Jean-Coutu ANNUL?E CANCELLED 29 CONF?RENCE CRMAA-CSACS PROFESSEUR FRANCESCO

Charette, André

328

Modulbezeichnung: Querschnittsbereich Medizin des Alterns und des alten Menschen (Geriatrie)  

E-Print Network (OSTI)

") Weiterführende Literatur: Platt D (Hrsg): Altersmedizin. Schattauer-Verlag, Stuttgart, New York, 1997 (ca. 900 Seiten) Nikolaus T (Hrsg) Klinische Geriatrie, Springer Verlag, Berlin, 2000 (ca. 900 Seiten). Kolb

Manstein, Dietmar J.

329

Andr Laperrire Laboratoire des technologies  

E-Print Network (OSTI)

customer confidence, leading ultimately to market transformation » (Electric Power Research Institute EPRI PERIOD no 1 : Integrating sphere Luminaire LED Luminaire T5HO Luminaire MH Power (Watts) 373 326 460 no 2 : Goniophotometer and dimming effect 100% of LED power 75% of LED power 50 % of LED power 25

California at Davis, University of

330

HABILITATION A DIRIGER DES RECHERCHES  

E-Print Network (OSTI)

CORSE M. BALBI JACQUES-HENRI PR, DIR. LAB. UMR CNRS 6134, U.DE CORSE M. LOUCHE ALAIN PR, U. DE CORSE M-Henri BALBI (Université de Corse) et Alain LOUCHE (Université de Corse) pour leur participation à cette

Paris-Sud XI, Université de

331

Das China des Carl Gtzlaff.  

E-Print Network (OSTI)

??Analysiert wird der 1. Opiumkrieg zwischen Grobritannien und China. Das zeitgenssische Chinabild wird anhand von Darstellungen in deutschsprachigen Zeitungen mittels Textanalyse hinterfragt. Es wird die (more)

Immervoll, Robert

2008-01-01T23:59:59.000Z

332

COMMISSION INTERNATIONALE DES GRANDS BARRAGES  

E-Print Network (OSTI)

of the dam (for example, concrete gravity section, main embankment or saddle embankment); · The estimateEstimating Overall Risk of Dam Failure: Practical Considerations in Combining Failure Probabilities ANCOLD 2003 Risk Workshop Page 1 ESTIMATING OVERALL RISK OF DAM FAILURE: PRACTICAL CONSIDERATIONS

Cirpka, Olaf Arie

333

Other Participants 1991 | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

1 1 National Science Bowl® (NSB) NSB Home About National Science Bowl Contacts Regional Science Bowl Coordinators National Science Bowl FAQ's Alumni Past National Science Bowl Winners Past National Science Bowl Photos National Science Bowl Logos High School Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Past High School National Science Bowl Winners (1991 - 2012) Other Participants 1991 Print Text Size: A A A RSS Feeds FeedbackShare Page Abraham Lincoln High School , Des Moines , IA Beavercreek High School , Beavercreek , OH Crystal Lake South High School , Crystal Lake , IL

334

Category:Utility Rate Impacts on PV Economics By Location | Open Energy  

Open Energy Info (EERE)

Utility Rate Impacts on PV Economics By Location Utility Rate Impacts on PV Economics By Location Jump to: navigation, search Impact of Utility Rates on PV Economics Montgomery, AL Little Rock, AR Flagstaff, AZ Phoenix, AZ Tucson, AZ Arcata, CA LA, CA San Francisco, CA Boulder, CO Eagle County, CO Pueblo, CO Bridgeport, CT Wilmington, DE Miami, FL Tampa, FL Atlanta, GA Savannah, GA Des Moines, IA Mason, IA Boise, ID Chicago, IL Springfield, IL Indianapolis, IN Goodland, KS Wichita, KS Lexington, KY New Orleans, LA Shreveport, LA Boston, MA Baltimore, MD Caribou, ME Portland, ME Detroit, MI Houghton-Lake, MI Traverse City, MI International Falls, MN Minneapolis, MN Kansas City, MO Jackson, MS Billings, MT Greensboro, NC Wilmington, NC Bismarck, ND Minot, ND Omaha, NE Concord, NH Atlantic City, NJ Albuquerque, NM Las Vegas, NV Reno, NV New York, NY

335

Roeder Farms | Open Energy Information  

Open Energy Info (EERE)

Roeder Farms Roeder Farms Jump to: navigation, search Name Roeder Farms Facility Roeder Farms Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner 5045 Wind Partners Developer 5045 Wind Partners Energy Purchaser Alliant Energy Location Des Moines IA Coordinates 43.29729211°, -93.28315258° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":43.29729211,"lon":-93.28315258,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

336

DOE - Office of Legacy Management -- Iowa Army Ammunition Plant - IA 02  

Office of Legacy Management (LM)

Army Ammunition Plant - IA 02 Army Ammunition Plant - IA 02 FUSRAP Considered Sites Iowa Army Ammunition Plant, IA Alternate Name(s): Burlington Ordnance Plant Iowa Ordnance Plant Silas Mason Company IA.02-3 Location: Located in Township 70 North, Range 3 West, Section 32, 5th Principal Meridian, Des Moines County, Burlington, Iowa IA.02-1 IA.02-5 Historical Operations: Assembled nuclear weapons, primarily high explosive components and conducted explosives testing using the high explosive components and depleted uranium. AEC and ERDA operations conducted under permit from the Department of the Army. IA.02-3 IA.02-4 Eligibility Determination: Eligible IA.02-5 Radiological Survey(s): Assessment Survey IA.02-2 Site Status: Cleanup pending by U.S. Army Corps of Engineers. IA.02-6

337

An Update ofthe U.S. Clean Coal Technology Demonstration Program Office of Fossil Energy, U.S. Department of Energy  

NLE Websites -- All DOE Office Websites (Extended Search)

3 Issue No. 4, Fat, ,991 3 Issue No. 4, Fat, ,991 An Update ofthe U.S. Clean Coal Technology Demonstration Program Office of Fossil Energy, U.S. Department of Energy Nine New Clean Coal Technology Projects Selected In Fourth Round of Competition Clean Coal Briefs Highlights ofthis past quarter of the Clean Coal Technology Demonstra- tion Program include the addition 01 nine new projects selected for funding under the fourth round of competition, a new $203 million cooperative agree- ment for a pressurized circulating flu- idized bed combustion plant in Des Moines, Iowa, and the kick-off of next year's planned fifth round with the announcement of public meetings (see separate stories for details). The 42 government-industry projects now in the Clean Coal Pro- gram family-with a total value ex-

338

 

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

B1.32 Traffic flow adjustments, existing roads B1.32 Traffic flow adjustments, existing roads 1) Reimbursement for the cost of preparing the energy efficiency and conservation strategy, 2) perform energy audits to benchmark the energy performance of municipal buildings and fund public education/outreach campaign, 3) revolving loan program for energy efficiency retrofits and incremental costs for purchasing hybrid vehicles, 4) establish a mortgage buy-down program for residential buildings, 5) energy efficiency window retrofits at City Hall and the Police Station, 6) fund program to increase cycling and walking opportunities in the city Energy Efficiency and Conservation Block Program Energy Audit, Revolving Loan Program, Mortgage Buy-down Program, EE Retrofits, and Fund Program Des Moines Iowa

339

Western Governors Association Technical advisory Group  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

performance cleanup closure performance cleanup closure M E Environmental Management WIPP Update William (Bill) Mackie bill.mackie@wipp.ws July 24, 2007 Kansas City, Missouri safety performance cleanup closure 2 M E Environmental Management Total Shipments (as of 7/17/07) Contact Handled 5,928 Remote Handled 41 Total 5,969 safety performance cleanup closure 3 M E Environmental Management Argonne National Laboratory Shipment Campaign * Anticipate starting shipping in November 2007 * FY-2008 Projected Shipment Profile - Nov 07 2 Mar 08 2 - Dec 07 2 Apr 08 2 - Jan 08 2 May 08 2 - Feb 08 2 Jun 08 2 * Road Show scheduled for week of August 20 th . Begin at ANL, stop at Des Moines, IA; Lincoln, NE; Grand

340

Obama Administration Announces More Than $16 Million for Energy Projects in  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

16 Million for Energy 16 Million for Energy Projects in Iowa Obama Administration Announces More Than $16 Million for Energy Projects in Iowa June 22, 2009 - 12:00am Addthis Des Moines, IA - U.S. Department of Energy Secretary Steven Chu today announced more than $16 million in American Recovery and Reinvestment Act funding to support energy efficiency and renewable energy projects in Iowa. Under DOE's State Energy Program, states have proposed statewide plans that prioritize energy savings, create or retain jobs, increase the use of renewable energy, and reduce greenhouse gas emissions. This initiative is part of the Obama Administration's national strategy to support job growth, while making a historic down payment on clean energy. "This funding will provide an important boost for state economies, help put

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


341

Top U.S. Energy Department Official Visits Iowa, Calls on Congress to  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Energy Department Official Visits Iowa, Calls on Congress Energy Department Official Visits Iowa, Calls on Congress to Extend Clean Energy Tax Credits Top U.S. Energy Department Official Visits Iowa, Calls on Congress to Extend Clean Energy Tax Credits July 25, 2012 - 2:42pm Addthis News Media Contact (202) 586-4940 WASHINGTON - Today, Under Secretary for Energy (Acting) and Assistant Secretary for Policy & International Affairs, David Sandalow traveled to Iowa to highlight President Obama's strategy to develop every source of American energy. During his trip, Under Secretary Sandalow toured Keystone Electrical Manufacturing Company in Des Moines and ACCIONA Windpower's wind turbine generator assembly plant in West Branch, Iowa - two companies in the wind energy supply chain that are benefitting from federal tax credits for renewable energy generation. The Production Tax

342

Making Stuff Outreach at the Ames Laboratory and Iowa State University  

SciTech Connect

The U. S. Department of Energy's Ames Laboratory in Ames, Iowa was a coalition partner for outreach activities connected with NOVA's Making Stuff television series on PBS. Volunteers affiliated with the Ames Laboratory and Iowa State University, with backgrounds in materials science, took part in activities including a science-themed Family Night at a local mall, Science Cafes at the Science Center of Iowa, teacher workshops, demonstrations at science nights in elementary and middle schools, and various other events. We describe a selection of the activities and present a summary of their outcomes and extent of their impact on Ames, Des Moines and the surrounding communities in Iowa. In Part 2, results of a volunteer attitude survey are presented, which shed some light on the volunteer experience and show how the volunteers participation in outreach activities has affected their views of materials education.

Ament, Katherine; Karsjen, Steven; Leshem-Ackerman, Adah; King, Alexander

2011-04-01T23:59:59.000Z

343

Reply to comment | OSTI, US Dept of Energy, Office of Scientific and  

Office of Scientific and Technical Information (OSTI)

Reply to comment Reply to comment Slide22 Submitted by gibsone on Fri, 2013-08-30 06:35 FY2011-Anderson Slide22 Spotlighting: .EDUconnections http://www.osti.gov/EDUconnections/ * OSTI "spotlights" individual universities and community colleges committed to supporting and advancing the U.S. Department of Energy's scientific research programs at DOE Laboratories and Scientific User Facilities. * Some Spotlights from the past year: - University of Illinois (Exceptional Students) Fermi Lab Connection. - Jackson State University (Science and Educational Initiatives) ORNL Connection. - Princeton University PPPL Connection. - Des Moines Area Community College (Research Feature) Ames Laboratory Connection. Add new comment Original Thumbnail Mobile_320x340 Icon_64x64 Reply (If you're a human, don't change the following field)

344

Chemical Abundances in Twelve Red Giants of the Large Magellanic Cloud from High-Resolution Infrared Spectroscopy  

E-Print Network (OSTI)

High-resolution infrared spectra (R=50,000) have been obtained for twelve red-giant members of the LMC with the Gemini South 8.3-meter telescope plus Phoenix spectrometer. Quantitative chemical abundances of carbon-12, carbon-13, nitrogen-14, and oxygen-16 were derived from molecular lines of CO, CN, and OH, while sodium, scandium, titanium, and iron abundances were derived from neutral atomic lines. The LMC giants have masses from about 1 to 4 solar masses and span a metallicity range from [Fe/H]= -1.1 to -0.3. The program red giants all show evidence of first dredge-up mixing, with low 12C/13C ratios, and low 12C correlated with high 14N abundances. Comparisons of the oxygen-to-iron ratios in the LMC and the Galaxy indicate that the trend of [O/Fe] versus [Fe/H] in the LMC falls about 0.2 dex below the Galactic trend. Such an offset can be modeled as due to an overall lower rate of supernovae per unit mass in the LMC relative to the Galaxy, as well as a slightly lower ratio of supernovae of type II to supernovae of type Ia.

V. V. Smith; K. H. Hinkle; K. Cunha; B. Plez; D. L. Lambert; C. A. Pilachowski; B. Barbuy; J. Melendez; S. Balachandran; M. S. Bessell; D. P. Geisler; J. E. Hesser; C. Winge

2002-08-22T23:59:59.000Z

345

SOFTWARE Open Access Cloud-scale RNA-sequencing differential  

E-Print Network (OSTI)

.ibm.com/ibm/ideasfromibm/us/google/index.shtml]. 21. Magellan | Argonne's DOE Cloud Computing. [http://magellan.alcf.anl.gov/ ]. 22. Pickrell JK

Leek, Jeffrey

346

Universit Paris XIII U.F.R. des Lettres, des Sciences de l'Homme et des Socits  

E-Print Network (OSTI)

-rartl-mnd-iopo-iopl-mnd-hm-pr-ht-pr-hl-iop-ho-ihm-h-abdo-sopo-opo-cl Fig.4.Continued © 2011 The Authors

Paris-Sud XI, Université de

347

V-Durabilit des cramiques et des verres Ce chapitre se propose de traiter de la tenue long terme des cramiques et des verres.  

E-Print Network (OSTI)

61. Nelson, D. C. Oil Shale: New Technologies Defining New Opportunities. Presented at the Platts I, II Modeling of the In-Situ Production of Oil from .',1 l ',".1" Oil Shale ilil 'I' 'I~ :' l of conventional oil reserves amidst increasing liquid fuel demand in the world have renewed interest in oil shale

348

Le nom des naksatrani en tibetain  

E-Print Network (OSTI)

drug ma drug bu, mang po skyes k?ttik?s agni ? maewX? *mmru? 2 snar ma skye dguvi bdag po, dal bavi lha ldan ma, bi rdzi rohi?? (br?hm?) praj?- pati ? pjit ? *pit 3 mgo mgo skyes, smal bo, zla skyes, ri dwags mgo m?ga?iras (?grah?ya??) soma ? tsje... gi lha mo sv?t? v?yu ? khangH ? *kkha?-s 14 sa ga brgyad ldan ma, dbang povi lha ldan vi??khe (r?dh?) indr?gn? ? tej ? *ttij 15 lhamtshams mdza bo anur?dh?s mitra ? bjang ? *ba? Revue dEtudes Tibtaines 6 16 snron gang bu, ldevu, lha ldan, lha...

Jacques, Guillaume

2007-01-01T23:59:59.000Z

349

Leseabschrift Studiengangsordnung (Satzung) fr Studierende des Bachelorstudienganges  

E-Print Network (OSTI)

. Allgemeine Chemie und im zweiten Semester die Module 1. Organische Chemie 2. Physik II § 5 Besondere1100-MLS Allgemeine Chemie 3V + 1? + 4P 10 A K, M, T LS1600-MLS Organische Chemie 3V + 1? + 4P 10 A K, M, T LS2300 Biophysikalische Chemie 4V + 1? + 3P 10 A K, M, T LS2600 Biologische Chemie 3V 4 A K, M

Groppe, Jinghua

350

Leseabschrift Studiengangsordnung (Satzung) fr Studierende des Bachelorstudienganges  

E-Print Network (OSTI)

. Allgemeine Chemie und im zweiten Semester die Module 1. Organische Chemie 2. Physik II § 5 Besondere 4 V + 1 S 6 A K, M MZ3000 Mikrobiologie 2V + 2P 6 A K, M, T LS1100-MLS Allgemeine Chemie 3V + 1? + 4P 10 A K, M, T LS1600-MLS Organische Chemie 3V + 1? + 4P 10 A K, M, T LS2301 Biophysikalische Chemie

351

Advanced DES System Evaluation Interim Report  

Science Conference Proceedings (OSTI)

A portfolio of electric energy storage options is emerging that provides electric utilities with new options for grid support and operational flexibility. This research and development (RD) project was initiated to assess and test an emerging zinc-bromine (Zn-Br) flow battery in an electric distribution system and to provide input on a utility application specification. This technology is based on a flow battery developed by Exxon in the 1970s and '80s and is now being advanced and commercialized by Prem...

2009-05-19T23:59:59.000Z

352

ACADEMrrE ROUMAThffi REVUE ROUMAINE DES  

E-Print Network (OSTI)

(fuel) exhaustion for Nuclear Reactors (NR) need to be discussed for some centuries. The fact of some NPPHC equipped with Nuclear Reactors (NRs) CANDU type from PHWR (Pressurized Heavy Water Reactor installation (NPSP) producing steam, containing the Nuclear Reactor (NR), a power unit with turbine operated

Baica, Malvina

353

NOUVELLES ACQUISITIONS DES BIBLIOTHQUES DE LA  

E-Print Network (OSTI)

direitos humanos, também exige o repúdio à onda de pornografia, drogas, violência, desrespeito à vida em

Schibler, Ueli

354

LISTE ALPHABTIQUE DES 3058 BAYONNAIS INTRA MUROS  

E-Print Network (OSTI)

Jacques Droault chaudronnier Mr Drouilhet ainé me voilier M. Drouilhet puisné Pre Drouille M. chirurgien

Paris-Sud XI, Université de

355

TABLE DES MATIRES MOT DU DIRECTEUR ...........................................................................................................3  

E-Print Network (OSTI)

Cotruvo and Associates, LLC The Coutu Foundation Cox Broadcasting Jim Cox Jr. Foundation Charles R. Crisp

Charette, André

356

Lehrer des Jahres kommt aus Wilhelmshaven  

E-Print Network (OSTI)

durch ihre geographische Lage für den Ausbau der Offshore- Windenergie an. Schon jetzt arbei- ten hier- PowerCluster ein. Er optimiert die Industrialisierungsprozesse im Be- reich Offshore-Windenergie, ver (BMBF) hat die Bewerbung für den Wind- PowerCluster von ForWind, dem Fraunhofer-Institut für Windenergie

Habel, Annegret

357

CNRS UMR 7039 Facult des Sciences  

E-Print Network (OSTI)

(Intelligent Control-Maintenance-technical Management Systems) formalisant la connaissance générique, de niveau, this goal can be implemented by CMMS (integrated Control, Maintenance and technical Management System synthesized and developed into ICMMS (Intelligent Control-Maintenance-Management System)[Wang 1999][Zhang 1999

Paris-Sud XI, Université de

358

s des sries de fractions rationnelles - Springer  

Science Conference Proceedings (OSTI)

x seer un ensemble d'dpaisseur circulaire I au point a, 2 sur une pleine dpaisseur ra- dime de sommet a. Le th6or~me I[ est une proposition d'Analysis Situs,...

359

Eine Forschungsanstalt des ETH-Bereichs  

E-Print Network (OSTI)

. Energie Ziel ist die Umwandlung der derzeitigen, auf fossilen Brennstoffen beruhenden Energiewirtschaft

Wehrli, Bernhard

360

Eine Forschungsanstalt des ETH-Bereichs  

E-Print Network (OSTI)

The GESIMA emission inventory for the FLUMOB episode was prepared by the IER (Institut f¨ur Energiewirtschaft

Wehrli, Bernhard

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


361

Eine Forschungsanstalt des ETH-Bereichs  

E-Print Network (OSTI)

.11.-11.11.11 Globale und regionale Rohstoff- und Energiewirtschaft aus geographischer Sicht 18.11.-19.11.11 Auf dem Weg

Wehrli, Bernhard

362

Eine Forschungsanstalt des ETH-Bereichs  

E-Print Network (OSTI)

, Germany d Institut fu¨r Energiewirtschaft und Rationelle Energieanwendung (IER), Universita¨t Stuttgart

Wehrli, Bernhard

363

Eine Forschungsanstalt des ETH-Bereichs  

E-Print Network (OSTI)

niedersächsischen Kompetenzen entlang der gesamten Wertschöpfungskette der Energiewirtschaft zusammenzuführen und

Wehrli, Bernhard

364

Eine Forschungsanstalt des ETH-Bereichs  

E-Print Network (OSTI)

Energiewirtschaft und Rationelle Energieanwendung (IER), Stuttgart, Germany. Lamarque, J.-F., Brasseur, G. P., Hess

Wehrli, Bernhard

365

Eine Forschungsanstalt des ETH-Bereichs  

E-Print Network (OSTI)

, Energiewirtschaft und regenerative Energiequellen · Prozesse, Geräte und Maschinen zur Bereitstellung, Verteilung verarbeitender Systeme · Energieumwandlung · Energiewirtschaft · Bauen und Wohnen unter energetischen

Wehrli, Bernhard

366

2 Grundlagen und Hypothesen des Ansatzes ... - Springer  

Science Conference Proceedings (OSTI)

wissenschaftlich kaum erfasst werden knnen.110 Dies fhrt ferner dazu, dass der Staat als zentraler, wenngleich nicht als alleiniger Akteur bei der Schaffung...

367

Erfahrungen des Kreiskrankenhauses Greiz mit dem ...  

Science Conference Proceedings (OSTI)

der von ihnen erbrachten Leistungen verpflichtet. Die Leistungen miissen dem jeweiligen Stand der wissenschaftlichen Erkenntnisse entsprechen und in der.

368

Diplomarbeit zur Erlangung des akademischen Grades  

E-Print Network (OSTI)

Allgemeine Angaben 3 2 Zusammenfassung 5 3 Einführung 6 4 Arbeits- und Ergebnisbericht 7 4.1 Ausgangsfragen Blattleitfähigkeiten und Transpirationsraten vorgesehen. #12;- 7 - 4 Arbeits- und Ergebnisbericht 4.1 Ausgangsfragen- chungsjahren wissenschaftliche Hilfskräfte zum Einsatz. #12;- 12 - Für die Blattstiele wurde ein abgewandelter

369

Jahresbericht 2010 Vorwort des Prsidenten 3  

E-Print Network (OSTI)

Kraftwerke und den Ausbau der Netzinfrastruktur aufbringen muss. Der weltweite investitions- bedarf für neue gro?e Kohle- und 300 noch grö?ere Gas- kraftwerke ersetzen, auch der von diesen Kraft- werken Solar- kraftwerke natürlich nur wenig und nachts überhaupt keine Elektrizität. Daher muss

370

NOUVELLES ACQUISITIONS DES BIBLIOTHQUES DE LA  

E-Print Network (OSTI)

. Pawlik (Hrsg.), Handbuch Psychologie (S. 89-108). Heidelberg, Germany: Springer. Funke, J. & Spering, M solving]. In J. Funke (Hrsg.), Enzyklopädie der Psychologie, Serie 2, Kognition, Band 8: Denken und

Schibler, Ueli

371

Entwicklung des sterreichischen Wirtschaftsrechts in der Zweiten ...  

Science Conference Proceedings (OSTI)

Jahrhundert (1999); Gerlich/ Grande/ Mller (Hrsg), Sozialpartnerschaft in der Krise (1985); Hrbek/ Nettesheim (Hrsg), Europische Union und mitgliedstaatliche...

372

Leseabschrift Studiengangsordnung (Satzung) fr Studierende des Bachelorstudienganges  

E-Print Network (OSTI)

Muttersprache nicht Deutsch ist, müssen das erfolgreiche Bestehen einer anerkannten Deutschprüfung nachweisen. Allgemeine Chemie und im zweiten Semester die Module 1. Organische Chemie 2. Physik II § 5 Besondere Mikrobiologie 2V + 2P 6 A K, M, T LS1100-MLS Allgemeine Chemie 3V + 1? + 4P 10 A K, M, T LS1600-MLS Organische

Groppe, Sven

373

Leseabschrift Studiengangsordnung (Satzung) fr Studierende des Bachelorstudienganges  

E-Print Network (OSTI)

Deutsch ist, müssen das erfolgreiche Bestehen einer anerkannten Deutschprüfung nachweisen. (4) Das Studium ersten Semester die Module 1. Analysis I 2. Biologie I 3. Physik I 4. Allgemeine Chemie und im zweiten Semester die Module 1. Organische Chemie 2. Physik II § 5 Besondere Zugangsvoraussetzungen zu

Groppe, Jinghua

374

Facult des Lettres INSTITUT Dr ETHNOLOGIE  

E-Print Network (OSTI)

of operation; and (d) flexibility to fuel changes. In a dry sorbent injection system, trona or sodium In a dry sorbent injection system, trona (Na2CO3·NaHCO3· 2H2O) or sodium bicarbonate (NaHCO3) is injected electrostatic precipitators or fabric filters. Figure 1: Raw Trona under Microscope The chemical reactions

Paris-Sud XI, Université de

375

Titel des Moduls: Hochspannungstechnik, Energieversorgungsnetze und  

E-Print Network (OSTI)

, liebe Kollegen, das thema,,energie" - gekennzeichnet z.B. durch die Schlagworte,,energiewende","erneuerbare Glasmacher "eRneueRBARe eneRGie iSt Die ZuKunft" Herrmann Scheer #12; energie und Gebäude ­ ieg, GSO nürnberg www.ieg.ohm-hochschule.de wolfram

Wichmann, Felix

376

UNIVERSITE LIBRE DE BRUXELLES Faculte des Sciences  

E-Print Network (OSTI)

TCE trichloroethene or trichloroethylene TCLP toxic characteristic leaching procedure (RCRA) TDS total

Van Den Eijnden, Eric

377

2012 Regional Conference Sponsorship Packages  

Science Conference Proceedings (OSTI)

... in conference e-mail marketing your organization's ... $7,500 exclusive (available in Arizona only) ... Moines, IA September 28, 2012 | Scottsdale, AZ

2012-09-08T23:59:59.000Z

378

Facult des arts et des sciences Service d'appui la formation interdisciplinaire  

E-Print Network (OSTI)

-175-7-4 Multimédia LINGUISTIQUE ET TRADUCTION 1-180-2-0 Majeure en linguistique 5 décembre à 13h30 3200 Jean- Brillant B-3325 http://www.ling.umontreal.ca/ 1-180-4-0 Mineure en linguistique 1-147-1-5 Bac. litt. langue française-linguistique 1-183-1-0 Bac. linguistique-psychologie 1-182-4-0 Mineure en sciences cognitives

Charette, André

379

Sujet: cole doctorale Sciences et Technologies de lInformation, des Tlcommunications et des Systmes  

E-Print Network (OSTI)

Coordination du rglage de la frquence entre plusieurs systmes lectriques non-synchrones relis par un rseau courant continu haute tension (Frequency control coordination among non-synchronous AC areas connected by a multi-terminal HVDC grid)

Thse De Doctorat; Prsente Par; Jing Dai; Mme Anne-marie Denis; Rseau De Transport Delectricit; La Dfense

2013-01-01T23:59:59.000Z

380

La naissance des toilesLa naissance des toiles Echelles de masses?  

E-Print Network (OSTI)

labsence de barrière (au début...): ! g = " GM r2 ! 1 2 g tcl 2 ~ r ! g ~ G"r tcl ~ 0.3 G" r M #12;104 105

Sicardy, Bruno

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


381

Donna Calhoun Laboratoire d'Etudes des Transferts et de Mechanique des Fluides  

E-Print Network (OSTI)

. · "Simulating potential hydrogen explosions in nuclear reactor containment buildings", SIAM Com- putational Peak Over-pressures in explosions in nuclear reactor con- tainment facilities", SIAM Numerical Saclay, France. Division of Nuclear Energy. Research engineer in computational fluids and mechanics group

Calhoun, Donna

382

Centrales au gaz et Energies renouvelables: comparer des pommes avec des pommes  

E-Print Network (OSTI)

prix fixe. Cest ce que fait Xcel Energy, densemble. Danspourraient suivre lexemple de Xcel Energy au Minne- sota toutes les formes dnergie, Xcel Energy oblige que les

Bolinger, Mark; Wiser, Ryan; Golove, William

2003-01-01T23:59:59.000Z

383

INSTITUT DES SCIENCES ET TECHNOLOGIES cole doctorale no 432 : Sciences des mtiers de l'ingnieur  

E-Print Network (OSTI)

, collector design, simple systems 7. Nuclear Energy - basic principles, the CANDU reactor Dr. W. Hallett, CBY

384

Facult des arts et des sciences Service d'appui la formation interdisciplinaire  

E-Print Network (OSTI)

universitaires Jean-Coutu S1-151 www.crim.umontreal.ca/1-065-4-0 Mineure en criminologie 1-066-5-1 Certificat en-Montpetit : 2910, boul. ?douard-Montpetit Pavillon Claire-McNicoll 2900, boul. ?douard-Montpetit Pavillon Jean-Coutu

Charette, André

385

Mthode de test sans fil en vue des SIP et des SOC.  

E-Print Network (OSTI)

??Aujourd'hui le test de fabrication de circuits intgrs au niveau wafer s'appuie sur une technologie par contact entre l'quipement de test et les circuits (more)

Noun, Ziad

2010-01-01T23:59:59.000Z

386

Studienjahr 2012/2013 Medizin des Alterns und des alten Menschen (Geriatrie)  

E-Print Network (OSTI)

Hilfsmittel") Weiterführende Litera- tur: Platt D (Hrsg.): Altersmedizin. Schattauer Verlag, Stuttgart, New York, 1997 (ca. 900 Seiten) Nikolaus T (Hrsg.): Klinische Geriatrie, Springer Verlag, Berlin, 2000 (ca

Manstein, Dietmar J.

387

UNIVERSIT CADI AYYAD UNIVERSIT DU SUD TOULON-VAR FACULT DES SCIENCES FACULT DES SCIENCES  

E-Print Network (OSTI)

. Charlie Matulka, who lost to Senator Chuck Hagel of Nebraska the same year, does not trust the results- counting machines, which happen to have been manufactured by a company Mr. Hagel used to run. Mr. Matulka, against Mr. Matulka, he won more than 80 percent of the vote. What gets conspiracy theorists excited

Paris-Sud XI, Université de

388

Railroad accident report: Head-on collision between Iowa Interstate Railroad Extra 470 West and Extra 406 East with release of hazardous materials near Altoona, Iowa, on July 30, 1988. Irregular report  

SciTech Connect

About 11:40 a.m. central daylight saving time on July 30, 1988, Iowa Interstate Railroad Ltd. (IAIS) freight trains Extra 470 West and Extra 406 East collided head on within the yard limits of Altoona, Iowa, about 10 miles east of Des Moines, Iowa. All 5 locomotive units from both trains; 11 cars of Extra 406 East; and 3 cars, including two tank cars containing denatured alcohol, of Extra 470 West derailed. The denatured alcohol, which was released through the pressure relief valves and the manway domes of the two derailed tank cars, was ignited by the fire resulting from the collision of the locomotives. Both crew members of Extra 470 West were fatally injured; the two crew members of Extra 406 East were only slightly injured. The estimated damage (including lading) as a result of this accident exceeded $1 million. The major safety issues in the accident include operational methods employed by the IAIS, training and selection of train and engine personnel, supervisory oversight by the IAIS, design of closure fittings on hazardous materials rail tanks, and oversight of regional railroads by the Federal Railroad Administration.

Not Available

1989-07-06T23:59:59.000Z

389

The Midwest Power PCFB demonstration projects: AHLSTROM PYROFLOW[reg sign] first and second generation pressurized circulating fluidized bed (PCFB) technology  

SciTech Connect

Midwest Power, Dairyland Power Cooperative, Pyropower Corporation (a subsidiary of Ahlstrom Pyropower Inc.), and Black Veatch, have embarked on the demonstration of Clean Coal Technology (CCT) at Midwest Power's Des Moines Energy Center (DMEC), in Pleasant Hill, Iowa. The DMEC-1 PCFB Demonstration Project was selected by the US Department of Energy for the demonstration of the First Generation Pressurized Circulating Fluidized Bed (PCFB) Technology. During Round 5 of the CCT Program, Midwest Power submitted a proposal for a second unit, to be known as DMEC-2. If selected by the DOE, the DMEC-2 unit will demonstrate Ahlstrom Pyropower's Second Generation (Advanced) PCFB technology which will incorporate a topping combustor fired on coal derived gas generated in a PCFB carbonizer, to raise the firing temperature of the gas turbine and the total net plant efficiency. The First Generation PCFB technology has the capability to achieve 40--42% efficiency, the Second Generation technology can obtain an efficiency in the range of 44--47% net. This paper will provide a comparison of the commercial versions of the First and Second Generation PCFB systems, and the plans for demonstrating these systems for repowering and new plant installations during the late 1990's and into the next century. A discussion of the DMEC-1 and DMEC-2 projects and their key technical features will be provided together with a projection of the future markets for these advanced clean coal technologies.

Ambrose, S.; Green, C.L.; Dryden, R.; Provol, S.J.

1993-01-01T23:59:59.000Z

390

The Midwest Power PCFB demonstration projects: AHLSTROM PYROFLOW{reg_sign} first and second generation pressurized circulating fluidized bed (PCFB) technology  

SciTech Connect

Midwest Power, Dairyland Power Cooperative, Pyropower Corporation (a subsidiary of Ahlstrom Pyropower Inc.), and Black & Veatch, have embarked on the demonstration of Clean Coal Technology (CCT) at Midwest Power`s Des Moines Energy Center (DMEC), in Pleasant Hill, Iowa. The DMEC-1 PCFB Demonstration Project was selected by the US Department of Energy for the demonstration of the First Generation Pressurized Circulating Fluidized Bed (PCFB) Technology. During Round 5 of the CCT Program, Midwest Power submitted a proposal for a second unit, to be known as DMEC-2. If selected by the DOE, the DMEC-2 unit will demonstrate Ahlstrom Pyropower`s Second Generation (Advanced) PCFB technology which will incorporate a topping combustor fired on coal derived gas generated in a PCFB carbonizer, to raise the firing temperature of the gas turbine and the total net plant efficiency. The First Generation PCFB technology has the capability to achieve 40--42% efficiency, the Second Generation technology can obtain an efficiency in the range of 44--47% net. This paper will provide a comparison of the commercial versions of the First and Second Generation PCFB systems, and the plans for demonstrating these systems for repowering and new plant installations during the late 1990`s and into the next century. A discussion of the DMEC-1 and DMEC-2 projects and their key technical features will be provided together with a projection of the future markets for these advanced clean coal technologies.

Ambrose, S.; Green, C.L.; Dryden, R.; Provol, S.J.

1993-04-01T23:59:59.000Z

391

Improving the Field Performance of Natural Gas Furnaces, Chicago, Illinois (Fact Sheet)  

SciTech Connect

The objective of this project is to examine the impact that common installation practices and age-induced equipment degradation may have on the installed performance of natural gas furnaces, as measured by steady-state efficiency and AFUE. PARR identified twelve furnaces of various ages and efficiencies that were operating in residential homes in the Des Moines Iowa metropolitan area and worked with a local HVAC contractor to retrieve them and test them for steady-state efficiency and AFUE in the lab. Prior to removal, system airflow, static pressure, equipment temperature rise, and flue loss measurements were recorded for each furnace. After removal from the field the furnaces were transported to the Gas Technology Institute (GTI) laboratory, where PARR conducted steady-state efficiency and AFUE testing. The test results show that steady-state efficiency in the field was 6.4% lower than that measured for the same furnaces under standard conditions in the lab, which included tuning the furnace input and air flow rate. Comparing AFUE measured under ASHRAE standard conditions with the label value shows no reduction in efficiency for the furnaces in this study over their 15 to 24 years of operation when tuned to standard conditions. Further analysis of the data showed no significant correlation between efficiency change and the age or the rated efficiency of the furnace.

Rothgeb, S.; Brand, L.

2013-11-01T23:59:59.000Z

392

Biomass power for rural development. Quarterly report, October 3, 1998--January 1, 1999  

DOE Green Energy (OSTI)

Information and education activities for this quarter include both the monthly progress activities with some copies of materials developed and a copy of the annual report prepared for the Leopold Center for Sustainable Agriculture. The Leopold Center is a project partner and the primary sponsor of the information and education activities. The Leopold annual report references many prepared documents and assorted presentation materials. The Energy and Geological Resources Division of the Iowa Department of Natural Resources sponsors a meeting four times a year in order to bring members of the Iowa biomass energy community together to share information. In this quarter the Stakeholders meeting was held on October 21, 1998, in Des Moines Iowa. The first phase of the Geographic Information System (GIS) efforts have been completed and a final report with a map presentation of materials will be included in the next Quarterly Report. A meeting with Ed Gray of The Antares Group and project staff/cooperators was held October 23, 1998. The authors discussed the Niagara Project and the efforts to value the biomass material and partner contributions. Niagara has identified a value to the grid support capabilities of the dispersed generation.

Cooper, J.T.

1999-02-01T23:59:59.000Z

393

Arizona public service utility solar central receiver study: Volume 1, Phase 1 topical report  

Science Conference Proceedings (OSTI)

The Arizona Public Service Company (APS), in association with Black and Veatch (BandV), Babcock and Wilcox (BandW), Solar Power Engineering Company (SPECO), Pitt-DesMoines (PDM), and the University of Houston (UH), has completed Phase I of the Utility Solar Central Receiver Study. This study was co-funded by the US Department of Energy (DOE) under Cooperative Agreement Number DE-FC04-86AL38741. The Phase I effort focused on defining the most cost-effective solar thermal central receiver (STCR) power plant configuration for commercial utility application. A team led by Pacific Gas and Electric (PGandE) performed a similar parallel effort; in addition, the Alternate Utility Team (AUT) under APS management completed work for Phase I to support the overall effort. By the conclusion of Phase I, the utilities had reached consensus on the key technical issues for the STCR technology and had performed assessments of the technology which showed similar and favorable economic potential in the commercial utility market. Furthermore, APS and PGandE have agreed to an integrated approach for Phase II to assess and mitigate key risk issues on the path to commercializing the technology. This topical report documents the Phase I efforts; a separate Phase II report will be submitted upon completion of Phase II. 114 figs., 74 tabs.

Not Available

1988-11-01T23:59:59.000Z

394

Lessons from Iowa : development of a 270 megawatt compressed air energy storage project in midwest Independent System Operator : a study for the DOE Energy Storage Systems Program.  

DOE Green Energy (OSTI)

The Iowa Stored Energy Park was an innovative, 270 Megawatt, $400 million compressed air energy storage (CAES) project proposed for in-service near Des Moines, Iowa, in 2015. After eight years in development the project was terminated because of site geological limitations. However, much was learned in the development process regarding what it takes to do a utility-scale, bulk energy storage facility and coordinate it with regional renewable wind energy resources in an Independent System Operator (ISO) marketplace. Lessons include the costs and long-term economics of a CAES facility compared to conventional natural gas-fired generation alternatives; market, legislative, and contract issues related to enabling energy storage in an ISO market; the importance of due diligence in project management; and community relations and marketing for siting of large energy projects. Although many of the lessons relate to CAES applications in particular, most of the lessons learned are independent of site location or geology, or even the particular energy storage technology involved.

Holst, Kent (Iowa Stored Energy Plant Agency, Traer, IA); Huff, Georgianne; Schulte, Robert H. (Schulte Associates LLC, Northfield, MN); Critelli, Nicholas (Critelli Law Office PC, Des Moines, IA)

2012-01-01T23:59:59.000Z

395

Nutrient Requirements Of Swine  

E-Print Network (OSTI)

no. 119, Midwestern Section meeting of the American Society of Animal Science, Des Moines, IA. Trotter, M., and C. L. Allee. 1979a. Availability of phosphorus in corn, soybean meal and wheat. J. Anim. Sci. 49(Suppl. 1):255 (Abstr.). Trotter, M., and G. L. Allee. 1979b. Availability of phosphorus in dry and high-moisture grain for pigs and chicks. J. Anim. Sci. 49(Suppl. 1):98 (Abstr.). Trotter, M., and G. L. Allee. 1979c. Effects of steam pelleting and extruding sorghum grain-soybean meal diets on phosphorus availability for swine. J. Anim. Sci. 49(Suppl. 1):255 (Abstr.). Tucker, H. F., and W. D. Salmon. 1955. Parakeratosis or zinc deficiency disease in the pig. Proc. Soc. Exp. Biol. Med. 88:613--616. Tunmire, D. L., D. E. Orr, Jr., and L. F. Tribble. 1983. Ammonium polyphosphate vs. dicalcium phosphate as a phosphorus supplement for growing-finishing swine. J. Anim. Sci. 57:632--637. Ullrey, D. E. 1992. Basis for regulation of selenium supplements in animal diets. J. Anim. Sci. ...

Tenth Revised Edition; Board On Agriculture

1998-01-01T23:59:59.000Z

396

Direct Distances to Cepheids in the Large Magellanic Cloud: Evidence for a Universal Slope of the Period-Luminosity Relation up to Solar Abundance  

E-Print Network (OSTI)

We have applied the infrared surface brightness (ISB) technique to derive distances to 13 Cepheids in the LMC which span a period range from 3 to 42 days. From the absolute magnitudes of the variables calculated from these distances, we find that the LMC Cepheids define tight period-luminosity relations in the V, I, W, J and K bands which agree exceedingly well with the corresponding Galactic PL relations derived from the same technique, and are significantly steeper than the LMC PL relations in these bands observed by the OGLE-II Project in V, I and W, and by Persson et al. in J and K. We find that the tilt-corrected true distance moduli of the LMC Cepheids show a significant dependence on period, which hints at a systematic error in the ISB technique related to the period of the stars. We identify as the most likely culprit the p-factor which converts the radial into pulsational velocities; our data imply a much steeper period dependence of the p-factor than previously thought, and we derive p=1.58 (+/-0.02) -0.15 (+/-0.05) logP as the best fit from our data, with a zero point tied to the Milky Way open cluster Cepheids. Using this revised p-factor law, the period dependence of the LMC Cepheid distance moduli disappears, and at the same time the Milky Way and LMC PL relations agree among themselves, and with the directly observed LMC PL relations, within the 1 sigma uncertainties. Our main conclusion is that the previous, steeper Galactic PL relations were caused by an erroneous calibration of the p-factor law, and that there is now evidence that the slope of the Cepheid PL relation is independent of metallicity up to solar metallicity, in both optical, and near-infrared bands.

W. Gieren; J. Storm; T. G. Barnes III; P. Fouque; G. Pietrzynski; F. Kienzle

2005-03-29T23:59:59.000Z

397

The ARAUCARIA project: Deep near-infrared survey of nearby galaxies. I. The distance to the Large Magellanic Cloud from K-band photometry of red clump stars  

E-Print Network (OSTI)

We have obtained deep imaging in the near-infrared J and K bands for 2 nearby fields in the bar of the LMC with the ESO NTT telescope, under exquisite seeing conditions. The K, J-K color-magnitude diagrams constructed from these data are of outstanding photometric quality and reveal the presence of several hundreds of red clump stars. Using the calibration of Alves for the K-band absolute magnitude of Hipparcos-observed red clump stars in the solar neigbourhood we derive a distance modulus to our observed LMC fields of 18.487 mag. Applying a correction for the tilt of the LMC bar with respect to the line of sight according to the geometrical model of van der Marel et al., the corresponding LMC barycenter distance is 18.501 mag. If we adopt a K-band population correction of -0.03 mag, as done by Alves et al. 2002, to account for the difference in age and metallicity between the solar neighborhood and LMC red clump star populations, we obtain an LMC barycenter distance modulus of 18.471 mag from our data. This is in excellent agreement with the result of Alves et al., and of another very recent study of Sarajedini et al. (2002) obtained from K-band photometry. However, we emphasize that current model predictions about the uncertainties of population corrections seem to indicate that errors up to about 0.12 mag may be possible, probably in any photometric band. Therefore, work must continue to tighten the constraints on these corrections. We also determine the mean red clump star magnitude in our LMC fields in the J band, which could be a useful alternative to the K band should future work reveal that population effect corrections for red clump stars in the J band are smaller, or more reliably determined than those for the K band.

G. Pietrzynski; W. Gieren

2002-08-07T23:59:59.000Z

398

Hermeneutique des Tantra : les Six extremes (ou possibilites alternatives) (satkoti ; mtha' drug). A propos d'un exemple de pregnance des modeles exegetiques des sutra  

E-Print Network (OSTI)

deux ornements ont pour fonction assigne, selon Tsong kha pa (1357-1419), de commenter la pense [ou lintention (dgongs pa ; abhiprya)] du tantra-racine12. Mais, alors que lesQuatre modes dexplication sont exclusivement utiliss pour les tantra... , Collge de France, Institut de Civilisation Indienne, 1978, p. 15). Bu ston rin chen grub (1290-1364) et Tsong kha pa (1357-1419) utilisent cette grille pour commenter le troisime et le quatrime ornement (v. A. Wayman, The Buddhist Tantras, Light...

Arenes, Pierre

2002-01-01T23:59:59.000Z

399

Le paysage comme reprsentation spaciale : le paysage viticole comme symbole des indications de provenance des vins des rgions Vale dos Vinhedos, Pinto Bandeira et Monte Belo (Brsil).  

E-Print Network (OSTI)

??Le sujet de cette thse est le paysage dans sa spcificit viticole analyse comme reprsentation spatiale dans le processus de construction de l'espace gographique de (more)

Falcade, Ivanira

2011-01-01T23:59:59.000Z

400

La diffrence entre la russite des garons et des filles l'cole : reprsentations de sexe, solutions et pratiques ducatives des enseignant.e.s du secondaire .  

E-Print Network (OSTI)

??Dans cette thse de matrise, nous avons tent de rpondre la question de recherche suivante : quelles sont les reprsentations de sexe que les (more)

Grenier, Vronique

2013-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


401

I/O Performance of Virtualized Cloud Environments  

E-Print Network (OSTI)

consistency. On systems such as NERSC, often there are twoMagellan compute resources at NERSC. Magellan is a 720 nodeagainst a high-speed NERSC file-system, Global Scratch. This

Ghoshal, Devarshi

2013-01-01T23:59:59.000Z

402

Texas - State Energy Profile Data - U.S. Energy Information ...  

U.S. Energy Information Administration (EIA)

ATA, Chevron, Citgo, Coastal, Conoco, DSE, Explorer, Exxon, Koch, Longhorn, Magellan, Mobil, Navajo, Phillips, Pride, Shell, Sigmor, SFPP, TEPPCO, Texaco, ...

403

Effects of Ca2+ on supramolecular aggregation of natural organic matter in aqueous  

E-Print Network (OSTI)

timeframe ­ Began joint Argonne/NERSC Magellan cloud project ­ Delivered 897M core hours of science 2010

Kalinichev, Andrey G.

404

Des Plaines, Illinois: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Plaines, Illinois: Energy Resources Plaines, Illinois: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 42.0333623°, -87.8833991° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":42.0333623,"lon":-87.8833991,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

405

A propos des toponymes de l'epopee de Gesar  

E-Print Network (OSTI)

, 35a, 37a, 38a,49a-b, 50b, 52a-b, 53b, 57a-b, 58a, 68a, 77a ; III, 14a-b, 17a-b, 22b, 24b, 27b,55b, 69b, 78a-b, 85b, 103a. DN : I : 12, 29, 30, 31, 37, 63, 83, 94, 95. II : 158. III :219.Ge mdzo Ri bo dbang zhu : Ge mdzo "Montagne Arc... -en-Ciel", variante deGer mdzo Ri dmar dbang zhu (qv) : DN : III : 172.Ger mdzo Ri dmar dbang zhu : Ger mdzo (parfois Ge mdzo) "MontagneRouge, Arc-en-ciel", v. aussi Ri dmar dbang zhu, Ge mdzo Ri bo dbang zhuet gNyan ri. Montagne gnyan du pays de rMa, prs de Klu ri...

Chayet, Anne

2003-01-01T23:59:59.000Z

406

Acadmie de Paris cole des Hautes tudes Internationales  

E-Print Network (OSTI)

problems, SIAM Journal on Optimization, Vol. 12, No. 4, pp. 1126­1146, 2002. [30] BASESCU, V. L Polytechnic Institute, Troy, NY 12180, August 2003. [31] BASESCU, V. L., and MITCHELL, J. E., An analytic

407

CALENDRIER D'VALUATION PRIODIQUE DES PROGRAMMES D'TUDES  

E-Print Network (OSTI)

.E.S.S. (informatique) (2-175-1-1) · Ph. D. (informatique) (3-175-1-0) Département de linguistique et traduction · B.A. en linguistique (1-180-1-0) · Majeur en linguistique (1-180-2-0) · Mineur en linguistique (1.A. en littératures de langue française et linguistique (1-147-1-0) · B.A. en linguistique et psychologie

Charette, André

408

La structure argumentale des nominalisations prdicatives Florence Lefeuvre*  

E-Print Network (OSTI)

poliment à Dominique Sopo si son association « n'a pas participé à la confusion dans laquelle nous vivons

409

Journal de Theorie des Nombres de Bordeaux 20 (2008), ixi  

E-Print Network (OSTI)

elle a ´et´e brillamment re¸cue, partageant la premi`ere place avec une condisciple. L'Inspection G avril 1979 (r´ef´erences [1] `a [4]). qui lui a permis de devenir Professeur `a l'Universit´e de

Martinet, Jacques

410

UNIVERSITE DE CORSE PASQUALE PAOLI FACULTE DES SCIENCES ET TECHNIQUES  

E-Print Network (OSTI)

the electricity you can produce with a solar PV array or wind turbine at your home or business. www.nrel.gov/eis farms are sited; sun must shine on solar farms; feedstock crops must grow for bioenergy; hot rocks velocity, solar irra- diation, precipitation, subsurface temperatures, stream flow) directly related

Paris-Sud XI, Université de

411

Distribution et association des inversions chromosomiques dans trois populations naturelles  

E-Print Network (OSTI)

, one on each of the major autosome arms, are cosmopolitan. The Tunisian popu- lation shows the greatest distribution of cosmopolitan inversions between individuals of the French population is observed in the Tunisian lines. Linkage disequilibrium exists between pair of cosmopolitan inversions of the #12;second

Recanati, Catherine

412

UNIVERSITE PARIS-SUD HABILITATION `A DIRIGER DES RECHERCHES  

E-Print Network (OSTI)

Open Cyc Open Corpo- rates Open Calais OpenEI Open Election Data Project Open Data Thesau- rus Ontos

413

Andrieu Bernard Pr. Epistmologie du corps et des pratiques corporelles  

E-Print Network (OSTI)

.. Modifier son corps, pourquoi ?, Paris, Ed La Martinière, 2009. 23 Pièces et main d'oeuvre, RIFD : la police

Paris-Sud XI, Université de

414

tudes conomtriques rcentes ralises partir des donnes de la CFTC  

E-Print Network (OSTI)

Light Sweet Crude Oil, et complètent celles qui étaient précédemment disponibles sur le site de la CFTC. Publication de la Deutsche Bank (2009) La note de la Deutsche Bank « Do speculators drive crude oil prices'auteur remercie également tous les experts consultés à cette occasion à la CFTC, US Treasury, US Department

Paris-Sud XI, Université de

415

Le Reseau des mille dieux et demons : mythes et classifications  

E-Print Network (OSTI)

, listes de huit, dans un ordre diffrent : lha, bdud, btsan, rgyal po, gnod sbyin, ma mo, the'u rang, klu). Par ailleurs, d'autres classes sont rpertories : hybride comme les klu btsan, sous-classes comme les ya bdud et les ma bdud, sp- cifiques... pour celle de gTing skyes par Khyentse Rinpoche, T pour celle de mTshams brag dont deux versions seront examines ici : celle en 53 chapitres (T53) et celle en 86 chapitres (T86). En fait, les versions "en 53 chapitres" en contiennent 54 car elles...

Blondeau, Anne-Marie

2008-01-01T23:59:59.000Z

416

Dissertation zur Erlangung des Doktorgrades der Fakultt fr Angewandte  

E-Print Network (OSTI)

. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 183 11.1.1 Conclusions and Intermediate Results that led to the Final MiSP Invariants . . 184 11 important advan- tages over other approaches like fluorescence spectra (Takahashi et al., 2000), antibody

417

Calmodulin-vermittelte Desensitisierung des olfaktorischen CNG-Kanals.  

E-Print Network (OSTI)

??Das Riechsystem erlaubt Tieren unter einer Vielzahl von Duftstoffen zu unterscheiden, was der Nahrungssuche, aber auch der Identifikation von Partnern oder Feinden, dient. Die Desensitisierung (more)

Ungerer, Nicole

2009-01-01T23:59:59.000Z

418

Advice to the beginner College de France, Institut des Hautes  

E-Print Network (OSTI)

'' manner, a small part of the mathematical world, as esoteric as it can look at first 1 , their trip can

Connes, Alain

419

Table des matires Pour obtenir le grade de  

E-Print Network (OSTI)

.sciencedirect.com RAPID COMMUNICATION Silicon-conductive nanopaper for Li-ion batteries Liangbing Hua,1 , Nian Liub,1 July 2012; received in revised form 14 August 2012; accepted 15 August 2012 KEYWORDS Li-ion battery-conductive nanopaper structure performs well as Li-ion battery anodes. A stable capacity of 1200 mA h/g for 100 cycles

Paris-Sud XI, Université de

420

Abschnitt Verpflichtung zum Handeln im besten Interesse des Kunden  

Science Conference Proceedings (OSTI)

Not logged in Google [Search Crawler] (3000811494) 66.249.75.90. Springer for Research & Development. UA-26408784-1. JavaScript is currently disabled,...

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


421

Origin and early history of Die Methode des Eichzusatzes or ...  

Science Conference Proceedings (OSTI)

... In practice, the sought amount of nickel may simply be read off the ... 16 presents a zinc determination: 5.4 mg Zn were present in a supporting ...

2011-07-15T23:59:59.000Z

422

Version du 8 octobre 2008 Table des matires  

E-Print Network (OSTI)

: however, it may by accident fall out, that some of the Consonants shall be oftener found in an Epistle

Le Meur, Anne-Françoise

423

ECOLE DES HAUTES ETUDES EN SCIENCES SOCIALES Formation doctorale  

E-Print Network (OSTI)

, and Optimization , in : Algorithms For Robotic Motion and Manipulation, J.-P. Laumond and M. Overmars (Eds.), A.K

Paris-Sud XI, Université de

424

Dpartement de gomatique applique Facult des lettres et sciences humaines  

E-Print Network (OSTI)

. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 63 3.1.1 Creating MODTRAN Input Files . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 64 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 314 C Horizon Calculator 317 C.1 Determine the MODTRAN horizon . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 317 C.2 The Function getModtran

425

HABILITATION DIRIGER DES RECHERCHES UMR 6134 -Universit de Corse  

E-Print Network (OSTI)

Henri BALBI, Examinateur Nicola BELLOMO, Rapporteur Didier BRESCH, Rapporteur Tomas CHACON REBOLLO de Corse (6134), dont je remercie le directeur Jacques Henri Balbi et les membres de m'y avoir

Paris-Sud XI, Université de

426

CONCIERGE-SERVICE ANGEBOTE UND LEISTUNGEN DES CONCIERGE-SERVICE  

E-Print Network (OSTI)

alle haushaltsnahen und handwerklichen Bereiche rund um Haus und Garten. Das sind insbesondere: Boten. Beratung ­ Wir sind Ansprechpartner für alle Fragen rund um Haus und Garten. Transparenz ­ Wir

Heermann, Dieter W.

427

Simulation et aide au dimensionnement des chaudires de rcupration.  

E-Print Network (OSTI)

??Heat recovery steam generators (HRSG) play a very important role in combined cycle (CC) power plants, where steam is generated from a gas turbine exhaust (more)

Dumont, Marie-Noelle

2007-01-01T23:59:59.000Z

428

Microsoft Word - NT42951PrelimDesCkean.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

Sleeve positions the Liner in the box tool joint. Sleeve material is currently type 360 Brass. Insulation: The Insulation is the most critical component of the IDP design. The...

429

www.sas-atw.com | ATW - Liste des catalogues  

U.S. Energy Information Administration (EIA)

We observed that sas-atw.com website has been registered on 2/17/2009 12:00:00 AM during our researches. sas-atw.com website opens slow with 81 ms ping time.

430

DES and Differential Power Analysis (The "Duplication" Method)  

Science Conference Proceedings (OSTI)

Paul Kocher recently developped attacks based on the electric consumption of chips that perform cryptographic computations. Among those attacks, the "Differential Power Analysis" (DPA) is probably one of the most impressive and most difficult to avoid.In ...

Louis Goubin; Jacques Patarin

1999-08-01T23:59:59.000Z

431

BAS DU SPECTRE ET GEOMETRIE DES VARIETES DE VOLUME INFINI.  

E-Print Network (OSTI)

??Cette thse tudie les varits non compactes dont le bas du spectre du Laplacien est une valeur propre isole. L'objectif gnral est de relier la (more)

Tapie, Samuel

432

prsente L'ECOLE NATIONALE DES PONTS ET CHAUSSEES  

E-Print Network (OSTI)

Research Center (NERPC) Southborough, MA 87 308 Harvard Depository Petersham, MA 2,867 73 Harvard Forest

Paris-Sud XI, Université de

433

Optimisation exergoconomique des systmes de trignration d'nergie.  

E-Print Network (OSTI)

??Voir rsum tendu en franais en fin de thse. In the actual energetic and economic context, energy polygeneration represents the answer regarding the efficient use (more)

Tirca-Dragomirescu, Georgiana

2012-01-01T23:59:59.000Z

434

Universit de Cergy-Pontoise Habilitation Diriger des Recherches  

E-Print Network (OSTI)

Operating Schedule Planning Schedule (subject to change) The HFIR Operating cycle length over the past 22 Mar Apr May Operation Outage Complete Milestone HFIR Operating Forecast & Planning Schedule Tue 12 May Operation Outage Complete Milestone HFIR Operating Forecast & Planning Schedule Tue 12/18/12 #12;

435

Synthse des travaux et activits scientifiques prsente par  

E-Print Network (OSTI)

1 ESnet Update Summer 2007 Joint Techs Workshop Joe Burrescia ESnet General Manager July 16) Singaren ESnet IP core: Packet over SONET Optical Ring and Hubs ELP commercial peering points MAE-E PAIX-PA Equinix, etc. PNWGPoP/PAcificWave ESnet 3 with Sites and Peers (Early 2007) ESnet core hubsIP Abilene high

436

Microsoft Word - FY12 Fee Des.doc  

National Nuclear Security Administration (NNSA)

REQUIREMENTS FOR DOE NUCLEAR FACILITIES 06-01-11 IB 430.1 Rev 0 LIFE CYCLE ASSET MANAGEMENT 08-11-98 IB 430.1B-100 Rev 0 REAL PROPERTY ASSET MANAGEMENT 08-11-98 IB 433.1-126...

437

Mesure des missions gazeuses au stockage de lisier porcin  

E-Print Network (OSTI)

followed in the steps of the Ministry of Energy and approved 60% of energy related project (mostly biogas

Paris-Sud XI, Université de

438

Laboratoire de Physique des Interfaces et Couches Minces LPICM...  

Open Energy Info (EERE)

of the Ecole Polytechnique in France, focussing on silicon based thin-films and nano materials, large area electronic applications, as well carbone nanotubes. Coordinates...

439

L'utilisation des hydro-jecteurs au CERN  

E-Print Network (OSTI)

Les jecteurs buse variable sont destins remplacer les vannes trois voies conventionnelles et les pompes secondaires de circulation dans les installations de chauffage eau chaude et de conditionnement d'air. Ces jecteurs liquide - liquide utilisent l'nergie d'un fluide primaire pour maintenir le dbit d'un fluide secondaire grce un saut de pression. L'utilisation de ces jecteurs permet notamment de rduire les co ts d'investissement, de consommation nergtique et aussi de maintenance. Cette technique qui a fait ses preuves depuis plus de 20 ans, est abondamment utilise en Allemagne, Italie et Belgique (50 000 boucles) et peu dans d'autres pays comme la France (500 boucles). Au CERN, aucune application d'hydro-jecteur de ce type n'a encore t mise en oeuvre ce jour. Ce document prsente cette technique en dtail avec ses avantages, ses inconvnients et ses possibles applications.

Deleval, S

2002-01-01T23:59:59.000Z

440

FIPS 46-3, Data Encryption Standard (DES) (withdrawn May ...  

Science Conference Proceedings (OSTI)

... 5131 of the Information Technology Management Reform Act of 1996 ... EEROM), and mainframe computers using Random Access Memory (RAM). ...

2012-12-12T23:59:59.000Z

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


441

Rechenschaftsbericht 2007 des Prsidiums der Humboldt-Universitt zu Berlin  

E-Print Network (OSTI)

.3 Anwendungsperspektiven. . . . . . . . . . . . . . . . . . . . . . . . . . . . 8 4 Arbeits- und Ergebnisbericht 10 4.3 Wissenschaftliche Mitarbeiter/in Dipl.-Ing. Vera Ebbing Besch¨aftigungszeitraum: seit 1. Oktober 2006 1.4 Fachgebiet;Zwischenbericht zum DFG-Forschungsvorhaben NE 902/2-1 SCHR 570/6-1 10 4 Arbeits- und Ergebnisbericht Basierend auf

Röder, Beate

442

wie vielfach zu lesen war, das ,,Ende des rheinischen  

E-Print Network (OSTI)

AG Degussa AG Daimler-Benz AG Wacker-Chemie GmbH Bayer AG Hoechst AG Deutsche Bank AG Daimler-Benz AG Projektverbund ,,Das deutsche System der Arbeitsbeziehungen un- ter dem Einfluss der Internationalisierung". Der zunehmende Internationalisierung die deutsche Wirtschaft? Wie verändert sie das Spannungsfeld zwischen

443

Studiengangsordnung (Satzung) fr Studierende des Bachelorstudienganges Molecular Life Science  

E-Print Network (OSTI)

Prüfungsverfahren befindet. (3) Bewerber, deren Muttersprache nicht Deutsch ist, müssen das erfolgreiche Bestehen. Analysis I 2. Biologie I 3. Physik I 4. Allgemeine Chemie und im zweiten Semester die Module 1. Organische Chemie 2. Physik II § 5 Besondere Zugangsvoraussetzungen zu Lehrveranstaltungen (1) Für den Besuch

Groppe, Jinghua

444

REPRAGE DES INDICATEURS DE CRISES RCURRENTES ET INDITES  

E-Print Network (OSTI)

. Wattiaux, J.C. Grenier andM. Pouchard, Sol. StateCommun., 9 1 0 , (1994) 501-507. 1171 J.C. Park, P.C. Johnston, A. Rigamonti and D.R. Torgeson, Physica C, 235-240, (1994) 1717-1723. [23] J-C. Grenier, N The Electrochemical Oxidation: a New Way for Preparing Highly Oxidized Ferrites J.-C. Grenier, A. Wattiaux, L. Foumes

Paris-Sud XI, Université de

445

EI0534_Techniken des Energy Harvesting_110608.xls Allgemeine Daten  

E-Print Network (OSTI)

Vibration energy harvesting from random force and motion excitations This article has been) 075025 (9pp) doi:10.1088/0964-1726/21/7/075025 Vibration energy harvesting from random force and motion A vibration energy harvester is typically composed of a spring­mass system with an electromagnetic

Kuehnlenz, Kolja

446

Microsoft Word - NT42951PrelimDesCkean.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

07 07 Project No. NT42951 Electronic File Name: NT42951PD.pdf Topical Report Preliminary Design of Insulated Drill Pipe for High Temperature, High Pressure Drilling Principal Authors: Al T. Champness Anthony J. Worthen John T. Finger Report Issued: February 1, 2007 DOE Award No.: DE-FC26-06NT42951 Submitted By: Drill Cool Systems, Inc. 627 Williams St. Bakersfield, CA 93305 i Disclaimer: This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus,

447

Liste des documentaires et des films de fiction disponibles la Mdiathque J.-A.-DeSve Mise jour : Avril 2011  

E-Print Network (OSTI)

'énergies renouvelables en 2020 [20% renewable energy by 2020 / 20% erneuerbare Energien im Jahr 2020] DVD 1350 206329 Blood : the last vampire DVD 0691 Blow out DVD1906 Blow-up RVI5698 The blue angel DVD2035 Blue

Charette, André

448

Les boursiers du Dpartement l'occasion des concours 2012-2013 des grands organismes subventionnaires (CRSH,  

E-Print Network (OSTI)

(linguistique) Fonds d'améliorations à la vie étudiante (FAVE) Nicolas Bourguignon (doctorat, linguistique) Luc (linguistique) Elena Dimova (linguistique) Jaïmé Dubé (linguistique) Cecilia Foglia (traduction) Kornebari Kumbe (traduction) Elena Nikilaeva Dimova (linguistique) Annaïch LeSerrec (traduction) Paula Andrea Montoya Arango

Parrott, Lael

449

Longueur de diffusion des porteurs minoritaires et structure de jonction des diodes Cu/Cu2O (*)  

E-Print Network (OSTI)

short circuit current and with the shift from cell to cell of the peak in the photovoltaic spectral cells are not sui- table for an efficient photovoltaic solar energy conversion. Revue Phys. Appl. 15, the photovoltaic spectrum and the electron beam induced current (EBIC) methods. In the two last cases, Cu/Cu2O

Paris-Sud XI, Université de

450

FACULT des ARTS et des SCIENCES -DPARTEMENT de CHIMIE SIGLE du COURS: CHM 6310 NOM DU PROFESSEUR: A. CHARETTE  

E-Print Network (OSTI)

méthode de Durst (Tet. Lett. 1995, 36, 2559-2562). Un seul diastéréoisomère de l'amine est obtenu lorsque of the most clever way to make an optically active -amino acid is to use Durst methodology (Tet. Lett. 1995

Charette, André

451

Universit de Pau et des Pays de l'Adour Ecole Doctorale des Sciences Exactes et de leurs Applications  

E-Print Network (OSTI)

for crops in the field, if farmer have available biogas tank, and liquid has been used for gas generating who use biogas effluents on the cultures jus- tify it more by the advantages of biogas itself than by qualities of effluent biogas product. Indeed, the inter- viewed people underlined the hygienic pro

Paris-Sud XI, Université de

452

L'archive comme enjeu de prsentation de soi : la mmoire du syndicat des ouvriers des savonneries Naplouse, Cisjordanie  

E-Print Network (OSTI)

-754, U.Bossel, Oberrohrdorf, Switzerland (1994) [10] F. Mauvy, C. Lalanne, J-M. Bassat, J-C. Grenier, H.C. Grenier Institut de Chimie de la Matière Condensée de Bordeaux (ICMCB-CNRS) Université de Bordeaux 1, Av-P.Manaud, P.Dordor and J-C.Grenier, "Oxygen electrode reaction on Nd2NiO4+ cathode materials: impedance

Paris-Sud XI, Université de

453

Welcome to the Efficient Windows Collaborative  

NLE Websites -- All DOE Office Websites (Extended Search)

Window Selection Tool: New Construction Windows Window Selection Tool: New Construction Windows The Window Selection Tool will take you through a series of design conditions pertaining to your design and location. It is a step-by-step decision-making tool to help determine the most energy efficient window for your house. SELECT LOCATION: AK Anchorage AK Fairbanks AL Birmingham AL Mobile AR Little Rock AZ Flagstaff AZ Phoenix AZ Tucson CA Arcata CA Bakersfield CA Daggett CA Fresno CA Los Angeles CA Red Bluff CA Sacramento CA San Diego CA San Francisco CO Denver CO Grand Junction CT Hartford DC Washington DE Wilmington FL Daytona Beach FL Jacksonville FL Miami FL Tallahassee FL Tampa GA Atlanta GA Savannah HI Honolulu IA Des Moines ID Boise IL Chicago IL Springfield IN Indianapolis KS Wichita KY Lexington KY Louisville LA Lake Charles LA New Orleans LA Shreveport MA Boston MD Baltimore ME Portland MI Detroit MI Grand Rapids MI Houghton MN Duluth MN Minneapolis MO Kansas City MO St. Louis MS Jackson MT Billings MT Great Falls NC Raleigh ND Bismarck NE Omaha NH Concord NJ Atlantic City NM Albuquerque NV Las Vegas NV Reno NY Albany NY Buffalo NY New York OH Cleveland OH Dayton OK Oklahoma City OR Medford OR Portland PA Philadelphia PA Pittsburgh PA Williamsport RI Providence SC Charleston SC Greenville SD Pierre TN Memphis TN Nashville TX Brownsville TX El Paso TX Fort Worth TX Houston TX Lubbock TX San Antonio UT Cedar City UT Salt Lake City VA Richmond VT Burlington WA Seattle WA Spokane WI Madison WV Charleston WY Cheyenne AB Edmonton MB Winnipeg ON Toronto PQ Montreal SELECT HOUSE TYPE:

454

JC3 High Impact Assessment Bulletins | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

1, 2013 1, 2013 V-059: MoinMoin Multiple Vulnerabilities Multiple vulnerabilities have been reported in MoinMoin, which can be exploited by malicious users to conduct script insertion attacks and compromise a vulnerable system and by malicious people to manipulate certain data. December 31, 2012 V-058: Microsoft Internet Explorer CDwnBindInfo Object Reuse Flaw Lets Remote Users Execute Arbitrary Code A vulnerability was reported in Microsoft Internet Explorer. A remote user can cause arbitrary code to be executed on the target user's system. December 27, 2012 V-056: FreeType BDF Glyph Processing Buffer Overflow Vulnerability Several vulnerabilities were reported in FreeType. A remote user can cause arbitrary code to be executed on the target user's system. December 25, 2012

455

Chariton Valley Biomass Project Final Environmental Assessment and Finding of No Significant Impact  

DOE Green Energy (OSTI)

Switchgrass is a warm-weather, native Iowa grass that grows well on marginal land. It has been identified and extensively studied for its potential as a biomass energy crop, especially its potential for use as co-fire feedstock in coal-burning plants. In this environmental assessment (EA), the term ''co-fire'' refers to the burning of switchgrass in the OGS boiler in conjunction with coal, with the goal of reducing the amount of coal used and reducing emissions of some objectionable air pollutants associated with coal combustion. The U.S. Department of Energy (DOE) is proposing to provide partial funding for (1) the design and construction of a biomass (switchgrass [Panicum virgatum]) storage, handling, and conveying system into the boiler at the Ottumwa Generating Station (OGS) near Chillicothe, Iowa; (2) operational testing of switchgrass as a biomass co-fire feedstock at OGS; and (3) ancillary activities related to growing, harvesting, storing, and transporting switchgrass in areas of the Rathbun Lake watershed. Chillicothe is in Wapello County on the south side of the Des Moines River, approximately 16 kilometers (10 miles) northwest of Ottumwa, Iowa, and 130 kilometers (80 miles) southeast of Des Moines. The OGS is a 725-megawatt (MW) maximum output, low-sulfur, pulverized coal-burning plant jointly owned by several Iowa utilities and operated by Alliant Energy. The plant is located about 1.6 kilometers (1 mile) northwest of Chillicothe, Iowa, on the Des Moines River. The following three-phase switchgrass co-fire test campaign has been planned and partially implemented at OGS: During Phase 1, which occurred from November 2000 through January 2001, Alliant Energy conducted Co-fire Test 1 at OGS. Phase 2 testing, the Proposed Action, would consist of two additional co-fire tests. Co-fire Test 2, which would utilize some residual equipment from Co-fire Test 1 and also test some new equipment, is currently planned for September/October 2003. It would be designed to test and demonstrate the engineering and environmental feasibility of co-firing up to 11.3 tonnes (12.5 tons) of switchgrass per hour and would burn a maximum of 5,440 tonnes (6,000 tons) of switchgrass. Co-fire Test 3, which is tentatively planned for winter 2004/2005, would test the long-term (approximately 2,000 hours) sustainability of processing 11.3 tonnes (12.5 tons) per hour. Co-fire Test 3 would be conducted using a proposed new process building and storage barn that would be constructed at the OGS as part of the Proposed Action. Phase 3, commercial operations, may occur if Phase 2 indicated that commercial operations were technically, environmentally, and economically feasible. Continuous, full-scale commercial operations could process up to 23 tonnes (25 tons) of switchgrass per hour, generate 35 MW per year of OGS's annual output, and replace 5 percent of the coal burned at OGS with switchgrass. Chariton Valley Resource Conservation and Development Inc. (Chariton Valley RC&D), a rural-development-oriented, non-profit corporation (Chariton Valley RC&D 2003a) and Alliant Energy would implement Phase 3 at their discretion after the completion of the Phase 2 co-fire tests. DOE's Proposed Action would support only Phase 2 testing; that is, Co-fire Tests 2 and 3. DOE has no plans to provide financial support for the commercial operations that would be performed during Phase 3. The new construction that DOE proposes to partially fund would include a new switchgrass processing facility and equipment and a new storage barn that would be used for Co-fire Test 3. This environmental assessment (EA) evaluates the environmental impacts that could result from the Proposed Action. It also evaluates the impacts that could occur if DOE decided not to partially fund the Proposed Action (the No Action Alternative). No other action alternatives are analyzed because (1) no generating plants other than OGS have the installed infrastructure and operating experience necessary to conduct Phase 2 co-fire testing, and (2) the Rathbun Lake watershed is the only viable

N /A

2003-07-11T23:59:59.000Z

456

Shane Canon  

NLE Websites -- All DOE Office Websites (Extended Search)

File: ioperformance.pdf (pdf: 174 KB) We compare the IO performance using IOR benchmarks on two cloud computing platforms - Amazon and the Magellan cloud testbed. Lavanya...

457

Berkeley Lab Selects IBM Technology to Power Cloud Computing...  

NLE Websites -- All DOE Office Websites (Extended Search)

of Energy (DOE). The Magellan system will be a testbed for National Energy Research Scientific Computing Center (NERSC) scientists to explore the effectiveness of cloud computing...

458

Optical observations of afterglows of gamma ray bursts localized by the high energy transient explorer.  

E-Print Network (OSTI)

??In this thesis, I discuss observations of the optical afterglows of seven HETE GRBs, carried out mainly with the Magellan Telescopes at Las Campanas Observatory (more)

Dullighan, Allyn, 1978-

2004-01-01T23:59:59.000Z

459

Scientists Look to the Clouds to Solve Complex Questions | U...  

Office of Science (SC) Website

factor in floor space, power demands, and staff support," said Yelick. The Department of Energy is tackling this challenge with the Magellan project, a research and development...

460

Scientists Studying Photosynthesis to Generate Electricity  

NLE Websites -- All DOE Office Websites (Extended Search)

supercomputers to investigate photosynthetic materials May 15, 2012 | Tags: Carver, Energy Technologies, HPSS, Magellan NERSC Contact: Linda Vu, lvu@lbl.gov, +1 510 495 2402...

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


462

Technique d'auto test pour les imageurs CMOS.  

E-Print Network (OSTI)

??Le test en production des imageurs CMOS est ralis avec des testeurs qui utilisent des sources de lumire prcises, aussi bien au niveau du test (more)

Lizarraga, L.

463

Quelques prcisions concernant les cours au choix. En plus des cours obligatoires (OB) et des cours option (OP), les programmes de premier  

E-Print Network (OSTI)

1215 - Civilisation espagnole ITL1120 - Introduction à la culture italienne Linguistique LNG1955 - Notions générales de linguistique LNG2011 - Courants théoriques en linguistique Littérature comparée LCO

Parrott, Lael

464

ETUDES NUMERIQUES DES MECANISMES D'INTERACTION D'UN LASER IMPULSIONNEL AVEC DES MATERIAUX: APPLICATION A LA SYNTHESE DE NANO AGREGATS.  

E-Print Network (OSTI)

??La prsentation de mes activits de recherche et d'encadrement qui fait l'objet de ce document est organise autour de trois thmes scientifiques : - les (more)

Itina, Tatiana

2008-01-01T23:59:59.000Z

465

Supporting Advanced Scientific Computing Research Basic Energy Sciences Biological  

E-Print Network (OSTI)

· NERSC / LBNL · ALCF / ANL ­ Will provide multiple 10's of teraflops and multiple petabytes of storageNetwork Sunnyvale NYC Nashville Chicago OLCF/ ORNL 100G ALCF/ANL NERSC Magellan Magellan 6 #12;ARRA/ANI Testbed (Oakland, CA) and ALCF (Argonne, IL) 9 #12;Network Testbed Components · Network Testbed will consist of

466

National Ignition Facility Target Chamber  

DOE Green Energy (OSTI)

On June 11, 1999 the Department of Energy dedicated the single largest piece of the National Ignition Facility (NIF) at Lawrence Livermore National Laboratory (LLNL) in Livermore, California. The ten (10) meter diameter aluminum target high vacuum chamber will serve as the working end of the largest laser in the world. The output of 192 laser beams will converge at the precise center of the chamber. The laser beams will enter the chamber in two by two arrays to illuminate 10 millimeter long gold cylinders called hohlraums enclosing 2 millimeter capsule containing deuterium, tritium and isotopes of hydrogen. The two isotopes will fuse, thereby creating temperatures and pressures resembling those found only inside stars and in detonated nuclear weapons, but on a minute scale. The NIF Project will serve as an essential facility to insure safety and reliability of our nation's nuclear arsenal as well as demonstrating inertial fusion's contribution to creating electrical power. The paper will discuss the requirements that had to be addressed during the design, fabrication and testing of the target chamber. A team from Sandia National Laboratories (SNL) and LLNL with input from industry performed the configuration and basic design of the target chamber. The method of fabrication and construction of the aluminum target chamber was devised by Pitt-Des Moines, Inc. (PDM). PDM also participated in the design of the chamber in areas such as the Target Chamber Realignment and Adjustment System, which would allow realignment of the sphere laser beams in the event of earth settlement or movement from a seismic event. During the fabrication of the target chamber the sphericity tolerances had to be addressed for the individual plates. Procedures were developed for forming, edge preparation and welding of individual plates. Construction plans were developed to allow the field construction of the target chamber to occur parallel to other NIF construction activities. This was necessary to achieve the overall schedule. Plans had to be developed for the precise location and alignment of laser beam ports. Upon completion of the fabrication of the aluminum target chamber in a temporary structure the 130 ton sphere was moved from the temporary construction enclosure to its final location in the target building. Prior to the installation of a concrete shield and after completion of the welding of the chamber penetrations vacuum leak checking was performed to insure the vacuum integrity of target chamber. The entire spherical chamber external surface supports a 40 cm thick reinforced concrete shield after installation in the target building. The final task is a total survey of the laser ports and the contour machining of spacer plates so that laser devices attached to these ports meet the alignment criteria.

Wavrik, R W; Cox, J R; Fleming, P J

2000-10-05T23:59:59.000Z

467

Process performance of Ahlstrom Pyroflow PCFB pilot plant  

Science Conference Proceedings (OSTI)

Ahlstrom Pyropower has designed and built a 10 MW[sub th] (34 MMBtu) pressurized circulating fluidized bed (PCFB) pilot plant in Karhula, Finland. The unit is now operating. Data from this unit supports the design of a nominal 80 MW, Des Moines Energy Center 1 (DMEC-1) PCFB Repowering Project. The pilot plant PCFB combustor is of square cross-section. It is housed in a 3.6 m (11.8 ft) diameter pressure vessel. A high pressure high temperature gas cleaning unit downstream of the PCFB exhaust is installed in a separate 2.6 m (8.5 ft) diameter pressure vessel. The maximum plant operating pressure is 16 bar (232 psia). The fuel is fed in slurry form; sorbent is also fed along with the fuel. The net heat input per unit cross section of the combustor is the highest of any known combustion mode. The heat release can go up to 40 MW/m[sup 2] (12.6 MMBtu/ft[sup 2] hr). Many types of coals including high sulfur, bituminous Illinois No. 6 coal and Western sub bituminous, low sulfur Powder River Basin coal were tested. Combustion efficiencies in the range of 99.5 to 99.9% have been consistently observed. Emissions of various gases such as NO[sub x] SO[sub 2] and CO at different operating pressures and loads were monitored. The gas emissions have been lower than expected based on atmospheric circulating fluidized bed boiler experience. The sulfur retention is over 95 % with a Ca/S molar ratio of 1 to 2 for high sulfur Illinois No.6 coal. A GAVS molar ratio of 2.5 to 3.5 was observed to retain 95 % of sulfur with low sulfur Powder River Basin coal. All gaseous emissions during testing with Illinois No. 6 coal and Powder River Basin coal are well within the projected limits for the DMEC1 project. Emission data from tests with Illinois No. 6 coal and Powder River Basin coal are presented in the paper.

Sellakumar, K.M. (R D Center, Ahlstrom Pyropower, Inc., San Diego, CA (United States)); Isaksson, J.; Tiensuu, J. (Ahlstroem Pyropower, Inc., Karhula (Finland). Hans Ahlstroem Lab.)

1993-05-01T23:59:59.000Z

468

Process performance of Ahlstrom Pyroflow PCFB pilot plant  

Science Conference Proceedings (OSTI)

Ahlstrom Pyropower has designed and built a 10 MW{sub th} (34 MMBtu) pressurized circulating fluidized bed (PCFB) pilot plant in Karhula, Finland. The unit is now operating. Data from this unit supports the design of a nominal 80 MW, Des Moines Energy Center 1 (DMEC-1) PCFB Repowering Project. The pilot plant PCFB combustor is of square cross-section. It is housed in a 3.6 m (11.8 ft) diameter pressure vessel. A high pressure high temperature gas cleaning unit downstream of the PCFB exhaust is installed in a separate 2.6 m (8.5 ft) diameter pressure vessel. The maximum plant operating pressure is 16 bar (232 psia). The fuel is fed in slurry form; sorbent is also fed along with the fuel. The net heat input per unit cross section of the combustor is the highest of any known combustion mode. The heat release can go up to 40 MW/m{sup 2} (12.6 MMBtu/ft{sup 2} hr). Many types of coals including high sulfur, bituminous Illinois No. 6 coal and Western sub bituminous, low sulfur Powder River Basin coal were tested. Combustion efficiencies in the range of 99.5 to 99.9% have been consistently observed. Emissions of various gases such as NO{sub x} SO{sub 2} and CO at different operating pressures and loads were monitored. The gas emissions have been lower than expected based on atmospheric circulating fluidized bed boiler experience. The sulfur retention is over 95 % with a Ca/S molar ratio of 1 to 2 for high sulfur Illinois No.6 coal. A GAVS molar ratio of 2.5 to 3.5 was observed to retain 95 % of sulfur with low sulfur Powder River Basin coal. All gaseous emissions during testing with Illinois No. 6 coal and Powder River Basin coal are well within the projected limits for the DMEC1 project. Emission data from tests with Illinois No. 6 coal and Powder River Basin coal are presented in the paper.

Sellakumar, K.M. [R& D Center, Ahlstrom Pyropower, Inc., San Diego, CA (United States); Isaksson, J.; Tiensuu, J. [Ahlstroem Pyropower, Inc., Karhula (Finland). Hans Ahlstroem Lab.

1993-05-01T23:59:59.000Z

469

d'ordre : 259-2009 Anne 2009 Influence des dfauts sur les proprits  

E-Print Network (OSTI)

LYON Discipline : Physique préparée au laboratoire de Physique dans le cadre de l'?cole Doctorale PHAST

470

UNIVERSITE MONTPELLIER I INSTITUT DES SCIENCES DE L'ENTREPRISE ET DU MANAGEMENT (ISEM)  

E-Print Network (OSTI)

; Porter, 1980 ; Heil & Robertson, 1991 ; Smith & al., 1992) ou le limit pricing (ou pratique de prix

Paris-Sud XI, Université de

471

THORIE D'IWASAWA DES REPRSENTATIONS DE DE RHAM D'UN CORPS LOCAL  

E-Print Network (OSTI)

.........................................................................................................................................1 2. Introduction to Critical Infrastructure and Key Resources (CIKR Resources (CIKR) models and simulations may be used to understand infrastructure systems interdependencies between CIKR systems. The goal of this document is to capture the current knowledge

Colmez, Pierre

472

Modles des contacts linguistiques dans lhistoire de la langue franaise.  

E-Print Network (OSTI)

??Cette recherche vise valuer l'ordre dans lequel les divers contacts linguistiques ont eu lieu dans l'histoire de la langue franaise. Nous confrontons d'abord quelques (more)

Amit, Aviv

2009-01-01T23:59:59.000Z

473

tude des pratiques linguistiques en camfranglais dans les centres urbains camerounais : le cas de Yaound.  

E-Print Network (OSTI)

??Mettant contribution les principes de la linguistique distributionnelle (aliments par les acquis de la smantaxe) et lapproche de la linguistique de corpus, cette tude (more)

Eloundou Eloundou, Venant

2011-01-01T23:59:59.000Z

474

RENTRE DES PERSONNELS Le 26 septembre, une runion de bienvenue a rassembl, salle  

E-Print Network (OSTI)

. Introduction à la linguistique théorique Benjamin SPECTOR Mercredi 17h-19h 45 rue d'Ulm : salle Cavaillès (1er de linguistique au second semestre : - ? partir du mardi 13 et mercredi 14 janvier de 10h30 à 12h30 : ECS11. Séminaire de linguistique théorique. Luigi RIZZI et Gennaro CHIERCHIA,Dominique SPORTICHE et

475

L'EXISTENCE DES LOIS : LES POUVOIRS CAUSAUX DANS LA NATURE Anjan Chakravartty  

E-Print Network (OSTI)

discours d'une manière purement linguistique (par opposition à une interprétation les prédicats. Par conséquent, nous devons distinguer une acceptation linguistique dispositif linguistique mais qu'il comporte une réelle signification ontologique

Chakravartty, Anjan

476

Planning des cours du Dpartement d'etudes cognitives Anne universitaire 2012-2013  

E-Print Network (OSTI)

3 Introduction à la linguistique Homer 6 Je 17-19 Salle 236 DEC-C02-S1 Introduction à la linguistique - TD Jeremy Zehr 4 Lu 15-17 235B DEC-CO3-S1 Introduction à la psychologie cognitive J.Sackur /T incluse). COURS DU MASTER DE LINGUISTIQUE à l'ENS DEC-B17-S2 Sémantique Intensive approches

Gutkin, Boris

477

cole doctorale nO Sciences des Mtiers de l'Ingnieur  

E-Print Network (OSTI)

Cell (SOFC) . . . . . . . . . . . . . . . . . . . . . . . . . . . 9 I.3.1 Advantages and Disadvantages . . . . . . . . . . . . . . . . . . . . . . 8 I.3 Solid Oxide Fuel Cell (SOFC) . . . . . . . . . . . . . . . . . . . . . 9 I.3.1 Advantages with delivering power from 10 kW to 2 MW have been tested. Solid Oxide Fuel Cell (SOFC) has dense mixed oxide

478

ED n 432 : Sciences des Mtiers de l'Ingnieur N attribu par la bibliothque  

E-Print Network (OSTI)

.................................................................................................................................................... 9 1.2.6 Working fluid and lubricating oil lubricated to avoid metal-to-metal contact, thus reducing energy losses and wear. #12;Chapter 1: Mobile Air that absorbs the lubricating oil that leaks through the shaft seal. The complexity of the shaft seal is related

Paris-Sud XI, Université de

479

Journal de Theorie des Nombres de Bordeaux 20 (2008), i--xi  

E-Print Network (OSTI)

elle a ??et??e brillamment re?cue, partageant la premi??ere place avec une condisciple. L'Inspection G??ese d' ?? Etat le 3 avril 1979 (r??ef??erences [1] ??a [4]). qui lui a permis de devenir Professeur ??a l

Martinet, Jacques

480

Journal de Th'eorie des Nombres de Bordeaux 20 (2008), i-xi  

E-Print Network (OSTI)

auquel elle a 'et'e brillamment re,cue, partageant la premi`ere place avec une condisciple. L'Inspection''Etat le 3 avril 1979 (r'ef'erences [1] `a [4]). qui lui a permis de d* *evenir Professeur `a l

Martinet, Jacques

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


481

Quoi de neuf? Une confrence runit au CERN des physiciens thoriciens du monde entier  

E-Print Network (OSTI)

On Monday 26 June Luciano Maiani, Director-General of CERN*, the European Organisation for Nuclear Research, opened the "Supersymmetry 2000" conference which is taking place at CERN in Geneva this week. Many of the world's top physicists are gathering to present their work and discuss possible signatures of new physics beyond the Standard Model of particle physics, such as novel particles and large extra dimensions of space, and the problem of energy in the vacuum, first raised by Einstein.

CERN Press Office. Geneva

2000-01-01T23:59:59.000Z

482

Entwurf und Implementation eines Expertensystems fr das Detektorkontrollsystem des ATLAS-Pixeldetektors  

E-Print Network (OSTI)

This thesis describes the design and implementation of an Expert System for the Detector Control System of the ATLAS Pixel Detector at the European center for particle physics, CERN. The ATLAS-Experiment is one of four big experiments installed at the Large Hadron Collider and is itself composed of multiple particle detectors. The innermost of these sub-detectors is the ATLAS Pixel detector, whose more than 30000 operating parameters impose high requirements on the hard- and software of the Detector Control System. In order to support the shift personnel during regular detector operation, an Expert System for the Detector Control System, which provides troubleshooting instructions, was developed within the scope of this work. To allow for a precise mapping of the available human experts knowledge to the Expert System, a rule based and easily adaptable system was designed. The use of the DIM protocol furthermore enables the adoption for other detectors or the data acquisition system. Special emphasis was pu...

Hen, Tobias

483

Water vapour effects in mass measurement LNE-INM : Conservatoire national des arts et mtiers  

E-Print Network (OSTI)

and an oil free pump associated to a turbo molecular pump. The working pressure range is between 1 Pa and standard atmosphere (105 Pa). The pressure inside the enclosure (vacuum pump shut off) goes from 1 Pa Airtightchamber Capacitive hygrometer Optical fibre Valve Pressure sensor Turbo molecular pump Diaphragm pump Near

Paris-Sud XI, Université de

484

Htrosexisme et le bien-tre des adolescents de mres lesbiennes.  

E-Print Network (OSTI)

??Les recherches comparatives entre les familles homoparentales et les familles htroparentales ont permis de montrer qu'il n'existe aucune diffrence statistique entre les enfants de familles (more)

Vyncke, Johanna

2009-01-01T23:59:59.000Z

485

ECOLE DES HAUTES ETUDES EN SCIENCES SOCIALES 2004 No. attribu par la bibliothqu  

E-Print Network (OSTI)

of Iran. There are other equally important stories about the Middle East and the worldwide Muslim commu to spur more sustainable economic development and growth throughout the Middle East. By lifting up of the Middle East into 21st-century global energy economies.As we look ahead to the coming decades

Paris-Sud XI, Université de

486

Les calcites de Fontainebleau : une cl pour dater la silicification des grs ?  

E-Print Network (OSTI)

as a model of a pile of sand. Now the problem of estimating y could be seen as the problem of ARTICLE the dissimilarity between the above conformations, let us suppose you must transfer the sand to one of the above such that By0 ðT? is tight and wclðBy0 ðT?? is contained in M. Then there is a py0 -null set N (which may

487

N: 2008-ENAM-0027 Ecole doctorale n 432 : Sciences des Mtiers de l'Ingnieur  

E-Print Network (OSTI)

LPSP loss of power supply probability MPPT maximum power point tracker NOCT nominal operating cell of the wind turbine is often interpolated from the tur- bine's power curve. This curve can be obtained feedback controller A dynamic model was created in Simulink with variable speed Cp and stall control

Paris-Sud XI, Université de

488

Concours Fermat Canada Canadian Team Honour Roll / Palmars des quipes l'chelle nationale  

E-Print Network (OSTI)

. IZMIR, TURKEY 9 14 RABBANI CYRUS ICAE TROY, MICHIGAN 8 14 SCHUELE JEFF ICAE TROY, MICHIGAN 8 13 INST. IZMIR, TURKEY 9 14 ZAMPANI MICHAEL ICAE TROY, MICHIGAN 8 13 Résultats internationaux INST. IZMIR, TURKEY 331 6 MATH TRAINERS GUILD PHILLIPINES QUIAPO MANILA, PHILLIPINES 330 7 INDIAN

Le Roy, Robert J.

489

Ecole doctorale n432 "Sciences des mtiers de l'ingnieur" N attribu par la bibliothque  

E-Print Network (OSTI)

......................................................................................26 4.4 Percentage Savings Relative to Baseline Energy Consumption.....................................................................28 Figure 4-4. Non-Coincident Peak Demand Savings (New York, New Jersey, California, Texas) account for 44% of market activity in our sample. Figure ES-2

Paris-Sud XI, Université de

490

Ecole Doctorale n432 Sciences des Mtiers de l'Ingnieur  

E-Print Network (OSTI)

....................................................................................... 44 2.2 Modélisation du stockage électrochimique ...........................................................................................134 4.4 Conclusion

Paris-Sud XI, Université de

491

Num ro d'ordre: 503 L'Institut National des Sciences Appliqu es de Toulouse  

E-Print Network (OSTI)

, op- timisation, contrainte, interface, Tcl/Tk. Laboratoire de G nie M canique de Toulouse (LGMT) D

Paris-Sud XI, Université de

492

Aktivierung und Desensibilsierung des olfaktorischen cAMP-gesteuerten-Kanal : Identifizerung von funktionellen Modulen.  

E-Print Network (OSTI)

??Der olfaktorische zyklisch-Nukleotid-gesteuerte Kanal (CNG-Kanal) wandelt in den Riechneuronen das chemische Duftstoffsignal in ein elektrisches Signal um und spielt somit eine wichtige Rolle bei der (more)

Prinz zu Waldeck, Clemens

2009-01-01T23:59:59.000Z

493

Advice to the beginner Coll`ege de France, Institut des Hautes Etudes  

E-Print Network (OSTI)

" manner, a small part of the mathematical world, as esoteric as it can look at first1 , their trip can

Connes, Alain

494

Prsente Universit du Maine U. F. R des Sciences et Techniques  

E-Print Network (OSTI)

, such as a hydrogen economy, greatly improved energy storage (batteries), fuel cells, nano-insulating foams for better

Paris-Sud XI, Université de

495

Prsente Universit du Maine U. F. R. des Sciences et Techniques  

E-Print Network (OSTI)

, including a gift from BASF for the lecture hall renovation, and in our scholarship drive. As always, we Michael Vance BASF Sherry L. Brewer Biogen Wendy Butterworth Joseph Lorenc Catalytica Leonard Nelson, Inc. Armstrong World Industries Ashland Chemical Company BASF Bayer Becton-Dickinson BOC Process

Paris-Sud XI, Université de

496

KIT-Jahresbericht KIT Universitt des Landes Baden-Wrttemberg und  

E-Print Network (OSTI)

for energy conversion and storage, such as fuel cells and batteries have a high potentiality to become key and components is the most important technological challenge that nowadays fuel cell and battery developers such as water electrolyzers and batteries are also discussed. tel-00740967,version1-11Oct2012 #12;10 tel

497

Collge doctoral ED n 432 : Sciences des Mtiers de l'Ingnieur  

E-Print Network (OSTI)

out battery safety tests. The BMBF is planning to set up a pilot produc- tion line for lithium ion batteries in Ulm within the framework of the Lithium Ion Batteries (KLiB) competence network, which Entwicklung effizienter Batterie- systeme befasst, an den Start. Für uns als Uni- versität Ulm ist diese

Paris-Sud XI, Université de

498

Transitions magntiques dans des alliages Pd-Co hydrogns B. Souffach et J. P. Burger  

E-Print Network (OSTI)

magnétiques du type verre de spin dans les alliages Pd-Co hydro- génés. Les températures d'ordre observées'abaisser considerablement la densite d'etats au niveau de Fermi car 1'electron ajoute par chaque atome d'hydrogene contribue hydro- g6nation du magnetisme d'alliages a base de Pd [5, 6]. Nous nous proposons surtout d'etendre nos

Paris-Sud XI, Université de

499

Institut de Minralogie et de Physique des Milieux Condenss UMR 7590 CNRS UPMC  

E-Print Network (OSTI)

in the vicinity of uranium mine tailings sites or for the safety assessment of potential high-level nuclear waste Spéciation de l'uranium dans l'environnement : Application aux opales de Nopal I (Mexique) et aux résidus nucléaires à haute activité. La spéciation de l'uranium, influencée par de nombreux facteurs biotiques ou

500

R\\'egularisation et optimisation pour l'imagerie sismique des fondations de pyl\\^ones  

E-Print Network (OSTI)

This research report summarizes the progress of work carried out jointly by the IRCCyN and the \\'Ecole Polytechnique de Montr\\'eal about the resolution of the inverse problem for the seismic imaging of transmission overhead line structure foundations. Several methods aimed at mapping the underground medium are considered. More particularly, we focus on methods based on a bilinear formulation of the forward problem on one hand (CSI, modified gradient, etc.) and on methods based on a "primal" formulation on the other hand. The performances of these methods are compared using synthetic data. This work was partially funded by RTE (R\\'eseau de Transport d'\\'Electricit\\'e), which has initiated the project, and was carried out in collaboration with EDF R&D (\\'Electricit\\'e de France - Recherche et D\\'eveloppement).

Vautrin, Denis; Idier, Jrme; Goussard, Yves

2010-01-01T23:59:59.000Z