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1

8JANVIER 2014 Direction DU PAtriMoine et Des services techniqUes  

E-Print Network [OSTI]

8JANVIER 2014 Direction DU PAtriMoine et Des services techniqUes Direction: régis cAPo Daniel NAHON Pôle espaces verts Jean-Luc GIULIANO Bernard D'AGOSTINO Pôle Parc automobile et téléphonie

Chamroukhi, Faicel

2

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

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump to:52c8ff988c1Dering Harbor, New York: Energy Resources Jump to:GruneDes

3

CX-006500: Categorical Exclusion Determination | Department of...  

Broader source: Energy.gov (indexed) [DOE]

Determination CX-006500: Categorical Exclusion Determination Magellan Des Moines Biodiesel Terminal Project CX(s) Applied: B5.1 Date: 09062011 Location(s): Des Moines, Iowa...

4

De moins en moins de pluies sur l'Amazonie  

E-Print Network [OSTI]

-temporelle des précipitations sur l'ensemble du bassin amazonien. Entre Andes et plaine amazonienne Six millions plaines, le climat varie beaucoup d'une région à l'autre. A partir de leur analyse, les chercheurs ont mis dans des Depuis les andes, où il trouve sa source, jusqu'à son embouchure dans l'atlantique, l

5

Des Moines, Washington: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump to:52c8ff988c1Dering Harbor, New York: Energy Resources Jump

6

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

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to:SeadovCooperative Jump to: navigation, search Name: West

7

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

Broader source: Energy.gov (indexed) [DOE]

the Iowa Office of Energy STATE: IA Independence) PROJECf TITLE: Magellan Des Moines Biodiesel Terminal Project Page 10f3 Funding Opportunity Announcement Number Procurement...

8

Recherches sur la rsistance des sols aux mala-dies. XV. Comparaison des populations de  

E-Print Network [OSTI]

le fer joue un rôle dans le mécanisme de résistance des sols de Chateaurenard. L'objet de cet article populations de Pseudomonas fluorescents du sol résistant de Chateaurenard et du sol sensible de Carque- fou sols de Chateaurenard semble réduite. Ils sont en effet moins nombreux en valeur relative et moins

Paris-Sud XI, Université de

9

Magellan Instant Camera testbed  

E-Print Network [OSTI]

The Magellan Instant Camera (MagIC) is an optical CCD camera that was built at MIT and is currently used at Las Campanas Observatory (LCO) in La Serena, Chile. It is designed to be both simple and efficient with minimal ...

McEwen, Heather K. (Heather Kristine), 1982-

2004-01-01T23:59:59.000Z

10

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

SciTech Connect (OSTI)

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

11

ISU College of Engineering/Des Moines Area Community College Transfer Plan  

E-Print Network [OSTI]

MAT 217 5 Phys 221 5 Classical Physics I PHY 213 6 *May also transfer for ABE 160, AerE 160, CE 160 AerE Aerospace Engineering CprE Computer Engineering AE Agricultural Engineering ConE Construction

Hu, Hui

12

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

Broader source: Energy.gov (indexed) [DOE]

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "ofEarly Career Scientists' ResearchThe Office ofReportingEnergy AdvancedAeroSysNNC_3-25.pdfDepartment of

13

Des Moines Area Community College | OSTI, US Dept of Energy, Office of  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: Vegetation Proposed Newcatalyst phasesData FilesShape, Density, and Morphology ofConvergenceScientific

14

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

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE:YearRound-Up from theDepartment(October-DecemberBasedToward a MoreA RisingA1A Touch of Green for

15

SEP Success Story: A Touch of Green for Des Moines' Sherman Hill |  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious RankCombustion | Department ofT ib l LPROJECTS IN7 Roadmap forDKT. NO. 14-98-LNG3365Energy 6Department

16

Energy Models for Drawing Signed Graphs Anne-Marie Kermarrec and Afshin Moin  

E-Print Network [OSTI]

Energy Models for Drawing Signed Graphs Anne-Marie Kermarrec and Afshin Moin INRIA Rennes Bretagne-dimensional space. Energy models are the prevalent approach to graph drawing. In this paper, we propose energy) or as negative (repulsive). The existent energy models do not discriminate against edge sign. Hence, they do

Paris-Sud XI, Université de

17

A propos des toponymes de l'epopee de Gesar  

E-Print Network [OSTI]

infini. Il n'en reste pas moins qu'un certainnombre d'enseignements peuvent tre tirs de l'examen des toponymes etdes formes toponymiques contenus dans l'pope, mais ils concernent plus S A propos des toponymes de lpope de Gesar 5 certains procds... bien procder de la cration potique que de lancessit de dfinir le "dcor" de l'pisode, ou bien contenir des allusions etdes rfrences personnelles qui nous chappent en gnral.La plupart des pithtes, prises ou non comme toponymes, dcrivent...

Chayet, Anne

2003-01-01T23:59:59.000Z

18

Recherches rcentes sur la radioactivit du thorium Extraits des mmoires de 0. Angelucci, G.-A. Blanc,  

E-Print Network [OSTI]

173 Recherches récentes sur la radioactivité du thorium Extraits des mémoires de 0. Angelucci, G publication des mémoires, des progrès accomplis dans l'étude de la radioactivité du thorium. L été établis avec une grande vraiselnblance. La famille du thorium est moins com- plètement connuc. Le

Boyer, Edmond

19

Gochimie des olivines plantaires : une approche micro-analytique par EPMA et LA-ICPMS  

E-Print Network [OSTI]

. Méthode : Une série d'olivines d'origines terrestre et extra-terrestre seront analysés : (1) Olivine (achondrites basaltiques, basaltes terrestres). Donc les olivines sont les témoins des processus de formation, Brachinites, HED, SNC) (5) Olivine terrestre (Manteau, Cumulat, Komatiites, MORB, OIB) (6) Olivine produit

Demouchy, Sylvie

20

Communication socitale des enseignes, le consommateur est-il toujours dupe ? le rle de la rputation  

E-Print Network [OSTI]

'améliorer leur image auprès des consommateurs. Néanmoins, face à la profusion d'arguments plus ou moins fondés, l reputation in brand-equity building with societal communication: an attribution theory approach Abstract: Many retailers communicate about their societal engagements to improve their image. Yet, overwhelmed

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.


21

E-Print Network 3.0 - aviation medicine Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Medicine Des Moines IA Des Moines University Osteopathic Medicine Des Moines IA Lake Erie College... Medicine Lake Erie PA Lake Erie College Osteopathic Physician Lake Erie...

22

Triggered star formation in the Magellanic Clouds  

E-Print Network [OSTI]

Abstract. We discuss how tidal interaction between the Large Magellanic Cloud (LMC), the Small Magellanic Cloud (SMC), and the Galaxy triggers galaxy-wide star formation in the Clouds for the last ? 0.2 Gyr based on our chemodynamical simulations on the Clouds. Our simulations demonstrate that the tidal interaction induces the formation of asymmetric spiral arms with high gas densities and consequently triggers star formation within the arms in the LMC. Star formation rate in the present LMC is significantly enhanced just above the eastern edge of the LMCs stellar bar owing to the tidal interaction. The location of the enhanced star formation is very similar to the observed location of 30 Doradus, which suggests that the formation of 30 Doradus is closely associated with the last Magellanic collision about 0.2 Gyr ago. The tidal interaction can dramatically compress gas initially within the outer part of the SMC so that new stars can be formed from the gas to become intergalactic young stars in the inter-Cloud region (e.g., the Magellanic Bridge). The metallicity distribution function of the newly formed stars in the Magellanic Bridge has a peak of [Fe/H] ? ?0.8, which is significantly lower than the stellar metallicity of the SMC.

B. G. Elmegreen; J. Palous; Kenji Bekki

2006-01-01T23:59:59.000Z

23

Argonne's Magellan Cloud Computing Research Project  

ScienceCinema (OSTI)

Pete Beckman, head of Argonne's Leadership Computing Facility (ALCF), discusses the Department of Energy's new $32-million Magellan project, which designed to test how cloud computing can be used for scientific research. More information: http://www.anl.gov/Media_Center/News/2009/news091014a.html

Beckman, Pete

2013-04-19T23:59:59.000Z

24

The Magellanic Stream in Modified Newtonian Dynamics  

E-Print Network [OSTI]

The dynamics of the Magellanic Stream (MS) as a series of clouds extending from the Magellanic Clouds (MCs) to the south Galactic pole is affected by the distribution and the amount of matter in the Milky Way. We calculate the gravitational effect of the Galactic disk on the MS in the framework of modified Newtonian dynamics(MOND) and compare with observations of the Stream's radial velocity. We consider the tidal force of the Galaxy, which strips material from the MCs to form the MS, and, using a no-halo model of the Galaxy, we ignore the effect of the drag of the Galactic halo on the MS. We also compare the MONDian dynamics with that in logarithmic and power-law dark halo models and show that the MOND theory seems plausible for describing the dynamics of satellite galaxies such as the MCs. Finally, we perform a maximum likelihood analysis to obtain the best MOND parameters for the Galactic disk.

Hossein Haghi; Sohrab Rahvar; Akram Hasani-Zonooz

2007-01-09T23:59:59.000Z

25

The Magellan Final Report on Cloud Computing  

SciTech Connect (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

How Common are the Magellanic Clouds  

SciTech Connect (OSTI)

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

27

Radio Planetary Nebulae in the Magellanic Clouds  

E-Print Network [OSTI]

We report the extragalactic radio-continuum detection of 15 planetary nebulae (PNe) in the Magellanic Clouds (MCs) from recent Australia Telescope Compact Array+Parkes mosaic surveys. These detections were supplemented by new and high resolution radio, optical and IR observations which helped to resolve the true nature of the objects. Four of the PNe are located in the Small Magellanic Cloud (SMC) and 11 are located in the Large Magellanic Cloud (LMC). Based on Galactic PNe the expected radio flux densities at the distance of the LMC/SMC are up to ~2.5 mJy and ~2.0 mJy at 1.4 GHz, respectively. We find that one of our new radio PNe in the SMC has a flux density of 5.1 mJy at 1.4 GHz, several times higher than expected. We suggest that the most luminous radio PN in the SMC (N S68) may represent the upper limit to radio peak luminosity because it is ~3 times more luminous than NGC 7027, the most luminous known Galactic PN. We note that the optical diameters of these 15 MCs PNe vary from very small (~0.08 pc or ...

Filipovi?, M D; Reid, W A; Payne, J L; Parker, Q A; Crawford, E J; Boji?i?, I S; De Horta, A Y; Hughes, A; Dickel, J; Stootman, F

2009-01-01T23:59:59.000Z

28

Magellan at NERSC Progress Report for June 2010  

SciTech Connect (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 MAGELLANIC QUASARS SURVEY. III. SPECTROSCOPIC CONFIRMATION OF 758 ACTIVE GALACTIC NUCLEI BEHIND THE MAGELLANIC CLOUDS  

SciTech Connect (OSTI)

The Magellanic Quasars Survey (MQS) has now increased the number of quasars known behind the Magellanic Clouds by almost an order of magnitude. All survey fields in the Large Magellanic Cloud (LMC) and 70% of those in the Small Magellanic Cloud (SMC) have been observed. The targets were selected from the third phase of the Optical Gravitational Lensing Experiment (OGLE-III) based on their optical variability, mid-IR, and/or X-ray properties. We spectroscopically confirmed 758 quasars (565 in the LMC and 193 in the SMC) behind the clouds, of which 94% (527 in the LMC and 186 in the SMC) are newly identified. The MQS quasars have long-term (12 yr and growing for OGLE), high-cadence light curves, enabling unprecedented variability studies of quasars. The MQS quasars also provide a dense reference grid for measuring both the internal and bulk proper motions of the clouds, and 50 quasars are bright enough (I ?< 18 mag) for absorption studies of the interstellar/intergalactic medium of the clouds.

Koz?owski, Szymon; Udalski, Andrzej; Szyma?ski, M. K.; Kubiak, M.; Pietrzy?ski, G.; Soszy?ski, I.; Wyrzykowski, ?.; Ulaczyk, K.; Poleski, R.; Pietrukowicz, P.; Skowron, J. [Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa (Poland); Onken, Christopher A. [Research School of Astronomy and Astrophysics, The Australian National University, Canberra 2611 (Australia); Kochanek, Christopher S. [Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210 (United States); Meixner, M. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Bonanos, A. Z., E-mail: simkoz@astrouw.edu.pl, E-mail: onken@mso.anu.edu.au, E-mail: ckochanek@astronomy.ohio-state.edu [National Observatory of Athens, Institute of Astronomy, Astrophysics, Space Applications and Remote Sensing, I. Metaxa and Vas. Pavlou St., Palaia Penteli, 15236 Athens (Greece); Collaboration: OGLE Collaboration

2013-10-01T23:59:59.000Z

30

Dans l'espace Le problme en volume est moins simple qu'il n'en a l'air.  

E-Print Network [OSTI]

Dans l'espace Le problème en volume est moins simple qu'il n'en a l'air. Cela ressemble à une de savon maximise l'aire enserrée par la ficelle (en minimisant l'aire du complémentaire). A New

Pansu, Pierre

31

MagellanHealth.com/member B-F1012rev1 (5/14) 2014 Magellan Health Services, Inc.  

E-Print Network [OSTI]

MagellanHealth.com/member B-F1012rev1 (5/14) 2014 Magellan Health Services, Inc. Finding the Right Care for Your Child Many children will spend part of their day in some form of child care setting and finding high quality, affordable child care is important. Resources and Referrals We understand no two

Meyers, Steven D.

32

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.

33

Spatial motion of the Magellanic Clouds. Tidal models ruled out?  

E-Print Network [OSTI]

Recently, Kallivayalil et al. derived new values of the proper motion for the Large and Small Magellanic Clouds (LMC and SMC, respectively). The spatial velocities of both Clouds are unexpectedly higher than their previous values resulting from agreement between the available theoretical models of the Magellanic System and the observations of neutral hydrogen (HI) associated with the LMC and the SMC. Such proper motion estimates are likely to be at odds with the scenarios for creation of the large-scale structures in the Magellanic System suggested so far. We investigated this hypothesis for the pure tidal models, as they were the first ones devised to explain the evolution of the Magellanic System, and the tidal stripping is intrinsically involved in every model assuming the gravitational interaction. The parameter space for the Milky Way (MW)-LMC-SMC interaction was analyzed by a robust search algorithm (genetic algorithm) combined with a fast restricted N-body model of the interaction. Our method extended ...

Ruzicka, Adam; Palous, Jan

2008-01-01T23:59:59.000Z

34

Dark Matter Annihilations in the Large Magellanic Cloud  

E-Print Network [OSTI]

The flat rotation curve obtained for the outer star clusters of the Large Magellanic Cloud is suggestive of an LMC dark matter halo. From the composite HI and star cluster rotation curve, I estimate the parameters of an isothermal dark matter halo added to a `maximum disk.' I then examine the possibility of detecting high energy gamma-rays from non-baryonic dark matter annihilations in the central region of the Large Magellanic Cloud.

P Gondolo

1993-12-06T23:59:59.000Z

35

Des villes sous influence. Gestion des risques et des catastrophes : des reprsentations  

E-Print Network [OSTI]

Des villes sous influence. Gestion des risques et des catastrophes : des reprsentations l bnfiques (cendres basiques fertilisant les sols dans le cas de certaines ruptions, activits et

Boyer, Edmond

36

Galactic and Magellanic Evolution with the SKA  

E-Print Network [OSTI]

As we strive to understand how galaxies evolve it is crucial that we resolve physical processes and test emerging theories in nearby systems that we can observe in great detail. Our own Galaxy, the Milky Way, and the nearby Magellanic Clouds provide unique windows into the evolution of galaxies, each with its own metallicity and star formation rate. These laboratories allow us to study with more detail than anywhere else in the Universe how galaxies acquire fresh gas to fuel their continuing star formation, how they exchange gas with the surrounding intergalactic medium, and turn warm, diffuse gas into molecular clouds and ultimately stars. The $\\lambda$21-cm line of atomic hydrogen (HI) is an excellent tracer of these physical processes. With the SKA we will finally have the combination of surface brightness sensitivity, point source sensitivity and angular resolution to transform our understanding of the evolution of gas in the Milky Way, all the way from the halo down to the formation of individual molecul...

McClure-Griffiths, Naomi M; Murray, Claire E; Li, Di; Dickey, John M; Vazquez-Semadeni, Enrique; Peek, Josh E G; Putman, Mary; Clark, Susan E; Miville-Deschenes, Marc-Antoine; Bland-Hawthorn, Joss; Staveley-Smith, Lister

2015-01-01T23:59:59.000Z

37

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 Refrigeration (AMRR) system. The heat transfer fluid is water, the regenerator consists of stacked gadolinium avoid using greenhouse gases and lower energy consumption by 20-30% over conventional technology

Boyer, Edmond

38

CHEMICAL EVOLUTION OF THE LARGE MAGELLANIC CLOUD  

SciTech Connect (OSTI)

We adopt a new chemical evolution model for the Large Magellanic Cloud (LMC) and thereby investigate its past star formation and chemical enrichment histories. The delay time distribution of Type Ia supernovae recently revealed by Type Ia supernova surveys is incorporated self-consistently into the new model. The principle results are summarized as follows. The present gas mass fraction and stellar metallicity as well as the higher [Ba/Fe] in metal-poor stars at [Fe/H] < -1.5 can be more self-consistently explained by models with steeper initial mass functions. The observed higher [Mg/Fe] ({>=}0.3) at [Fe/H] {approx} -0.6 and higher [Ba/Fe] (>0.5) at [Fe/H] {approx} -0.3 could be due to significantly enhanced star formation about 2 Gyr ago. The observed overall [Ca/Fe]-[Fe/H] relation and remarkably low [Ca/Fe] (< - 0.2) at [Fe/H] > -0.6 are consistent with models with short-delay supernova Ia and with the more efficient loss of Ca possibly caused by an explosion mechanism of Type II supernovae. Although the metallicity distribution functions do not show double peaks in the models with a starburst about 2 Gyr ago, they show characteristic double peaks in the models with double starbursts {approx}200 Myr and {approx}2 Gyr ago. The observed apparent dip of [Fe/H] around {approx}1.5 Gyr ago in the age-metallicity relation can be reproduced by models in which a large amount ({approx}10{sup 9} M{sub Sun }) of metal-poor ([Fe/H] < -1) gas can be accreted onto the LMC.

Bekki, Kenji [ICRAR, M468, University of Western Australia, 35 Stirling Highway, Crawley Western Australia 6009 (Australia); Tsujimoto, Takuji [National Astronomical Observatory of Japan, Mitaka-shi, Tokyo 181-8588 (Japan)

2012-12-20T23:59:59.000Z

39

THE MAGELLANIC INTER-CLOUD PROJECT (MAGIC). I. EVIDENCE FOR INTERMEDIATE-AGE STELLAR POPULATIONS IN BETWEEN THE MAGELLANIC CLOUDS  

SciTech Connect (OSTI)

The origin of the gas in between the Magellanic Clouds (MCs)-known as the ''Magellanic Bridge'' (MB)-is puzzling. Numerical simulations suggest that the MB formed from tidally stripped gas and stars in a recent interaction between the MCs. However, the apparent lack of stripped intermediate- or old-age stars associated with the MB is at odds with this picture. In this paper, we present the first results from the MAGellanic Inter-Cloud program (MAGIC) aimed at probing the stellar populations in the inter-Cloud region. We present observations of the stellar populations in two large fields located in between the Large and Small Magellanic Clouds (LMC/SMC), secured using the WFI camera on the 2.2 m telescope in La Silla. Using a synthetic color-magnitude diagram technique, we present the first quantitative evidence for the presence of intermediate-age and old stars in the inter-Cloud region. The intermediate-age stars-which make up {approx}28% of all stars in the region-are not present in fields at a similar distance from the SMC in a direction pointing away from the LMC. This provides potential evidence that these intermediate-age stars could have been tidally stripped from the SMC. However, spectroscopic studies will be needed to confirm or rule out the tidal origin for the inter-Cloud gas and stars.

Noeel, N. E. D.; Read, J. I. [ETH Zuerich, Institute for Astronomy, Wolfgang-Pauli-Strasse 27, CH-8093 Zuerich (Switzerland); Conn, B. C.; Rix, H.-W. [Max Planck Institut fuer Astronomie, Koenigstuhl 17, D-69117, Heidelberg (Germany); Carrera, R. [Instituto de Astrofisica de Canarias, C/Via Lactea s/n, E-38200, La Laguna, Tenerife (Spain); Dolphin, A., E-mail: noelia@phys.ethz.ch [Raytheon Company, P.O. Box 11337, Tucson, AZ 85734-1337 (United States)

2013-05-10T23:59:59.000Z

40

Utilisation des dfibrillateurs  

ScienceCinema (OSTI)

Information faite par le service medical et le service des pompiers sur l'utilisation des defibrillateurs.

None

2011-10-06T23:59:59.000Z

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

Constraints on the Cosmic Rays in the Small Magellanic Cloud  

E-Print Network [OSTI]

We show that recent $\\gamma$-ray observations of the Small Magellanic Cloud with EGRET rule out a universal cosmic ray flux only at energies below $\\approx 10$ GeV, while the observed diffuse X-ray and $\\gamma$-ray background radiations have already ruled out, by more than three orders of magnitude, a universal extragalactic cosmic ray flux identical to that observed in the local solar neighborhood at energies below $10^6$ GeV.

Arnon Dar; Ari Laor; Abraham Loeb

1993-02-25T23:59:59.000Z

42

The Magellanic Bridge: The Nearest Purely Tidal Stellar Population  

E-Print Network [OSTI]

We report on observations of the stellar populations in twelve fields spanning the region between the Magellanic Clouds, made with the Mosaic-II camera on the 4-meter telescope at the Cerro-Tololo Inter-American Observatory. The two main goals of the observations are to characterize the young stellar population (which presumably formed in situ in the Bridge and therefore represents the nearest stellar population formed from tidal debris), and to search for an older stellar component (which would have been stripped from either Cloud as stars, by the same tidal forces which formed the gaseous Bridge). We determine the star-formation history of the young inter-Cloud population, which provides a constraint on the timing of the gravitational interaction which formed the Bridge. We do not detect an older stellar population belonging to the Bridge in any of our fields, implying that the material that was stripped from the Clouds to form the Magellanic Bridge was very nearly a pure gas.

Jason Harris

2006-12-04T23:59:59.000Z

43

The Star Formation History of the Small Magellanic Cloud  

E-Print Network [OSTI]

We present the spatially-resolved star formation and chemical enrichment history of the Small Magellanic Cloud (SMC) across the entire central $4-degree x 4.5-degree area of the main body, based on UBVI photometry from our Magellanic Clouds Photometric Survey. We find that 1) approximately 50% of the stars that ever formed in the SMC formed prior to 8.4 Gyr ago (z >1.2 for WMAP cosmology), 2) the SMC formed relatively few stars between 8.4 and 3 Gyr ago, 3) there was a rise in the mean star formation rate during the most recent 3 Gyr punctuated by "bursts" at ages of 2.5, 0.4, and 0.06 Gyr, 4) the bursts at 2.5 and 0.4 Gyr are temporally coincident with past perigalactic passages of the SMC with the Milky Way, 5) there is preliminary evidence for a large-scale annular structure in the 2.5 Gyr burst, and 6) the chemical enrichment history derived from our analysis is in agreement with the age-metallicity relation of the SMC's star clusters. Consistent interpretation of the data required an ad hoc correction of 0.1-0.2 mag to the B-V colors of 25% of the stars; the cause of this anomaly is unknown, but we show that it does not strongly influence our results.

J. Harris; D. Zaritsky

2003-12-03T23:59:59.000Z

44

YELLOW AND RED SUPERGIANTS IN THE LARGE MAGELLANIC CLOUD  

SciTech Connect (OSTI)

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

45

ANALYSE DES DETERMINANTS DE LA GESTION DES RESULTATS : CAS DES FIRMES CANADIENNES FRANCAISES ET TUNISIENNES  

E-Print Network [OSTI]

- 1 - ANALYSE DES DETERMINANTS DE LA GESTION DES RESULTATS : CAS DES FIRMES CANADIENNES FRANCAISES)" #12;- 2 - ANALYSE DES DETERMINANTS DE LA GESTION DES RESULTATS : CAS DES FIRMES CANADIENNES FRANCAISES article sans l'aval écrit des auteurs'' "Please do not cote wihout authors' written permission" Adresse de

Paris-Sud XI, Université de

46

The Near-infrared Period-luminosity Relations of Cepheids in the Large Magellanic Cloud  

E-Print Network [OSTI]

We present near-infrared (J & Ks) observations of Cepheids in the Large Magellanic Cloud. The goals of these observations are to better characterize the Cepheid Period-Luminosity relation at these wavelengths, especially for periods below 10 days...

Mahzooni, Salma

2011-08-08T23:59:59.000Z

47

V-059: MoinMoin Multiple Vulnerabilities | Department of Energy  

Broader source: Energy.gov (indexed) [DOE]

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...

48

Rotation of the Milky Way and the formation of the Magellanic Stream  

E-Print Network [OSTI]

We studied the impact of the revisited values for the LSR circular velocity of the Milky Way (Reid et al. 2004) on the formation of the Magellanic Stream. The LSR circular velocity was varied within its observational uncertainties as a free parameter of the interaction between the Large (LMC) and the Small (SMC) Magellanic Clouds and the Galaxy. We have shown that the large-scale morphology and kinematics of the Magellanic Stream may be reproduced as tidal features, assuming the recent values of the proper motions of the Magellanic Clouds (Kallivayalil et al. 2006). Automated exploration of the entire parameter space for the interaction was performed to identify all parameter combinations that allow for modeling the Magellanic Stream. Satisfactory models exist for the dynamical mass of the Milky Way within a wide range of 0.6*10^12Msun to 3.0*10^12Msun and over the entire 1-sigma errors of the proper motions of the Clouds. However, the successful models share a common interaction scenario. The Magellanic Clou...

Ruzicka, Adam; Palous, Jan

2010-01-01T23:59:59.000Z

49

Interstellar O VI in the Large Magellanic Cloud  

E-Print Network [OSTI]

I summarize Far Ultraviolet Spectroscopic Explorer (FUSE) observations of interstellar O VI absorption towards 12 early-type stars in the Large Magellanic Cloud (LMC), the closest disk galaxy to the Milky Way. LMC O VI is seen towards all 12 stars with properties (average column densities, kinematics) very similar to those of the Milky Way halo, even though O/H in the LMC is lower by a factor of ~2.5. Sight lines projected onto known LMC superbubbles show little enhancement in O VI column density compared to sight lines towards quiescent regions of the LMC. The O VI absorption is displaced by \\~-30 km/sec from the corresponding low-ionization absorption associated with the bulk of the LMC gas. The LMC O VI most likely arises in a vertically-extended distribution, and I discuss the measurements in the context of a halo composed of radiatively-cooling hot gas. In this case, the mass-flow rate from one side of the LMC disk is of the order 1 solar mass/yr.

J. Christopher Howk

2001-09-14T23:59:59.000Z

50

A Catalog of HI Clouds in the Large Magellanic Cloud  

E-Print Network [OSTI]

A 21 cm neutral hydrogen interferometric survey of the Large Magellanic Cloud (LMC) combined with the Parkes multi-beam HI single-dish survey clearly shows that the HI gas is distributed in the form of clumps or clouds. The HI clouds and clumps have been identified using a thresholding method with three separate brightness temperature thresholds ($T_b$). Each catalog of HI cloud candidates shows a power law relationship between the sizes and the velocity dispersions of the clouds roughly following the Larson Law scaling $\\sigma_v \\propto R^{0.5}$, with steeper indices associated with dynamically hot regions. The clouds in each catalog have roughly constant virial parameters as a function mass suggesting that that the clouds are all in roughly the same dynamical state, but the values of the virial parameter are significantly larger than unity showing that turbulent motions dominate gravity in these clouds. The mass distribution of the clouds is a power law with differential indices between -1.6 and -2.0 for the three catalogs. In contrast, the distribution of mean surface densities is a log-normal distribution.

S. Kim; E. Rosolowsky; Y. Lee; Y. Kim; Y. C. Jung; M. A. Dopita; B. G. Elmegreen; K. C. Freeman; R. J. Sault; M. J. Kesteven; D. McConnell; Y. -H. Chu

2007-06-28T23:59:59.000Z

51

Gestion des aleas : utilisation des incertitudes en tp  

E-Print Network [OSTI]

ENSIM 4A Gestion des aleas : utilisation des incertitudes en tp http ://umtice,version4-4Jul2014 #12;Table des mati`eres 1 Methode de travail 3 2 dictionnaire 6 3 Gestion des aleas 8 3.1 Les ceintures de gestion des aleas . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8 3

Boyer, Edmond

52

The Formation of Constellation III in the Large Magellanic Cloud  

E-Print Network [OSTI]

We present a detailed reconstruction of the star-formation history of the Constellation III region in the Large Magellanic Cloud, to constrain the formation mechanism of this enigmatic feature. Star formation in Constellation III seems to have taken place during two distinct epochs: there is the 8-15 Myr epoch that had previously been recognized, but we also see strong evidence for a separate "burst" of star formation 25-30 Myr ago. The "super-supernova" or GRB blast wave model for the formation of Constellation III is difficult to reconcile with such an extended, two-epoch star formation history, because the shock wave should have induced star formation throughout the structure simultaneously, and any unconsumed gas would quickly be dissipated, leaving nothing from which to form a subsequent burst of activity. We propose a "truly stochastic" self-propagating star formation model, distinct from the canonical model in which star formation proceeds in a radially-directed wave from the center of Constellation III to its perimeter. As others have noted, and we now confirm, the bulk age gradients demanded by such a model are simply not present in Constellation III. In our scenario, the prestellar gas is somehow pushed into these large-scale arc structures, without simultaneously triggering immediate and violent star formation throughout the structure. Rather, star formation proceeds in the arc according to the local physical conditions of the gas. Self-propagating star formation is certainly possible, but in a truly stochastic manner, without a directed, large scale pattern.

Jason Harris; Dennis Zaritsky

2007-12-13T23:59:59.000Z

53

QUANTIFICATION DES AMPLITUDES ET DES TAUX DE DEFORMATION  

E-Print Network [OSTI]

'horizons sismo- sédimentaires dans des tranchées paléosismologiques: Récurrence des séismes: 2000-3000 ans

54

QUANTIFICATION DES AMPLITUDES ET DES TAUX DE DEFORMATION  

E-Print Network [OSTI]

ruptures et datation d'horizons sismo- sédimentaires dans des tranchées paléosismologiques: Récurrence des

55

Des pouvoirs en quilibre  

E-Print Network [OSTI]

©IRD-ThierryRuf Réunion de concertation entre irrigants dans la vallée des Aït Bouguemez, Maroc. 21 #12;

56

X-Ray Binary Systems in the Small Magellanic Cloud  

E-Print Network [OSTI]

We present the result of a systematic search for spectrally hard and soft X-ray binary systems in the Small Magellanic Cloud (SMC). This search has been applied to ROSAT PSPC data (0.1-2.4 keV) collected during 9 pointed observations towards this galaxy covering a time span of 2 years from October 91 till October 93. Selection criteria have been defined in order to confine the sample of candidates. Finally 7 spectrally hard and 4 spectrally soft sources were selected from the list as candidates for binaries in the SMC. The sample is luminosity limited (>3.10**35 erg/s). SMC X-1 has been observed during a full binary orbit starting with a low-state covering an X-ray eclipse and emerging into a bright long-duration flare with two short-duration flares separated by 10 hours. The Be type transient SMC X-2 has been redetected with ROSAT. Variability has been found in the sources RX J0051.8-7231 and RX J0052.1-731 already discovered with Einstein. RX J0101.0-7206 has been discovered at the north-eastern boundary of the giant SMC HII region N66 during an X-ray outburst and half a year later during a quiescent phase. A variable source, RX J0049.1-7250, located north-east of the SMC supernova remnant N19 and which may either be an X-ray binary or an AGN turns out to be strongly absorbed. It may be located behind the SMC. If it is an X-ray binary then it radiates at the Eddington limit in the X-ray bright state. Another variable and hard X-ray source RX J0032.9-7348 has been discovered at the south-eastern border of the body of the SMC. A high mass X-ray binary nature is favored for this source. We searched for CAL87 like systems in the SMC catalog and found none. A new candidate supersoft source RX J0103.8-7254 has been detected. We cannot exclude that it is a foreground object.

P. Kahabka; W. Pietsch

1997-06-09T23:59:59.000Z

57

Factorisons la gestion des vnements des applications interactives !  

E-Print Network [OSTI]

Factorisons la gestion des vnements des applications interactives ! Stphane Conversy, Paul et nous dgageons les lments essentiels un systme unifi de gestion d'vnements. Nous examinons'une conception de l'application base sur des vnements de diffrents niveaux. FACTORISATION DE LA GESTION DES

58

Facult des arts et des sciences Dpartement de communication  

E-Print Network [OSTI]

Faculté des arts et des sciences Département de communication Plans de cours cadre Cours des programmes de premier cycle en sciences de la communication Comité des études de premier cycle Adopté par l..................................................................................................................................3 COM 1150 Rédaction en communication 1

Parrott, Lael

59

Quantum Magellan theorem(the simplest NO-GO Theorem for hidden variables)  

E-Print Network [OSTI]

In this work we study time reversal (that can be realistically simulated using two total mirrors) of the interaction between single photon and beam splitter, without any measuring apparatus (detector). For description of this effect we use, on the one hand, standard quantum mechanical formalism, $SQM$. On the other hand, for description of the same effect, we use a hypothetical extension of the standard quantum mechanical formalism, so-called hidden variables theory, $HVT$, that should satisfy only few following general propositions. First proposition is that at the $SQM$ level of the analysis accuracy there are no effective distinctions between experimental facts, $SQM$ predictions and $HVT$ predictions. Second proposition is that at the hypothetically more accurate $HVT$ level of the analysis accuracy there is deterministic, one-to-one correspondence between initial and final dynamical state of the physical system so that $HVT$ dynamics is principally symmetric in respect to $HVT$ characteristic time reversal transformation. However, we simply demonstrate on mentioned example that such $HVT$ cannon exist that can be simply called quantum Magellan theorem (quantum mechanics represents "unique, Magellan straight" between "Atlantic ocean" of the macroscopic phenomena and "Great, Pacific ocean" of the microscopic phenomena). Obviously Magellan theorem can be considered as the simplest no-go theorem for a wide (potentially physically realistic) class of the hidden variables theories.

Vladan Pankovic; Darko Kapor

2014-06-18T23:59:59.000Z

60

Status Update and Closed-Loop Performance of the Magellan Adaptive Optics VisAO Camera  

E-Print Network [OSTI]

We present laboratory results of the closed-loop performance of the Magellan Adaptive Optics (AO) Adaptive Secondary Mirror (ASM), pyramid wavefront sensor (PWFS), and VisAO visible adaptive optics camera. The Magellan AO system is a 585-actuator low-emissivity high-throughput system scheduled for first light on the 6.5 meter Magellan Clay telescope in November 2012. Using a dichroic beamsplitter near the telescope focal plane, the AO system will be able to simultaneously perform visible (500-1000 nm) AO science with our VisAO camera and either 10 micron or 3-5 micron science using either the BLINC/MIRAC4 or CLIO cameras, respectively. The ASM, PWS, and VisAO camera have undergone final system tests in the solar test tower at the Arcetri Institute in Florence, Italy, reaching Strehls of 37% in i'-band with 400 modes and simulated turbulence of 14 cm ro at v-band. We present images and test results of the assembled VisAO system, which includes our prototype advanced Atmospheric Dispersion Corrector (ADC), prot...

Kopon, Derek; Males, Jared; Gasho, Victor; Morzinski, Katie; Follette, Katherine

2014-01-01T23:59:59.000Z

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

Prdiction des conflits dans des systmes homme-machine.  

E-Print Network [OSTI]

??Prdiction des conflits dans le systmes homme-machine. Le travail fait partie de la recherche consacre des problmes d'interaction homme-machine et aux conflits entre l'homme (more)

Pizziol, Sergio

2013-01-01T23:59:59.000Z

62

The University of Iowa College of Engineering Engineering Professional Development  

E-Print Network [OSTI]

Athena GTX Des Moines, IA Caterpillar Mossville, IL Caterpillar Peoria, IL Cerner Kansas City, MO Eaton Rapids, IA Siemens Corporate Research Princeton, NJ Source Allies Des Moines, IA Square D Cedar Rapids

Jacob, Mathews

63

Qualit des composts et des digestats Fabienne MULLER  

E-Print Network [OSTI]

Qualit des composts et des digestats Fabienne MULLER Direction consommation durable et dchets organiques se construit, avec aujourd'hui le dveloppement important de la mthanisation. Les composts actuellement produits, peuvent l'tre avec des digestats ou non. Les quantits de compost produit ne cessent d

Boyer, Edmond

64

Les nanosciences : (r)volution des savoirs et des technologies ?  

E-Print Network [OSTI]

1 Les nanosciences : (r)évolution des savoirs et des technologies ? Jean-Louis Pautrat Physicien, ancien Directeur de la Fondation "Nanosciences aux limites de la nanoélectronique" 23 rue des Martyrs : miniaturisation ; microélectronique ; nanomatériaux ; nanosciences ; nanomédecine 1 - Introduction Tout « honnête

Boyer, Edmond

65

Evaluation des performances des protocoles de routage Ad hoc  

E-Print Network [OSTI]

Evaluation des performances des protocoles de routage Ad hoc Abdelali Boushaba1 , Mohammed Oumsis2 quatre protocoles de routage Ad hoc: DSR, AODV, OLSR et DSDV et d'autre part, d'examiner l'impact de la'activité. Mots-clés--Réseaux mobiles Ad hoc; DSR; AODV; DSDV; OLSR; évaluation des performances; simulation, NS-2

Paris-Sud XI, Université de

66

The Properties of Early-type Stars in the Magellanic Clouds  

E-Print Network [OSTI]

The past decade has witnessed impressive progress in our understanding of the physical properties of massive stars in the Magellanic Clouds, and how they compare to their cousins in the Galaxy. I summarise new results in this field, including evidence for reduced mass-loss rates and faster stellar rotational velocities in the Clouds, and their present-day compositions. I also discuss the stellar temperature scale, emphasizing its dependence on metallicity across the entire upper-part of the Hertzsprung-Russell diagram.

Christopher J. Evans

2008-09-15T23:59:59.000Z

67

The distance modulus of the Large Magellanic Cloud: Constraints from RR Lyrae pulsation properties  

E-Print Network [OSTI]

It has recently been suggested that the discrepancy between the "long" and "short" distance moduli of the Large Magellanic Cloud (LMC), as inferred from the properties of the Cepheid and RR Lyrae variables, respectively, might be due to the action of "third parameters" between the Galaxy and the LMC, which would make the RR Lyraes in the old LMC globular clusters brighter than their Galactic counterparts by $\\simeq 0.3 {mag}$. Through analysis of the RR Lyrae pulsation properties, we show that this idea is not supported by the available data. A satisfactory explanation of the problem has yet to be found.

M. Catelan

1996-01-05T23:59:59.000Z

68

Conservation des Textiles  

E-Print Network [OSTI]

Conservation des Textiles Les 22 et 23 mai 2013 Soit 2 jours - 14 heures OBJECTIFS DE LA FORMATION essentielles dans la gestion de collections textiles, depuis leur identification jusqu'à leur conservation conservation d'éléments et de collections textiles, et toutes personnes travaillant dans le domaine du

Brest, Université de

69

Habilitation `a diriger des recherches preparee au  

E-Print Network [OSTI]

Approche par contraintes des probl`emes d'ordonnancement et d'affectation : structures temporelles et m´en´eraux de propagation de contraintes. Des rapprochements sont faits avec des techniques issues des probl`emes de satisfaction de contraintes. Le cas des probl`emes d'ordonnancement purement temporels est

Boyer, Edmond

70

A ``Short'' Distance to the Large Magellanic Cloud With the Hipparcos Calibrated Red Clump Stars  

E-Print Network [OSTI]

Following an approach developed by Paczy\\'nski & Stanek, we derive a distance to the Large Magellanic Cloud (LMC) by comparing red clump stars from the Hipparcos catalog with the red clump stars observed in two fields in the LMC that were selected from the ongoing photometric survey of the Magellanic Clouds to lie in low extinction regions. The use of red clump stars allows a single step determination of the distance modulus to the LMC, $\\mu_{0,LMC} = 18.065\\pm 0.031\\pm 0.09 $mag (statistical plus systematic error), and the corresponding distance, $R_{LMC}= 41.02\\pm 0.59\\pm 1.74 kpc$. This measurement is in excellent agreement with the recent determination by Udalski et al., also based on the red clump stars, but is $\\sim 0.4 $mag smaller than the generally accepted value of $\\mu_{0,LMC} = 18.50\\pm 0.15 $mag. We discuss possible reasons for this discrepancy and how it can be resolved.

K. Z. Stanek; D. Zaritsky; J. Harris

1998-03-16T23:59:59.000Z

71

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

SciTech Connect (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

72

THE SPATIAL DISTRIBUTION OF DUST AND STELLAR EMISSION OF THE MAGELLANIC CLOUDS  

SciTech Connect (OSTI)

We study the emission by dust and stars in the Large and Small Magellanic Clouds, a pair of low-metallicity nearby galaxies, as traced by their spatially resolved spectral energy distributions. This project combines Herschel Space Observatory PACS and SPIRE far-infrared photometry with other data at infrared and optical wavelengths (the data were obtained as part of the HERschel Inventory of The Agents of Galaxy Evolution survey; PI: M. Meixner). We build maps of dust, stellar luminosity, and mass of both Magellanic Clouds, and analyze the spatial distribution of dust/stellar luminosity and mass ratios. These ratios vary considerably throughout the galaxies, generally between the range 0.01 {<=} L{sub dust}/L{sub *} {<=} 0.6 and 10{sup -4} {<=} M{sub dust}/M{sub *} {<=} 4 Multiplication-Sign 10{sup -3}. We observe that the dust/stellar ratios depend on the interstellar medium environment, such as the distance from currently or previously star-forming regions, and on the intensity of the interstellar radiation field. In addition, we construct star formation rate (SFR) maps, and find that the SFR is correlated with the dust/stellar luminosity and dust temperature in both galaxies, demonstrating the relation between star formation, dust emission, and heating, though these correlations exhibit substantial scatter.

Skibba, Ramin A.; Engelbracht, Charles W.; Misselt, Karl; Montiel, Edward [Steward Observatory, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721 (United States); Aniano, Gonzalo [Princeton University Observatory, Peyton Hall, Princeton, NJ 08544 (United States); Babler, Brian [Department of Astronomy, 475 North Charter St., University of Wisconsin, Madison, WI 53706 (United States); Bernard, Jean-Philippe [Universite de Toulouse, UPS-OMP, IRAP, Toulouse (France); Bot, Caroline [Universite de Strasbourg, Observatoire Astronomique de Strasbourg, F-67000 Strasbourg (France); Carlson, Lynn Redding; Israel, Frank [Sterrewacht Leiden, Leiden University, P.O. Box 9513, 2300 RA Leiden (Netherlands); Galametz, Maud [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA (United Kingdom); Galliano, Frederic; Hony, Sacha; Lebouteiller, Vianney; Madden, Suzanne; Okumura, Koryo; Panuzzo, Pasquale [AIM, CEA/Saclay, L'Orme des Merisiers, 91191 Gif-sur-Yvette (France); Gordon, Karl; Meixner, Margaret [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Li, Aigen, E-mail: rskibba@ucsd.edu [314 Physics Building, Department of Physics and Astronomy, University of Missouri, Columbia, MO 65211 (United States); and others

2012-12-10T23:59:59.000Z

73

CHEMICAL SIGNATURE OF A MAJOR MERGER IN THE EARLY FORMATION OF THE SMALL MAGELLANIC CLOUD  

SciTech Connect (OSTI)

The formation history of the Small Magellanic Cloud (SMC) is unraveled based on the results of our new chemical evolution models constructed for the SMC, highlighting the observed anomaly in the age-metallicity relation for star clusters in the SMC. We first propose that evidence of a major merger is imprinted in the age-metallicity relation as a dip in [Fe/H]. Our models predict that the major merger with a mass ratio of 1:1 to 1:4 occurred at {approx}7.5 Gyr ago, with a good reproduction of the abundance distribution function of field stars in the SMC. Furthermore, our models predict a relatively large scatter in [Mg/Fe] for -1.4 {<=} [Fe/H] {<=} -1.1 as a reflection of a looping feature resulting from the temporally inverse progress of chemical enrichment, which can be tested against future observational results. Given that the observed velocity dispersion ({approx}30 km s{sup -1}) of the SMC is much smaller than that ({approx}160 km s{sup -1}) of the Galactic halo, our finding strongly implies that the predicted merger event happened in a small group environment that was far from the Galaxy and contained a number of small gas-rich dwarfs comparable to the SMC. This theoretical view is extensively discussed in the framework that considers a connection with the formation history of the Large Magellanic Cloud.

Tsujimoto, Takuji [National Astronomical Observatory, Mitaka-shi, Tokyo 181-8588 (Japan); Bekki, Kenji [School of Physics, University of New South Wales, Sydney 2052, NSW (Australia)], E-mail: taku.tsujimoto@nao.ac.jp

2009-08-01T23:59:59.000Z

74

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

75

UNIVERSITE DE NANTES FACULTE DES SCIENCES ET DES TECHNIQUES  

E-Print Network [OSTI]

'`a beaucoup d'autres), le go^ut et le plaisir des math´emati- ques, gr^ace `a ses cours passionnants et l

Boyer, Edmond

76

UNIVERSIT DE NANTES FACULT DES SCIENCES ET DES TECHNIQUES  

E-Print Network [OSTI]

remerci´e pour son soutien qui s'est poursuivi par le financement d'une partie des sismos acquis par le

Paris-Sud XI, Université de

77

Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds  

E-Print Network [OSTI]

The EROS-2 project was designed to test the hypothesis that massive compact halo objects (the so-called ``machos'') could be a major component of the dark matter halo of the Milky Way galaxy. To this end, EROS-2 monitored millions of stars in the Magellanic clouds for microlensing events caused by such objects. About $33\\times10^6$ Magellanic stars were observed over a period of 6.7 years. Unlike all previous studies of Magellanic microlensing, we use only a subsample of $7\\times10^6$ bright stars. This strategy minimizes backgrounds due to variable stars and ensures accurate determination of lensing parameters by minimizing source confusion (blending). Using this sample of bright stars, only one candidate event was found, whereas $\\sim42$ events would have been expected if the Halo were entirely populated by objects of mass $M\\sim0.4M_{\\odot}$. Combined with the results of EROS-1, this implies that the optical depth toward the Large Magellanic Cloud (\\object{LMC}) due to such lenses is $\\tau<0.36\\times10^...

Tisserand, P; Afonso, C; Albert, J N; Andersen, J; Ansari, R; Aubourg, E; Bareyre, P; Beaulieu, J P; Charlot, X; Coutures, C; Ferlet, R; Fouqu, P; Glicenstein, J F; Goldman, B; Gould, A; Graff, D; Gros, M; Hassinski, J; Hamadache, C; De Kat, J; Lasserre, T; Lesquoy, E; Loup, C; Magneville, C; Marquette, J B; Maurice, E; Maury, A; Milsztajn, A; Moniez, M; Palanque-Delabrouille, Nathalie; Perdereau, O; Rahal, Y R; Rich, J; Spiro, M; Vidal-Madjar, A; Vigroux, L; Zylberajch, S

2006-01-01T23:59:59.000Z

78

en partenariat Des partenariats  

E-Print Network [OSTI]

attribuées 5 jeunes équipes du Sud soutenues Au Maroc, accord intergouvernemental et accord- cadre avec l mathématique et informatique des systèmes complexes, implantée principalement au Maroc et en France. 1er et mathématiques appliquées, au Maroc. Congrès international de génétique, de biologie moléculaire et

79

La gestion des transactions La gestion des transactions  

E-Print Network [OSTI]

La gestion des transactions 1 #12;La gestion des transactions On ne doit appliquer `a une base de`erement. En cas de parallelisme entre transactions, chacune doit ^etre executee de facon en apparence

Wolper, Pierre

80

UNIVERSIT DE NANTES FACULT DES SCIENCES ET DES TECHNIQUES  

E-Print Network [OSTI]

recherche INRIA Rocquencourt Responsable Scientifique : Jean-Marc Menaud, Ma^itre-assistant ´Ecole des Mines´e hallucinante pour r´ev´eler des probl`emes que j'aurais mis un temps fou `a enfouir. Enfin, `a Jean-Marc Menaud

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.


81

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

SciTech Connect (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

82

PERFORMANCE COMPTABLE GESTION DES RESULTATS  

E-Print Network [OSTI]

1 PERFORMANCE COMPTABLE ET GESTION DES RESULTATS Yves Mard Enseignant l'IAE de Lyon 6, cours Albert Thomas 69 008 Lyon Docteur en Sciences de Gestion (IAE d'Aix en Provence) Coordonnes personnelles : Tl : 06 64 19 39 74 E-mail : ymard @aol.com Rsum L'tude porte sur la gestion des rsultats afin d

Boyer, Edmond

83

The HI Environment of Three Superbubbles in the Large Magellanic Cloud  

E-Print Network [OSTI]

The ambient interstellar environment of wind- and supernova-driven superbubbles strongly affects their evolution, but its properties are rarely well-determined. We have therefore obtained HI aperture synthesis imaging of the environment around three similar, optically-selected superbubble nebulae in the Large Magellanic Cloud. The resulting HI maps show that the ambient gas distribution around these superbubbles differ to an extreme: DEM L25 shows no neutral shell component, but is nestled within an HI hole; DEM L50 shows a massive neutral shell component, but is otherwise within an HI void; and DEM L301 shows no correspondence at all between the optical nebula and HI distribution. There is also poor correspondence between the HI and optical kinematics. These results strongly caution against inferring properties of the ambient neutral environment of individual superbubbles without direct observations. Finally, all three objects show some evidence of shock activity.

M. S. Oey; B. Groves; L. Staveley-Smith; R. C. Smith

2001-12-04T23:59:59.000Z

84

The exceptionally powerful TeV gamma-ray emitters in the Large Magellanic Cloud  

E-Print Network [OSTI]

The Large Magellanic Cloud, a satellite galaxy of the Milky Way, has been observed with the High Energy Stereoscopic System (H.E.S.S.) above an energy of 100 billion electron volts for a deep exposure of 210 hours. Three sources of different types were detected: the pulsar wind nebula of the most energetic pulsar known N 157B, the radio-loud supernova remnant N 132D and the largest non-thermal X-ray shell - the superbubble 30 Dor C. The unique object SN 1987A is, surprisingly, not detected, which constrains the theoretical framework of particle acceleration in very young supernova remnants. These detections reveal the most energetic tip of a gamma-ray source population in an external galaxy, and provide via 30 Dor C the unambiguous detection of gamma-ray emission from a superbubble.

:,; Aharonian, F; Benkhali, F Ait; Akhperjanian, A G; Angner, E O; Backes, M; Balenderan, S; Balzer, A; Barnacka, A; Becherini, Y; Becker-Tjus, J; Berge, D; Bernhard, S; Bernlhr, K; Birsin, E; Biteau, J; Bttcher, M; Boisson, C; Bolmont, J; Bordas, P; Bregeon, J; Brun, F; Brun, P; Bryan, M; Bulik, T; Carrigan, S; Casanova, S; Chadwick, P M; Chakraborty, N; Chalme-Calvet, R; Chaves, R C G; Chrtien, M; Colafrancesco, S; Cologna, G; Conrad, J; Couturier, C; Cui, Y; Dalton, M; Davids, I D; Degrange, B; Deil, C; de Wilt, P; Djannati-Ata, A; Domainko, W; Donath, A; Drury, L O'C; Dubus, G; Dutson, K; Dyks, J; Dyrda, M; Edwards, T; Egberts, K; Eger, P; Espigat, P; Farnier, C; Fegan, S; Feinstein, F; Fernandes, M V; Fernandez, D; Fiasson, A; Fontaine, G; Frster, A; ling, M F; Gabici, S; Gajdus, M; Gallant, Y A; Garrigoux, T; Giavitto, G; Giebels, B; Glicenstein, J F; Gottschall, D; Grondin, M -H; Grudzi?ska, M; Hadasch, D; Hffner, S; Hahn, J; Harris, J; Heinzelmann, G; Henri, G; Hermann, G; Hervet, O; Hillert, A; Hinton, J A; Hofmann, W; Hofverberg, P; Holler, M; Horns, D; Ivascenko, A; Jacholkowska, A; Jahn, C; Jamrozy, M; Janiak, M; Jankowsky, F; Jung, I; Kastendieck, M A; Katarzy?ski, K; Katz, U; Kaufmann, S; Khlifi, B; Kieffer, M; Klepser, S; Klochkov, D; Klu?niak, W; Kolitzus, D; Komin, Nu; Kosack, K; Krakau, S; Krayzel, F; Krger, P P; Laffon, H; Lamanna, G; Lefaucheur, J; Lefranc, V; Lemire, A; Lemoine-Goumard, M; Lenain, J -P; Lohse, T; Lopatin, A; Lu, C -C; Marandon, V; Marcowith, A; Marx, R; Maurin, G; Maxted, N; Mayer, M; McComb, T J L; Mhault, J; Meintjes, P J; Menzler, U; Meyer, M; Mitchell, A M W; Moderski, R; Mohamed, M; Mor, K; Moulin, E; Murach, T; de Naurois, M; Niemiec, J; Nolan, S J; Oakes, L; Odaka, H; Ohm, S; Opitz, B; Ostrowski, M; Oya, I; Panter, M; Parsons, R D; Arribas, M Paz; Pekeur, N W; Pelletier, G; Perez, J; Petrucci, P -O; Peyaud, B; Pita, S; Poon, H; Phlhofer, G; Punch, M; Quirrenbach, A; Raab, S; Reichardt, I; Reimer, A; Reimer, O; Renaud, M; Reyes, R de los; Rieger, F; Rob, L; Romoli, C; Rosier-Lees, S; Rowell, G; Rudak, B; Sahakian, C B Rulten V; Salek, D; Sanchez, D A; Santangelo, A; Schlickeiser, R; Schssler, F; Schulz, A; Schwanke, U; Schwarzburg, S; Schwemmer, S; Sol, H; Spanier, F; Spengler, G; Spies, F; Stawarz, ?; Steenkamp, R; Stegmann, C; Stinzing, F; Stycz, K; Sushch, I; Tavernet, J -P; Tavernier, T; Taylor, A M; Terrier, R; Tluczykont, M; Trichard, C; Valerius, K; van Eldik, C; van Soelen, B; Vasileiadis, G; Veh, J; Venter, C; Viana, A; Vincent, P; Vink, J; Vlk, H J; Volpe, F; Vorster, M; Vuillaume, T; Wagner, S J; Wagner, P; Wagner, R M; Ward, M; Weidinger, M; Weitzel, Q; White, R; Wierzcholska, A; Willmann, P; Wrnlein, A; Wouters, D; Yang, R; Zabalza, V; Zaborov, D; Zacharias, M; Zdziarski, A A; Zech, A; Zechlin, H -S

2015-01-01T23:59:59.000Z

85

Optical Spectra of Radio Planetary Nebulae in the Small Magellanic Cloud  

E-Print Network [OSTI]

We present preliminary results from spectral observations of four candidate radio sources co-identified with known planetary nebulae (PNe) in the Small Magellanic Cloud (SMC). These were made using the Radcliffe 1.9-meter telescope in Sutherland, South Africa. These radio PNe were originally found in Australia Telescope Compact Array (ATCA) surveys of the SMC at 1.42 and 2.37 GHz, and were further confirmed by new high resolution ATCA images at 6 and 3 cm (4"/2"). Optical PNe and radio candidates are within 2" and may represent a subpopulation of selected radio bright objects. Nebular ionized masses of these objects may be 2.6 MSol or greater, supporting the existence of PNe progenitor central stars with masses up to 8 MSol.

J. L. Payne; M. D. Filipovi?; E. J. Crawford; A. Y. De Horta; G. L. White; F. H. Stootman

2008-04-29T23:59:59.000Z

86

Optical Spectra of Radio Planetary Nebulae in the Small Magellanic Cloud  

E-Print Network [OSTI]

We present preliminary results from spectral observations of four candidate radio sources co-identified with known planetary nebulae (PNe) in the Small Magellanic Cloud (SMC). These were made using the Radcliffe 1.9-meter telescope in Sutherland, South Africa. These radio PNe were originally found in Australia Telescope Compact Array (ATCA) surveys of the SMC at 1.42 and 2.37 GHz, and were further confirmed by new high resolution ATCA images at 6 and 3 cm (4"/2"). Optical PNe and radio candidates are within 2" and may represent a subpopulation of selected radio bright objects. Nebular ionized masses of these objects may be 2.6 MSol or greater, supporting the existence of PNe progenitor central stars with masses up to 8 MSol.

Payne, J L; Crawford, E J; De Horta, A Y; White, G L; Stootman, F H

2008-01-01T23:59:59.000Z

87

SIGECORIS : un simulateur pour explorer des modalits de gestion prventive des inondations  

E-Print Network [OSTI]

SIGECORIS : un simulateur pour explorer des modalits de gestion prventive des inondations rflexion sur la politique amricaine, avance que la premire ambition de toute politique de gestion des philosophies de gestion des inondations dont l'objectif serait la rduction des dommages. Le point de vue

Boyer, Edmond

88

Toxicite des emissions des vehicules diesel Docteur en mededne l'INERIS  

E-Print Network [OSTI]

94-53 .'X- Toxicite des emissions des vehicules diesel D. LAFON Docteur en mededne l'INERIS De nombreuses questions ont ete posees au cours de ce debat sur la toxicite des emissions des moteurs diesel. II de la tche que nous avons effectuee. I. Composition des emissions du diesel Avant d'aborder la

Paris-Sud XI, Universit de

89

ORIGIN OF THE UNUSUALLY LOW NITROGEN ABUNDANCES IN YOUNG POPULATIONS OF THE LARGE MAGELLANIC CLOUD  

SciTech Connect (OSTI)

It is a longstanding problem that H II regions and very young stellar populations in the Large Magellanic Cloud (LMC) have nitrogen abundances ([N/H]) that are a factor of {approx}7 lower than the solar value. We here discuss a new scenario in which the observed unusually low nitrogen abundances can be closely associated with recent collisions and subsequent accretion of H I high velocity clouds (HVCs) that surround the Galaxy and have low nitrogen abundances. We show that if the observed low [N/H] is limited to very young stars with ages less than {approx}10{sup 7} yr, then the collision/accretion rate of the HVCs onto the LMC needs to be {approx}0.2 M{sub sun} yr{sup -1} (corresponding to the total HVC mass of 10{sup 6}-10{sup 7} M{sub sun}) to dilute the original interstellar medium (ISM) before star formation. The required accretion rate means that even if the typical mass of HVCs accreted onto the LMC is {approx}10{sup 7} M{sub sun}, the Galaxy needs to have {approx}2500 massive HVCs within the LMC's orbital radius with respect to the Galactic center. The rather large number of required massive HVCs drives us to suggest that the HVCs are not likely to efficiently dilute the ISM of the LMC and consequently lower the [N/H]. We thus suggest the transfer of gas with low [N/H] from the Small Magellanic Cloud to the LMC as a promising scenario that can explain the observed low [N/H].

Bekki, Kenji [ICRAR, M468, University of Western Australia, 35 Stirling Highway, Crawley Western Australia 6009 (Australia); Tsujimoto, Takuji [National Astronomical Observatory, Mitaka-shi, Tokyo 181-8588 (Japan)

2010-10-01T23:59:59.000Z

90

Scurit au-del des mythes et des croyances  

ScienceCinema (OSTI)

Prsentation orale en franais, support visuel en franais et en anglais. La pire des failles de scurit est l'impression de scurit. Le dcalage entre la comprhension que l?on a des technologies utilises, et leurs potentiels rels, ainsi que l'impact potentiellement ngatif qu'elles peuvent avoir sur nos vies, n'est pas toujours compris, ou pris en compte par la plupart d'entre-nous. On se contente de nos perceptions pour ne pas avoir se confronter la ralit... Alors qu'en est-il vraiment ? En matire de scurit qui de l'humain ou des technologies a le contrle ?

None

2011-10-06T23:59:59.000Z

91

CONSERVATION ET SURVIE PROLONGE DES SPERMATOZODES  

E-Print Network [OSTI]

CONSERVATION ET SURVIE PROLONG?E DES SPERMATOZOÏDES DANS LES VOIES G?NITALES FEMELLES DES VERT?BR?S'épithélium des sites de conservation sont de trois types : les spermatozoïdes peuvent demeurer pêle-mêle dans la cellulaire. Mais il ne semble pas exister de relation entre le type de contact et la durée de conservation

Paris-Sud XI, Université de

92

Analyse des erreurs orthographiques des tudiants iraniens en langue franaise.  

E-Print Network [OSTI]

??Lobjectif de cette recherche consiste dcrire les types derreurs dorthographe des tudiants iraniens en langue franaise et mener une analyse qualitative et quantitative (more)

Katoozian, Katayoon

2013-01-01T23:59:59.000Z

93

Examining the Infrared Variable Star Population Discovered in the Small Magellanic Cloud Using the SAGE-SMC Survey  

E-Print Network [OSTI]

We present our study on the infrared variability of point sources in the Small Magellanic Cloud (SMC). We use the data from the Spitzer Space Telescope Legacy Program "Surveying the Agents of Galaxy Evolution in the Tidally Stripped, Low Metallicity Small Magellanic Cloud" (SAGE-SMC) and the "Spitzer Survey of the Small Magellanic Cloud" (S$^{3}$MC) survey, over three different epochs, separated by several months to three years. Variability in the thermal infrared is identified using a combination of Spitzer's IRAC 3.6, 4.5, 5.8, and 8.0 $\\mu$m bands, and the MIPS 24 $\\mu$m band. An error-weighted flux difference between each pair of three epochs ("variability index") is used to assess the variability of each source. A visual source inspection is used to validate the photometry and image quality. Out of $\\sim$2 million sources in the SAGE-SMC catalog, 814 meet our variability criteria. We matched the list of variable star candidates to the catalogs of SMC sources classified with other methods, available in th...

Polsdofer, Elizabeth; Sewilo, Marta; Vijh, Uma; Meixner, Margaret; Marengo, Massimo; Terrazas, Maverick

2015-01-01T23:59:59.000Z

94

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

E-Print Network [OSTI]

pour le sant des turbines gaz (TAG). Au Ca- Qubec. nadades annes gie des turbines gaz reprsentera 1990, qui ont

Bolinger, Mark; Wiser, Ryan; Golove, William

2003-01-01T23:59:59.000Z

95

Diplme d'Universit valuation de la Qualit des Soins  

E-Print Network [OSTI]

sant ; n CONTENU Semaine 1 METHODES et OUTILS des DMARCHES QUALIT niveau I - Les principaux outils et METHODES et OUTILS des DMARCHES QUALIT niveau II - Suite des mthodes et outils des dmarques qualit

Brest, Universit de

96

AKARI INFRARED CAMERA SURVEY OF THE LARGE MAGELLANIC CLOUD. II. THE NEAR-INFRARED SPECTROSCOPIC CATALOG  

SciTech Connect (OSTI)

We performed a near-infrared spectroscopic survey toward an area of {approx}10 deg{sup 2} of the Large Magellanic Cloud (LMC) with the infrared satellite AKARI. Observations were carried out as part of the AKARI Large-area Survey of the Large Magellanic Cloud (LSLMC). The slitless multi-object spectroscopic capability of the AKARI/IRC enabled us to obtain low-resolution (R {approx} 20) spectra in 2-5 {mu}m for a large number of point sources in the LMC. As a result of the survey, we extracted about 2000 infrared spectra of point sources. The data are organized as a near-infrared spectroscopic catalog. The catalog includes various infrared objects such as young stellar objects (YSOs), asymptotic giant branch (AGB) stars, supergiants, and so on. It is shown that 97% of the catalog sources have corresponding photometric data in the wavelength range from 1.2 to 11 {mu}m, and 67% of the sources also have photometric data up to 24 {mu}m. The catalog allows us to investigate near-infrared spectral features of sources by comparison with their infrared spectral energy distributions. In addition, it is estimated that about 10% of the catalog sources are observed at more than two different epochs. This enables us to study a spectroscopic variability of sources by using the present catalog. Initial results of source classifications for the LSLMC samples are presented. We classified 659 LSLMC spectra based on their near-infrared spectral features by visual inspection. As a result, it is shown that the present catalog includes 7 YSOs, 160 C-rich AGBs, 8 C-rich AGB candidates, 85 O-rich AGBs, 122 blue and yellow supergiants, 150 red super giants, and 128 unclassified sources. Distributions of the classified sources on the color-color and color-magnitude diagrams are discussed in the text. Continuous wavelength coverage and high spectroscopic sensitivity in 2-5 {mu}m can only be achieved by space observations. This is an unprecedented large-scale spectroscopic survey toward the LMC in the near-infrared. A large number of near-infrared spectral data provided by the survey possess scientific potential that can be applied to various studies. In this paper, we present the details of the spectroscopic survey and the catalog, and discuss its scientific applications.

Shimonishi, Takashi [Department of Earth and Planetary Sciences, Graduate School of Science, Kobe University, Nada Kobe 657-8501 (Japan); Onaka, Takashi; Kato, Daisuke; Sakon, Itsuki [Department of Astronomy, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan); Ita, Yoshifusa [Astronomical Institute, Graduate School of Science, Tohoku University, 6-3 Aramaki Aoba, Aoba-ku, Sendai, Miyagi 980-8578 (Japan); Kawamura, Akiko [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Kaneda, Hidehiro, E-mail: shimonishi@penguin.kobe-u.ac.jp [Graduate School of Science, Nagoya University, Chikusa-ku, Nagoya 464-8602 (Japan)

2013-02-01T23:59:59.000Z

97

On the Spatial Distribution of Stellar Populations in the Large Magellanic Cloud  

E-Print Network [OSTI]

We measure the angular correlation function of stars in a region of the Large Magellanic Cloud (LMC) that spans 2 degrees by 1.5 degrees. We find that the correlation functions of stellar populations are represented well by exponential functions of the angular separation for separations between 2 and 40 arcmin (corresponding to ~ 30 pc and 550 pc for an LMC distance of 50 kpc). The inner boundary is set by the presence of distinct, highly correlated structures, which are the more familiar stellar clusters, and the outer boundary is set by the observed region's size and the presence of two principal centers of star formation within the region. We also find that the normalization and scale length of the correlation function changes systematically with the mean age of the stellar population. The existence of positive correlation at large separations (~300 pc), even in the youngest population, argues for large-scale hierarchical structure in current star formation. The evolution of the angular correlation toward lower normalizations and longer scale lengths with stellar age argues for the dispersion of stars with time. We show that a simple, stochastic, self-propagating star formation model is qualitatively consistent with this behavior of the correlation function.

Jason Harris; Dennis Zaritsky

1999-02-20T23:59:59.000Z

98

Mean age gradient and asymmetry in the star formation history of the Small Magellanic Cloud  

E-Print Network [OSTI]

We derive the star formation history in four regions of the Small Magellanic Cloud (SMC) using the deepest VI color-magnitude diagrams (CMDs) ever obtained for this galaxy. The images were obtained with the Advanced Camera for Surveys onboard the Hubble Space Telescope and are located at projected distances of 0.5-2 degrees from the SMC center, probing the main body and the wing of the galaxy. We derived the star-formation histories (SFH) of the four fields using two independent procedures to fit synthetic CMDs to the data. We compare the SFHs derived here with our earlier results for the SMC bar to create a deep pencil-beam survey of the global history of the central SMC. We find in all the six fields observed with HST a slow star formation pace from 13 to 5-7 Gyr ago, followed by a ~ 2-3 times higher activity. This is remarkable because dynamical models do not predict a strong influence of either the LMC or the Milky Way (MW) at that time. The level of the intermediate-age SFR enhancement systematically inc...

Cignoni, M; Tosi, M; Gallagher, J S; Sabbi, E; Anderson, J; Grebel, E K; Nota, A

2013-01-01T23:59:59.000Z

99

The beat Cepheids in the Magellanic Clouds: an analysis from the EROS-2 database  

E-Print Network [OSTI]

A number of microlensing dark-matter surveys have produced tens of millions of light curves of individual background stars. These data provide an unprecedented opportunity for systematic studies of whole classes of variable stars and their host galaxies. We aim to use the EROS-2 survey of the Magellanic Clouds to detect and study the population of beat Cepheids (BCs) in both Clouds. BCs pulsating simultaneously in the first overtone and fundamental modes (FO/F) or in the second and first overtone modes (SO/FO) are of particular interest. Using special software designed to search for periodic variables, we have scanned the EROS-2 data base for variables in the typical period range of Cepheids. Metallicities of FO/F objects were then calculated from linear nonadiabatic convective stellar models. We identify 74 FO/F BCs in the LMC and 41 in the SMC, and 173 and 129 SO/FO pulsators in the LMC and SMC, respectively; 185 of these stars are new discoveries. For nearly all the FO/F objects we determine minimum, mean,...

Marquette, J B; Buchler, J R; Szab, R; Tisserand, P; Belghith, S; Fouqu, P; Lesquoy, E; Milsztajn, A; Schwarzenberg-Czerny, A; Afonso, C; Albert, J N; Andersen, J; Ansari, R; Aubourg, E; Bareyre, P; Charlot, X; Coutures, C; Ferlet, R; Glicenstein, J F; Goldman, B; Gould, A; Graff, D; Gros, M; Hassinski, J; Hamadache, C; De Kat, J; Guillou, L Le; Loup, C; Magneville, C; Maurice, E; Maury, A; Moniez, M; Palanque-Delabrouille, Nathalie; Perdereau, O; Rahal, Y R; Rich, J; Spiro, M; Vidal-Madjar, A

2009-01-01T23:59:59.000Z

100

Quantifying the Drivers of Star Formation on Galactic Scales. I. The Small Magellanic Cloud  

E-Print Network [OSTI]

We use the star formation history of the Small Magellanic Cloud (SMC) to place quantitative limits on the effect of tidal interactions and gas infall on the star formation and chemical enrichment history of the SMC. The coincident timing of two recent (driver of star formation, but is only near the SMC during the most recent burst. The poorly constrained LMC-SMC orbit is our principal uncertainty. To explore the correspondence between bursts and MW pericenter passages further, we model star formation in the SMC using a combination of continuous and tidally-triggered star formation. The behavior of the tidally-triggered mode is a strong inverse function of the SMC-MW separation (preferred behavior ~ r^-5, resulting in a factor of ~100 difference in the rate of tidally-triggered star formation at pericenter and apocenter). Despite the success of these closed-box evolutionary models in reproducing the recent SMC star formation history and current chemical abundance, they have some systematic shortcomings that are remedied by postulating that a sizable infall event (~ 50% of the total gas mass) occured about 4 Gyr ago. Regardless of whether this infall event is included, the fraction of stars in the SMC that formed via a tidally triggered mode is > 10% and could be as large as 70%.

Dennis Zaritsky; Jason Harris

2003-12-04T23:59:59.000Z

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101

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

SciTech Connect (OSTI)

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

102

DUST EMISSION FROM EVOLVED AND UNEVOLVED H II REGIONS IN THE LARGE MAGELLANIC CLOUD  

SciTech Connect (OSTI)

We present a study of the dust properties of 12 classical and superbubble H II regions in the Large Magellanic Cloud. We use infrared photometry from Spitzer (8, 24, 70, and 160 {mu} m bands), obtained as part of the Surveying the Agents of a Galaxy's Evolution (SAGE) program, along with archival spectroscopic classifications of the ionizing stars to examine the role of stellar sources on dust heating and processing. Our infrared observations show surprisingly little correlation between the emission properties of the dust and the effective temperatures or bolometric magnitudes of stars in the H II regions, suggesting that the H II region evolutionary timescale is not on the order of the dust processing timescale. We find that the infrared emission of superbubbles and classical H II regions shows little differentiation between the two classes, despite the significant differences in age and morphology. We do detect a correlation of the 24 {mu} m emission from hot dust with the ratio of 70-160 {mu} m flux. This correlation can be modeled as a trend in the temperature of a minority hot dust component, while a majority of the dust remains significantly cooler.

Slater, C. T.; Oey, M. S. [Astronomy Department, University of Michigan, Ann Arbor, MI 48109 (United States); Li, A. [Department of Physics and Astronomy, University of Missouri, Columbia, MO 65211 (United States); Bernard, J.-Ph.; Paradis, D. [Universit de Toulouse, UPS-OMP, IRAP, Toulouse (France); Churchwell, E. [Department of Astronomy, University of Wisconsin-Madison, 475 North Charter Street, Madison, WI 53706 (United States); Gordon, K. D.; Lawton, B.; Meixner, M. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Indebetouw, R. [Department of Astronomy, University of Virginia, P.O. Box 3818, Charlottesville, VA 22903 (United States); Reach, W.T. [Universities Space Research Association, Stratospheric Observatory for Infrared Astronomy, NASA Ames Research Center, MS 211-3, Moffett Field, CA 94035 (United States)

2011-05-10T23:59:59.000Z

103

DETECTION OF AN ULTRA-BRIGHT SUBMILLIMETER GALAXY BEHIND THE SMALL MAGELLANIC CLOUD  

SciTech Connect (OSTI)

We report the discovery of a new ultra-bright submillimeter galaxy (SMG) behind the Small Magellanic Cloud (SMC). This SMG is detected as a 43.3 {+-} 8.4 mJy point source (MM J01071-7302, hereafter MMJ0107) in the 1.1 mm continuum survey of the SMC by AzTEC on the ASTE telescope. MMJ0107 is also detected in the radio (843 MHz), Herschel/SPIRE, Spitzer MIPS 24 {mu}m, all IRAC bands, Wide-field Infrared Survey Explorer, and near-infrared (J, H, K{sub S} ). We find an optical (U, B, V) source, which might be the lensing object, at a distance of 1.''4 from near-infrared and IRAC sources. Photometric redshift estimates for the SMG using representative spectral energy distribution templates show the redshifts of 1.4-3.9. We estimate total far-infrared luminosity of (0.3-2.2) Multiplication-Sign 10{sup 14} {mu}{sup -1} L{sub Sun} and a star formation rate of 5600-39, 000 {mu}{sup -1} M{sub Sun} yr{sup -1}, where {mu} is the gravitational magnification factor. This apparent extreme star formation activity is likely explained by a highly magnified gravitational lens system.

Takekoshi, Tatsuya; Minamidani, Tetsuhiro; Sorai, Kazuo; Habe, Asao [Department of Cosmosciences, Graduate School of Science, Hokkaido University, Sapporo 060-0810 (Japan); Tamura, Yoichi; Kohno, Kotaro [Institute of Astronomy, University of Tokyo, Osawa, Mitaka, Tokyo 181-0015 (Japan); Oogi, Taira [Department of Physics, Faculty of Science, Hokkaido University, Sapporo 060-0810 (Japan); Ezawa, Hajime; Komugi, Shinya; Mizuno, Norikazu; Muller, Erik; Kawamura, Akiko [Chile Observatory, National Astronomical Observatory, Mitaka, Tokyo 181-8588 (Japan); Oshima, Tai [Nobeyama Radio Observatory, National Astronomical Observatory of Japan, Minamimaki, Minamisaku, Nagano 384-1305 (Japan); Scott, Kimberly S. [North American ALMA Science Center, National Radio Astronomy Observatory, Charlottesville, VA 22903 (United States); Austermann, Jason E. [Center for Astrophysics and Space Astronomy, University of Colorado, Boulder, CO 80309 (United States); Tosaki, Tomoka [Joetsu University of Education, Joetsu, Niigata 943-8512 (Japan); Onishi, Toshikazu [Department of Physical Science, Osaka Prefecture University, Gakuen 1-1, Sakai, 599-8531 Osaka (Japan); Fukui, Yasuo [Department of Astrophysics, Nagoya University, Chikusa-ku, Nagoya 464-8602 (Japan); Matsuo, Hiroshi [Advanced Technology Center, National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588 (Japan); Aretxaga, Itziar [Instituto Nacional de Astrofisica, Optica y Electronica (INAOE), 72000 Puebla (Mexico); and others

2013-09-10T23:59:59.000Z

104

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

SciTech Connect (OSTI)

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

105

Chemical Signature of a Major Merger in the Early Formation of Small Magellanic Cloud  

E-Print Network [OSTI]

The formation history of the Small Magellanic cloud (SMC) is unraveled based on the results of our new chemical evolution models constructed for the SMC, highlighting the observed anomaly in the age-metallicity relation for star clusters in the SMC. We first propose that evidence of a major merger is imprinted in the age-metallicity relation as a dip in [Fe/H]. Our models predict that the major merger with a mass ratio of 1:1 to 1:4 occurred at ~7.5 Gyr ago, with a good reproduction of the abundance distribution function of field stars in the SMC. Furthermore, our models predict a relatively large scatter in [Mg/Fe] for -1.4 < [Fe/H] <-1.1 as a reflection of a looping feature resulting from the temporally inverse progress of chemical enrichment, which can be tested against future observational results. Given that the observed velocity dispersion (~30 km/s) of the SMC is much smaller than that (~160 km/s) of the Galactic halo, our finding strongly implies that the predicted merger event happened in a sma...

Tsujimoto, Takuji

2009-01-01T23:59:59.000Z

106

FACULT DES SCIENCES HUMAINES ET SOCIALES -SORBONNE  

E-Print Network [OSTI]

FACULT? DES SCIENCES HUMAINES ET SOCIALES - SORBONNE LICENCE EN SCIENCES HUMAINES ET SOCIALES ANN?E UNIVERSITAIRE 2013-2014 MENTION SCIENCES DU Vaillant 92100 Boulogne-Billancourt L3, M1 et M2 Faculté des Sciences

Pellier, Damien

107

FACULT DES SCIENCES HUMAINES ET SOCIALES -SORBONNE  

E-Print Network [OSTI]

FACULT? DES SCIENCES HUMAINES ET SOCIALES - SORBONNE LICENCE EN SCIENCES HUMAINES ET SOCIALES ANN?E UNIVERSITAIRE 2013-2014 MENTION SCIENCES DE L'?DUCATION L3 Faculté des Sciences humaines et sociales

Pellier, Damien

108

G. GNIN. -LA CORROSION DES MTAUX 159 LA CORROSION DES MTAUX  

E-Print Network [OSTI]

G. G?NIN. - LA CORROSION DES M?TAUX 159 LA CORROSION DES M?TAUX AU COURS DE LA FABRICATION DU LAIT corrosion des métaux par le lait, au cours des transformations successives que ce produit subit dans l spéciale- ment attachés à l'étude de la corrosion des métaux dans la fabrica- . tion du lait condensé. et

Paris-Sud XI, Université de

109

GESTION DES RISQUES ET PROCESSUS STRATEGIQUES  

E-Print Network [OSTI]

processus ; enfin, nous mettons en oeuvre cette approche sur un cas de gestion des risques, dans une grandeGESTION DES RISQUES ET PROCESSUS STRATEGIQUES Ren Demeestre et Philippe Lorino1 Rsum Abstract nombreuses entreprises investir dans leur systme de pilotage et la gestion des risques est une composante

Boyer, Edmond

110

A SPITZER SPACE TELESCOPE FAR-INFRARED SPECTRAL ATLAS OF COMPACT SOURCES IN THE MAGELLANIC CLOUDS. I. THE LARGE MAGELLANIC CLOUD  

SciTech Connect (OSTI)

We present far-infrared spectra, {lambda} = 52-93 {mu}m, obtained with the Spitzer Space Telescope in the spectral energy distribution mode of its MIPS instrument, of a representative sample of the most luminous compact far-infrared sources in the Large Magellanic Cloud (LMC). These include carbon stars, OH/IR asymptotic giant branch (AGB) stars, post-AGB objects and planetary nebulae, the R CrB-type star HV 2671, the OH/IR red supergiants (RSGs) WOH G064 and IRAS 05280 - 6910, the three B[e] stars IRAS 04530 - 6916, R 66 and R 126, the Wolf-Rayet star Brey 3a, the luminous blue variable (LBV) R 71, the supernova remnant N 49, a large number of young stellar objects (YSOs), compact H II regions and molecular cores, and a background galaxy at a redshift z {approx_equal} 0.175. We use the spectra to constrain the presence and temperature of cold dust and the excitation conditions and shocks within the neutral and ionized gas, in the circumstellar environments and interfaces with the surrounding interstellar medium (ISM). First, we introduce a spectral classification scheme. Then, we measure line strengths, dust temperatures, and IR luminosities. Objects associated with star formation are readily distinguished from evolved stars by their cold dust and/or fine-structure lines. Evolved stars, including the LBV R 71, lack cold dust except in some cases where we argue that this is swept-up ISM. This leads to an estimate of the duration of the prolific dust-producing phase ('superwind') of several thousand years for both RSGs and massive AGB stars, with a similar fractional mass loss experienced despite the different masses. We tentatively detect line emission from neutral oxygen in the extreme RSG WOH G064, which suggests a large dust-free cavity with implications for wind driving. In N 49, the shock between the supernova ejecta and ISM is revealed in spectacular fashion by its strong [O I] {lambda}63 {mu}m emission and possibly water vapor; we estimate that 0.2 M {sub sun} of ISM dust was swept up. On the other hand, some of the compact H II regions display pronounced [O III] {lambda}88 {mu}m emission. The efficiency of photoelectric heating in the interfaces of ionized gas and molecular clouds is estimated at 0.1%-0.3%. We confirm earlier indications of a low nitrogen content in the LMC. Evidence for solid state emission features is found in both young and evolved objects, but the carriers of these features remain elusive; some of the YSOs are found to contain crystalline water ice. The spectra constitute a valuable resource for the planning and interpretation of observations with the Herschel Space Observatory and the Stratospheric Observatory For Infrared Astronomy.

Van Loon, Jacco Th.; Oliveira, Joana M. [Astrophysics Group, Lennard-Jones Laboratories, Keele University, Staffordshire ST5 5BG (United Kingdom); Gordon, Karl D.; Meixner, Margaret; Shiao, Bernie; Boyer, Martha L. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Kemper, F.; Woods, Paul M. [Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester M13 9PL (United Kingdom); Tielens, A. G. G. M. [Leiden Observatory, P.O. Box 9513, NL-2300 RA Leiden (Netherlands); Marengo, Massimo [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Indebetouw, Remy; Chen, C.-H. Rosie [Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904 (United States); Sloan, G. C. [Department of Astronomy, Cornell University, Ithaca, NY 14853 (United States)], E-mail: jacco@astro.keele.ac.uk

2010-01-15T23:59:59.000Z

111

Revealing the Large-Scale Structures of Interstellar Gas Associated with the Magellanic SNR N132D  

E-Print Network [OSTI]

We report preliminary results of large-scale distribution toward the Magellanic supernova remnant N132D using Mopra and Chandra archival datasets. We identified a cavity-like CO structure along the X-ray shell toward the southern half of it. The total mass of associating molecular gas is $\\sim10^4 M_\\odot$, which is smaller than the previous study by an order of magnitude. Further observations using ALMA, ASTE, and Mopra will reveal the detailed spatial structures and its physical conditions.

Sano, H; Yoshiike, S; Fukuda, T; Tachihara, K; Inutsuka, S; Kawamura, A; Fujii, K; Mizuno, N; Inoue, T; Onishi, T; Acero, F; Vink, J

2015-01-01T23:59:59.000Z

112

A SEARCH FOR RAPIDLY ACCRETING WHITE DWARFS IN THE SMALL MAGELLANIC CLOUD  

SciTech Connect (OSTI)

The nature of the progenitors of Type Ia supernovae (SNe Ia) is still a mystery. While plausible candidates are known for both the single-degenerate and double-degenerate models, the observed numbers fall significantly short of what is required to reproduce the SNe Ia rate. Some of the most promising single-degenerate Type Ia progenitors are recurrent novae and super-soft sources (SSS). White dwarfs (WDs) with higher mass transfer rates can also be SN Ia progenitors. For these rapidly accreting white dwarfs (RAWDs), more material than is needed for steady burning accretes on the WD, and extends the WD's photosphere. Unlike SSS, such objects will likely not be detectable at soft X-ray energies, but will be bright at longer wavelengths, such as the far-ultraviolet (UV). Possible examples include LMC N66 and the V Sagittae stars. We present a survey using multi-object spectrographs looking for RAWDs in the central core of the Small Magellanic Cloud (SMC), from objects selected to be bright in the far-UV and with blue far UV - V colors. While we find some unusual objects, and recover known planetary nebula and Wolf-Rayet (WR) stars, we detect no candidate RAWD. The upper limits from this non-detection depend on our expectations of what an RAWD should look like, as well assumptions about the internal extinction of the SMC. Assuming they resemble LMC N66 or fainter versions of WR stars we set an upper limit of 10-14 RAWDs in the SMC. However, our survey is unlikely to detect objects like V Sge, and hence we cannot set meaningful upper limits if RAWDs generally resemble V Sge.

Lepo, Kelly; Van Kerkwijk, Marten, E-mail: lepo@astro.utoronto.ca, E-mail: mhvk@astro.utoronto.ca [Department of Astronomy and Astrophysics, University of Toronto, 50 Saint George St., Toronto, ON M5S 3H4 (Canada)

2013-07-01T23:59:59.000Z

113

ICE CHEMISTRY IN EMBEDDED YOUNG STELLAR OBJECTS IN THE LARGE MAGELLANIC CLOUD  

SciTech Connect (OSTI)

We present spectroscopic observations of a sample of 15 embedded young stellar objects (YSOs) in the Large Magellanic Cloud (LMC). These observations were obtained with the Spitzer Infrared Spectrograph (IRS) as part of the SAGE-Spec Legacy program. We analyze the two prominent ice bands in the IRS spectral range: the bending mode of CO{sub 2} ice at 15.2 mum and the ice band between 5 and 7 mum that includes contributions from the bending mode of water ice at 6 mum among other ice species. The 5-7 mum band is difficult to identify in our LMC sample due to the conspicuous presence of polycyclic aromatic hydrocarbon emission superimposed onto the ice spectra. We identify water ice in the spectra of two sources; the spectrum of one of those sources also exhibits the 6.8 mum ice feature attributed in the literature to ammonium and methanol. We model the CO{sub 2} band in detail, using the combination of laboratory ice profiles available in the literature. We find that a significant fraction (approx>50%) of CO{sub 2} ice is locked in a water-rich component, consistent with what is observed for Galactic sources. The majority of the sources in the LMC also require a pure-CO{sub 2} contribution to the ice profile, evidence of thermal processing. There is a suggestion that CO{sub 2} production might be enhanced in the LMC, but the size of the available sample precludes firmer conclusions. We place our results in the context of the star formation environment in the LMC.

Oliveira, J. M.; Van Loon, J. Th. [School of Physical and Geographical Sciences, Lennard-Jones Laboratories, Keele University, Staffordshire ST5 5BG (United Kingdom); Chen, C.-H. R.; Indebetouw, R. [Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904 (United States); Tielens, A. G. G. M. [Leiden Observatory, P.O. Box 9513, NL-2300 RA Leiden (Netherlands); Sloan, G. C. [Department of Astronomy, Cornell University, Ithaca, NY 14853 (United States); Woods, P. M.; Kemper, F. [Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL (United Kingdom); Gordon, K. D.; Boyer, M. L.; Shiao, B.; Meixner, M. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Madden, S. [Service d'Astrophysique, Commissariat a L'Energie Atomique de Saclay, 91191 Gif-sur-Yvette (France); Speck, A. K. [Physics and Astronomy, University of Missouri, Columbia, MO 65211 (United States); Marengo, M. [Department of Physics and Astronomy, Iowa State University, Ames, IA 50010 (United States)

2009-12-20T23:59:59.000Z

114

DISCOVERY OF X-RAY EMISSION FROM YOUNG SUNS IN THE SMALL MAGELLANIC CLOUD  

SciTech Connect (OSTI)

We report the discovery of extended X-ray emission within the young star cluster NGC 602a in the Wing of the Small Magellanic Cloud (SMC) based on observations obtained with the Chandra X-Ray Observatory. X-ray emission is detected from the cluster core area with the highest stellar density and from a dusty ridge surrounding the H II region. We use a census of massive stars in the cluster to demonstrate that a cluster wind or wind-blown bubble is unlikely to provide a significant contribution to the X-ray emission detected from the central area of the cluster. We therefore suggest that X-ray emission at the cluster core originates from an ensemble of low- and solar-mass pre-main-sequence (PMS) stars, each of which would be too weak in X-rays to be detected individually. We attribute the X-ray emission from the dusty ridge to the embedded tight cluster of the newborn stars known in this area from infrared studies. Assuming that the levels of X-ray activity in young stars in the low-metallicity environment of NGC 602a are comparable to their Galactic counterparts, then the detected spatial distribution, spectral properties, and level of X-ray emission are largely consistent with those expected from low- and solar-mass PMS stars and young stellar objects (YSOs). This is the first discovery of X-ray emission attributable to PMS stars and YSOs in the SMC, which suggests that the accretion and dynamo processes in young, low-mass objects in the SMC resemble those in the Galaxy.

Oskinova, L. M.; Hainich, R. [Institute for Physics and Astronomy, University Potsdam, D-14476 Potsdam (Germany)] [Institute for Physics and Astronomy, University Potsdam, D-14476 Potsdam (Germany); Sun, W.; Chen, Y. [Department of Astronomy, Nanjing University, Nanjing, 210093 Jiangsu (China)] [Department of Astronomy, Nanjing University, Nanjing, 210093 Jiangsu (China); Evans, C. J. [UK Astronomy Technology Centre, Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom)] [UK Astronomy Technology Centre, Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Henault-Brunet, V. [Scottish Universities Physics Alliance (SUPA), Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom)] [Scottish Universities Physics Alliance (SUPA), Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Chu, Y.-H.; Gruendl, R. A. [Department of Astronomy, University of Illinois, 1002 West Green Street, Urbana, IL 61801 (United States)] [Department of Astronomy, University of Illinois, 1002 West Green Street, Urbana, IL 61801 (United States); Gallagher, J. S. III [Department of Astronomy, University of Wisconsin-Madison, 5534 Sterling, 475 North Charter Street, Madison, WI 53706 (United States)] [Department of Astronomy, University of Wisconsin-Madison, 5534 Sterling, 475 North Charter Street, Madison, WI 53706 (United States); Guerrero, M. A. [Instituto de Astrofisica de Andalucia, IAA-CSIC, Glorieta de la Astronomia s/n, E-18008 Granada (Spain)] [Instituto de Astrofisica de Andalucia, IAA-CSIC, Glorieta de la Astronomia s/n, E-18008 Granada (Spain); Guedel, M. [Department of Astrophysics, University of Vienna, Tuerkenschanzstrasse 17, A-1180 Vienna (Austria)] [Department of Astrophysics, University of Vienna, Tuerkenschanzstrasse 17, A-1180 Vienna (Austria); Silich, S. [Instituto Nacional de Astrofisica Optica y Electronica, AP 51, 72000 Puebla (Mexico)] [Instituto Nacional de Astrofisica Optica y Electronica, AP 51, 72000 Puebla (Mexico); Naze, Y. [GAPHE, Departement AGO, Universite de Liege, Allee du 6 Aout 17, Bat. B5C, B-4000 Liege (Belgium)] [GAPHE, Departement AGO, Universite de Liege, Allee du 6 Aout 17, Bat. B5C, B-4000 Liege (Belgium); Reyes-Iturbide, J. [LATO-DCET/Universidade Estadual de Santa Cruz, Rodovia Jorge Amado, km 16, 45662-000 Ilheus, BA (Brazil)] [LATO-DCET/Universidade Estadual de Santa Cruz, Rodovia Jorge Amado, km 16, 45662-000 Ilheus, BA (Brazil)

2013-03-01T23:59:59.000Z

115

ENREGISTREMENT DES MICROPULSATIONS GOMAGNTIQUES UTILISANT DES MAGNTOMTRES A NOYAU SATUR  

E-Print Network [OSTI]

et sovié- tiques [4], pour mesurer le champ magnétique de l'espace extra-terrestre, de grandeur. 2014 On présente une installation d'enregistrement des micropulsations du champ magnétique terrestre

Paris-Sud XI, Université de

116

Fiche technique Dtail des panneaux  

E-Print Network [OSTI]

- Biodiversité des cultures Panneau 4 - Paysage à Madagascar Panneau 5 - Labour d'un champ au Maroc Panneau 6 9 - Récolte d'un essaim d'abeilles au Maroc Panneau 10 - L'innovation en marche Panneau 11

117

Andr Laperrire Laboratoire des technologies  

E-Print Network [OSTI]

, meal cooking,...) Probably not critical for an Indoor Hockey Ice Rink #12;Groupe ­ Technologie9 PERIODAndré Laperrière Laboratoire des technologies de l'énergie d'Hydro-Québec Shawinigan Indoor Ice Rinks and LED Technology 2013 Biannual Joint Meeting of CIE/USA and CNC/CIE University of California (UC

California at Davis, University of

118

Universite d' Avignon et des  

E-Print Network [OSTI]

le sous-problème · TAD dans le Doubs Central · Conclusion et perspectives ´Etude et r et des Pays de Vaucluse www.univ-avignon.fr Plan Contexte, objectifs Contexte · TAD · DARP · R.univ-avignon.fr Plan Contexte, objectifs · Contexte TAD · DARP · R´esolution · Doubs Central · Conclusion et

Ingrand, François

119

Expression des constantes de distorsion centrifuge des hexafluorures en fonction des frquences harmoniques.  

E-Print Network [OSTI]

'application est faite aux molécules SF6 et UF6. 4 constantes cubiques de SF6 ont été déterminées à partir des for the centrifugal distortion constants as a function of harmonic frequencies ; application is made to SF6 and UF6. 4

Paris-Sud XI, Université de

120

THE MID-INFRARED EXTINCTION LAW IN THE LARGE MAGELLANIC CLOUD  

SciTech Connect (OSTI)

Based on photometric data from the Spitzer/SAGE survey, using red giants as extinction tracers, the mid-infrared (MIR) extinction laws in the Large Magellanic Cloud (LMC) are derived for the first time in the form of A{sub ?}/A{sub K{sub S}}. This quantity refers to the extinction in the four Infrared Array Camera (IRAC) bands (i.e., [3.6], [4.5], [5.8], and [8.0] ?m) relative to the Two Micron All Sky Survey K{sub S} band at 2.16 ?m. We obtain the near-infrared extinction coefficient to be E(J H)/E(H K{sub S} ) ? 1.29 0.04 and E(J K{sub S} )/E(H K{sub S} ) ? 1.94 0.04. The wavelength dependence of the MIR extinction A{sub ?}/A{sub K{sub S}} in the LMC varies from one sightline to another. The overall mean MIR extinction is A{sub [3.6]}/A{sub K{sub S}}?0.720.03, A{sub [4.5]}/A{sub K{sub S}}?0.940.03, A{sub [5.8]}/A{sub K{sub S}}?0.580.04, and A{sub [8.0]}/A{sub K{sub S}}?0.620.05. Except for the extinction in the IRAC [4.5] ?m band, which may be contaminated by the 4.6 ?m CO gas absorption of red giants used to trace LMC extinction, the extinction in the other three IRAC bands show a flat curve, close to the Milky Way R{sub V} = 5.5 model extinction curve, where R{sub V} is the optical total-to-selective extinction ratio. The possible systematic bias caused by the correlated uncertainties of K{sub S} ? and J K{sub S} is explored in terms of Monte Carlo simulations. We find that this bias could lead to an overestimation of A{sub ?}/A{sub K{sub S}} in the MIR.

Gao, Jian; Jiang, B. W.; Xue, M. Y. [Department of Astronomy, Beijing Normal University, Beijing 100875 (China); Li, Aigen, E-mail: jiangao@bnu.edu.cn, E-mail: bjiang@bnu.edu.cn, E-mail: lia@missouri.edu [Department of Physics and Astronomy, University of Missouri, Columbia, MO 65211 (United States)

2013-10-10T23:59:59.000Z

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

AKARI INFRARED CAMERA SURVEY OF THE LARGE MAGELLANIC CLOUD. I. POINT-SOURCE CATALOG  

SciTech Connect (OSTI)

We present a near- to mid-infrared point-source catalog of five photometric bands at 3.2, 7, 11, 15, and 24 {mu}m for a 10 deg{sup 2} area of the Large Magellanic Cloud (LMC) obtained with the Infrared Camera on board the AKARI satellite. To cover the survey area the observations were carried out at three separate seasons from 2006 May to June, 2006 October to December, and 2007 March to July. The 10{sigma} limiting magnitudes of the present survey are 17.9, 13.8, 12.4, 9.9, and 8.6 mag at 3.2, 7, 11, 15, and 24 {mu}m, respectively. The photometric accuracy is estimated to be about 0.1 mag at 3.2 {mu}m and 0.06-0.07 mag in the other bands. The position accuracy is 0.''3 at 3.2, 7, and 11 {mu}m and 1.''0 at 15 and 24 {mu}m. The sensitivities at 3.2, 7, and 24 {mu}m are roughly comparable to those of the Spitzer SAGE LMC point-source catalog, while the AKARI catalog provides the data at 11 and 15 {mu}m, covering the mid-infrared spectral range contiguously. Two types of catalog are provided: a Catalog and an Archive. The Archive contains all the detected sources, while the Catalog only includes the sources that have a counterpart in the Spitzer SAGE point-source catalog. The Archive contains about 650,000, 140,000, 97,000, 43,000, and 52,000 sources at 3.2, 7, 11, 15, and 24 {mu}m, respectively. Based on the catalog, we discuss the luminosity functions at each band, the color-color diagram, and the color-magnitude diagram using the 3.2, 7, and 11 {mu}m band data. Stars without circumstellar envelopes, dusty C-rich and O-rich stars, young stellar objects, and background galaxies are located at distinct regions in the diagrams, suggesting that the present catalog is useful for the classification of objects toward the LMC.

Kato, Daisuke; Onaka, Takashi; Shimonishi, Takashi; Sakon, Itsuki [Department of Astronomy, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan); Ita, Yoshifusa [Astronomical Institute, Tohoku University, 6-3 Aramaki, Aoba-ku, Sendai, Miyagi 980-8578 (Japan); Tanabe, Toshihiko; Takahashi, Hidenori [Institute of Astronomy, School of Science, University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015 (Japan); Kaneda, Hidehiro [Graduate School of Science, Nagoya University, Chikusa-ku, Nagoya 464-8602 (Japan); Kawamura, Akiko [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Wada, Takehiko; Usui, Fumihiko [Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshino-dai, Chuo-ku, Sagamihara, Kanagawa 252-5210 (Japan); Koo, Bon-Chul [Department of Physics and Astronomy, Seoul National University, Seoul 151-742 (Korea, Republic of); Matsuura, Mikako, E-mail: kato@ir.isas.jaxa.jp, E-mail: onaka@astron.s.u-tokyo.ac.jp [Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT (United Kingdom)

2012-12-01T23:59:59.000Z

122

L'importance des probabilits a priori pour la recherche des pages d'entre1  

E-Print Network [OSTI]

Search », Proceedings of the 25th annual international ACM SIGIR Conference on Research and Cevelopment structure des liens, les URL et les textes d'ancrage sont des sources intéressantes d'information pour la

Hiemstra, Djoerd

123

Nr. 129 / 2011 // 12. Juli 2011 Empfehlung des Wissenschaftsrates  

E-Print Network [OSTI]

. Der Leiter des Forschungszentrums für Bio-Makromoleküle und des Lehrstuhls für Biopolymere, Prof. Dr PD Dr. Stephan Schwarzinger, Mitglied des Lehrstuhls für Biopolymere. biologie und Molekularmedizin

Ullmann, G. Matthias

124

Partager : des technologies de pointe au service de la socit  

ScienceCinema (OSTI)

Mdecine, climatologie, mtrologie et informatique, les techniques utilises par le LHC trouvent dj des rpercussions dans d?autres domaines scientifiques. Utilisant des techniques indites, la physique des particules en fait bnficier la socit toute entire.

None

2011-10-06T23:59:59.000Z

125

Introduction L'Encyclopdie des Carabes ou Encyclopdie des Kali'na du Suriname  

E-Print Network [OSTI]

Introduction « L'Encyclopédie des Caraïbes » ou Encyclopédie des Kali'na du Suriname Odile Renault Suriname, jusqu'à la deuxième moitié du 20ème siècle5, pour désigner les peuples et langues de famille étude comparée des langues de la famille caribe du Suriname, ainsi que des descriptions grammaticales et

Boyer, Edmond

126

DES Chapter 4DES Chapter 4 Estimating the Value of ACME  

E-Print Network [OSTI]

Estimate cost of capital (WACC) Debt Equity P j t fi i l t t t d FCFProject financial statements and FCF ACME has debt and equity The cost of capital for each type of financing depends on it riskDES Chapter 4DES Chapter 4 Estimating the Value of ACME DES Chapter 4 1 #12;Steps in a valuation

Schubart, Christoph

127

CONTRIBUTION L'TUDE DE LA GENSE DES SYSTMES D'INFORMATION COMPTABLE DES  

E-Print Network [OSTI]

) souffrent traditionnellement d'une carence au niveau des outils de gestion utiliss. Ce qui contribuerait intuition une analyse davantage formelle, avec diffrents outils de gestion (Chapellier, 1994). Aussi, le1 CONTRIBUTION L'TUDE DE LA GENSE DES SYSTMES D'INFORMATION COMPTABLE DES PME : UNE RECHERCHE

Paris-Sud XI, Universit de

128

Influence de la teneur en lignines des aliments sur la composition des digesta et la production  

E-Print Network [OSTI]

Note Influence de la teneur en lignines des aliments sur la composition des digesta et la essentiellement par leur teneur en lignines Van Soest : 7,4 ; 12,8 et 16 p. 100. Les contenus de l'estomac, de l trois heures, durant 24 heures. L'accroissement de la teneur en lignines des aliments augmente la teneur

Paris-Sud XI, Université de

129

argillacea huebner caterpillars: Topics by E-print Network  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Des Moines, IA Caterpillar Mossville, IL Caterpillar Peoria, IL Cerner Kansas City, MO Eaton Naperville, IL Procter &Gamble (Oral B) Iowa City, IA RISE-Cancer Research Center...

130

Solar Car  

SciTech Connect (OSTI)

Des Moines Central Academy Middle School students compete in the Solar Car Challenge at the National Science Bowl, May 2 in Washington D.C.

None

2010-01-01T23:59:59.000Z

131

The Araucaria Project. The Distance of the Large Magellanic Cloud from Near-Infrared Photometry of RR Lyrae Variables  

E-Print Network [OSTI]

We have obtained deep infrared $J$ and $K$ band observations of five fields located in the Large Magellanic Cloud (LMC) bar with the ESO New Technology Telescope equipped with the SOFI infrared camera. In our fields, 65 RR Lyrae stars catalogued by the OGLE collaboration were identified. Using different theoretical and empirical calibrations of the period-luminosity-metallicity relation, we find consistent LMC distance moduli values. Since the observed fields are situated very close to the center of the LMC, the correction for the tilt of the LMC bar with respect to the line of sight is negligible. Our adopted best true distance modulus to the LMC of $18.58 \\pm 0.03$ (statistical) $\\pm$ 0.11 (systematic) mag agrees very well with most independent determinations to this galaxy.

Olaf Szewczyk; Grzegorz Pietrzynski; Wolfgang Gieren; Jesper Storm; Alistair Walker; Luca Rizzi; Karen Kinemuchi; Fabio Bresolin; Rolf-Peter Kudritzki; Massimo Dall'Ora

2008-04-21T23:59:59.000Z

132

Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds  

E-Print Network [OSTI]

The EROS-2 project was designed to test the hypothesis that massive compact halo objects (the so-called ``machos'') could be a major component of the dark matter halo of the Milky Way galaxy. To this end, EROS-2 monitored over 6.7 years $33\\times10^6$ stars in the Magellanic clouds for microlensing events caused by such objects. In this work, we use only a subsample of $7\\times10^6$ bright stars spread over $84 \\deg^2$ of the LMC and $9 \\deg^2$ of the SMC. The strategy of using only bright stars helps to discriminate against background events due to variable stars and allows a simple determination of the effects of source confusion (blending). The use of a large solid angle makes the survey relatively insensitive to effects that could make the optical depth strongly direction dependent. Using this sample of bright stars, only one candidate event was found, whereas $\\sim39$ events would have been expected if the Halo were entirely populated by objects of mass $M\\sim0.4M_{\\odot}$. Combined with the results of EROS-1, this implies that the optical depth toward the Large Magellanic Cloud (\\object{LMC}) due to such lenses is $\\tau<0.36\\times10^{-7}$ (95%CL), corresponding to a fraction of the halo mass of less than 8%. This optical depth is considerably less than that measured by the MACHO collaboration in the central region of the LMC. More generally, machos in the mass range $0.6\\times10^{-7}M_\\odot

P. Tisserand; L. Le Guillou; C. Afonso; J. N. Albert; J. Andersen; R. Ansari; E. Aubourg; P. Bareyre; J. P. Beaulieu; X. Charlot; C. Coutures; R. Ferlet; P. Fouqu; J. F. Glicenstein; B. Goldman; A. Gould; D. Graff; M. Gros; J. Haissinski; C. Hamadache; J. de Kat; T. Lasserre; E. Lesquoy; C. Loup; C. Magneville; J. B. Marquette; E. Maurice; A. Maury; A. Milsztajn; M. Moniez; N. Palanque-Delabrouille; O. Perdereau; Y. R. Rahal; J. Rich; M. Spiro; A. Vidal-Madjar; L. Vigroux; S. Zylberajch

2007-04-19T23:59:59.000Z

133

Design Project -SIE 2010 Inventaire des missions  

E-Print Network [OSTI]

miscanthus Mise en place d'un outil d'aide la dcision pour la gestion des sites contamins: le cas de la gestion des parcelles de terrain contamines autour de l'ancienne usine de Metaleurop Nord en se: NOx, particules fines, Zn, Al, CO2, NH3 et Atrazine (pesticides) Mesures au niveau rgional Gestion

134

Anne Bamberg* Former des prtres Sourds  

E-Print Network [OSTI]

, Understanding Deaf Culture. In Search of Deafhood, Clevedon, Buffalo, Toronto, Sydney, Multilingual Matters Philippe Furtado, Le Père Agustin Yanes Valer prêtre sourd en Espagne, in Le lien des sourds catholiques et dans le monde et le Témoignage d'un prêtre sourd, in Le lien des sourds catholiques et de leurs amis, 9

Boyer, Edmond

135

Note d'information Contribution la matrise des problmes  

E-Print Network [OSTI]

Note d'information Contribution la matrise des problmes biologiques des stations d et priv (encadr ) qui se consacre la gestion des aspects biologiques des stations d'pu- ration'une tude de cas ; ou la mise en place d'tudes spcifiques sur un sujet qui le ncessite. Dans tous les cas

Boyer, Edmond

136

Untersuchungen zur Messung von Elektronen im au eren Randbereich des  

E-Print Network [OSTI]

, eine reduzierte Elektronenenergie gemessen. Die minimale Energie des gestreuten Elektrons tritt bei

137

Science du sol Le phosphore assimilable des sols : sa reprsentation  

E-Print Network [OSTI]

Science du sol Le phosphore assimilable des sols : sa représentation par un modèle fonctionnel à'échange isotopique des ions phosphate permet de démon- trer que le phosphore (P) biodisponible des sols est un des fertilisations excédentaires de phosphore modifient tous les compartiments. Cette représentation

Boyer, Edmond

138

E-Print Network 3.0 - avec des plasmas Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

DES PLASMAS A DEUX COMPOSANTES Summary: 'QUILIBRE DES PLASMAS A DEUX COMPOSANTES C. DEUTSCH Physique des Plasmas, Universit Paris-Sud, 91405 Orsay... , France Rsum. -- Les...

139

Etude des possibilits d'utilisation agronomique des composts d'ordures mnagres en milieu tropical (1)  

E-Print Network [OSTI]

Etude des possibilits d'utilisation agronomique des composts d'ordures mnagres en milieu'avre ncessaire uniquement en saison sche pour obtenir un compost dont le rapport C/N se situe autour de Ordures les composts des paysompos age. industrialiss. La proportion quilibre des oligo-lments et la

Paris-Sud XI, Universit de

140

A PROPOS DE L'HISTORICITE DES FORETS SACREES DE L'ANCIENNE COTE DES ESCLAVES  

E-Print Network [OSTI]

1 A PROPOS DE L'HISTORICITE DES FORETS SACREES DE L'ANCIENNE COTE DES ESCLAVES Dominique Juhé'autres nuancent cette opinion et signalent que, dans quelques cas, les bois sacrés ne sont pas des formations sources anciennes. Cette région est constituée de plateaux de basse altitude. Ils sont formés au Nord par

Boyer, Edmond

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

Fachprfungsordnung des Masterstudiengangs Health Care Management  

E-Print Network [OSTI]

Fachprfungsordnung des Masterstudiengangs Health Care Management an der Ernst-Moritz-Arndt-Universitt Greifs- wald die folgende Prfungsordnung fr den Masterstudiengang (M. Sc.) ,,Health Care Management Prfungsverfahren im Studiengang ,,Health Care Management". Ergnzend gilt die Gemeinsame Prfungsord- nung fr

Greifswald, Ernst-Moritz-Arndt-Universitt

142

FACULT DES SCIENCES HUMAINES ET SOCIALES -SORBONNE  

E-Print Network [OSTI]

FACULT? DES SCIENCES HUMAINES ET SOCIALES - SORBONNE MASTERS EN SCIENCES HUMAINES ET SOCIALES ANN?E UNIVERSITAIRE 2013-2014 MENTION SCIENCES DU LANGAGE ­ M1 ET M2 Spécialités > Linguistique et

Pellier, Damien

143

Differential Cryptanalysis of DES-like Cryptosystems  

E-Print Network [OSTI]

The Data Encryption Standard (DES) is the best known and most widely used cryptosystem for civilian applications. It was developed at IBM and adopted by the National Buraeu of Standards in the mid 70's, and has successfully withstood all the attacks published so far in the open literature. In this paper we develop a new type of cryptanalytic attack which can break the reduced variant of DES with eight rounds in a few minutes on a PC and can break any reduced variant of DES (with up to 15 rounds) in less than 2 56 operations. The new attack can be applied to a variety of DES-like substitution/permutation cryptosystems, and demonstrates the crucial role of the (unpublished) design rules.

Eli Biham; Adi Shamir

1991-01-01T23:59:59.000Z

144

Liste des Livres 2013 Group theory in physics : an introduction to symmetry  

E-Print Network [OSTI]

, MARTIN P., BIOTOPE EDITIONS, 2011 TU MOURRAS MOINS BETE. TOME 1: LA SCIENCE, C'EST PAS DU CINEMA mechanics with applications to nanotechnology and information science, Band Y.B., Avishai Y., Academic Press'impact on science. Solid state and liquid crystal. Vol 1, Bok J., Prost J., Brochard-Wyart F., World Scientific

Paris-Sud 11, Universit de

145

Chapitres Choisis de Theorie des Probabilites  

E-Print Network [OSTI]

;2 #12;Table des mati`eres Table des mati`eres 3 1 Le th´eor`eme limite local 5 1.1 La probl´ematique . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 1.2 ´Enonc´e du th´eor`eme limite local . . . . . . . . . . . . . . . . . . . . . . . . 5 1.3 Preuve du th´eor`eme limite local . . . . . . . . . . . . . . . . . . . . . . . . . 7 1.4 Br

Velenik, Yvan

146

Grosplansurl'anne desMathspourlaTerre  

E-Print Network [OSTI]

on le souhai tera ;c'estlatechniqueCAES(compressed air energy storage). « Pour le stockage à grande leur nombre, pour des raisons géographiques. Suivant la même logique, l'eau peut être remplacée par l'air primerl'air,quipourraêtredétenduulté rieurement dans des turbines afin de restituer l'électricité quand

Dambrine, Marc

147

Discovery of a peculiar Cepheid-like star towards the northern edge of the Small Magellanic Cloud  

E-Print Network [OSTI]

For seven years, the EROS-2 project obtained a mass of photometric data on variable stars. We present a peculiar Cepheid-like star, in the direction of the Small Magellanic Cloud, which demonstrates unusual photometric behaviour over a short time interval. We to report on data of the photometriy acquired by the MARLY telescope and spectroscopy from the EFOSC instrument for this star, called EROS2 J005135-714459(sm0060n13842), which resembles the unusual Cepheid HR 7308. The light curve of our target is analysed using the Analysis of Variance method to determine a pulsational period of 5.5675 days. A fit of time-dependent Fourier coefficients is performed and a search for proper motion is conducted. The light curve exhibits a previously unobserved and spectacular change in both mean magnitude and amplitude, which has no clear theoretical explanation. Our analysis of the spectrum implies a radial velocity of 104 km s$^{-1}$ and a metallicity of -0.4$\\pm$0.2 dex. In the direction of right ascension, we measure a...

Marquette, J B; Franois, P; Beaulieu, J P; Doublier, V; Lesquoy, E; Milsztajn, A; Pritchard, J; Schwarzenberg-Czerny, A; Afonso, C; Albert, J N; Andersen, J; Ansari, R; Aubourg, E; Bareyre, P; Charlot, X; Coutures, C; Ferlet, R; Fouqu, P; Glicenstein, J F; Goldman, B; Gould, A; Graff, D; Gros, M; Hassinski, J; Hamadache, C; De Kat, J; Guillou, L Le; Loup, C; Magneville, C; Maurice, E; Maury, A; Moniez, M; Palanque-Delabrouille, Nathalie; Perdereau, O; Rahal, Y R; Rich, J; Spiro, M; Vidal-Madjar, A; Zylberajch, S

2008-01-01T23:59:59.000Z

148

INFO-F-309 Administration des Systmes TP1: Installation de Linux et gestion des packages  

E-Print Network [OSTI]

INFO-F-309 Administration des Systmes TP1: Installation de Linux et gestion des packagesBox. Ensuite nous verrons comment fonctionne la gestion de packages, la mise jour du systme et l la gestion de packages. 2 Installation de Linux 2.1 Prparation Surtout lorsqu'il s'agit d'un serveur

Collette. Sbastien

149

Actes du colloque, fvrier 2003, Montpellier, France N Organisation spatiale et gestion des ressources et des  

E-Print Network [OSTI]

Actes du colloque, fvrier 2003, Montpellier, France N Organisation spatiale et gestion des l'origine d'une extrme diversit des scnarios d'volution : Le cas de la zone tampon de la rserve cas de la zone tampon de la rserve de U Minh Thong (delta du Mkong, Vietnam). L'objectif de ce

Boyer, Edmond

150

Bilan de la digestion des matires azotes du lait et des bactries cultives sur mthanol  

E-Print Network [OSTI]

Bilan de la digestion des matires azotes du lait et des bactries cultives sur mthanol la fin digestion at the end of the small intestine and the digestive tract of the preruminant calf. Two milk and synthetic amino acids (bacteria diet). Nine Friesian bull calves were used : digestibility was measured

Paris-Sud XI, Universit de

151

Contribution du gros intestin la digestion des glucides et des matires azotes chez le monogastrique omnivore  

E-Print Network [OSTI]

Contribution du gros intestin la digestion des glucides et des matires azotes chez le-en-Josas (France). Summary. Contribution of the large intestine to the digestion of carbohydrates and proteins in omnivorous simple-stomached animals. Owing to its special situation in relation to the rest of the digestive

Paris-Sud XI, Universit de

152

ISDA 2010, Montpellier 28-30 Juin 2010 1 CONTRIBUTIONS DES PARTENARIATS POUR  

E-Print Network [OSTI]

CONNAISSANCES AGRONOMIQUES SUR LA GESTION DE L'HERBE ET DEVELOPPER DES OUTILS ACTIONNABLES PAR DES CONSEILLERS'quipe Orphe (Outils modles et Rfrences Pour la gestion des systmes HErbagErs) produire des connaissancesISDA 2010, Montpellier 28-30 Juin 2010 1 CONTRIBUTIONS DES PARTENARIATS POUR CONCEVOIR DES

Boyer, Edmond

153

adsorption dans des: Topics by E-print Network  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

de Px par exemple ; Py s Paris-Sud XI, Universit de 48 Commande des liaisons HVDC dans un contexte reseau Physics Websites Summary: Commande des liaisons HVDC dans un...

154

CONTRIBUTION A L'TUDE DES COMPORTEMENTS DYSFONCTIONNELS  

E-Print Network [OSTI]

[1] CONTRIBUTION A L'TUDE DES COMPORTEMENTS DYSFONCTIONNELS DES AUDITEURS SENIORS : UNE APPROCHE MANAGRIALE (LE CAS FRANAIS) Ins GADDOUR, doctorante, Universit Paris-Dauphine, ines avoir un impact significatif sur tels comportements. Ensuite, nous tenterons d'identifier d

Paris-Sud XI, Universit de

155

absorption des wasserstoffs: Topics by E-print Network  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

. . . . . . . . 41 3.2.2 Kristallines Eis im Volumen Wolf, Martin 5 ABSORPTION PHOTOLECTRIQUE DES RAYONS 03B3 DANS LA COUCHE L DES ATOMES Par Mme NADINE MARTY....

156

Gocarrefour, n 84/4, 2009, pp. 229-239 Gohistoire/go-histoire : quelles mthodes pour quel rcit ?  

E-Print Network [OSTI]

-Marc Antoine*, Bertrand Desailly*, Anne Peltier* Introduction Les sources historiques, du moins dans les pays crue torrentielle, n'est plus dmontrer. Elle rejoint celle des repres de crues sur les faades des

Paris-Sud XI, Universit de

157

LETTRES A LA RDACTION DIFFUSION LASTIQUE DES PHOTONS  

E-Print Network [OSTI]

spectrometrie par scintillation 6choue, 6 cause des empilements de photons diffus6s de basse nergie. FIG. 1

Paris-Sud XI, Universit de

158

UNE BR`EVE HISTOIRE DES NOMBRES PHILIPPE LANGEVIN  

E-Print Network [OSTI]

'eologiques montrent que l'histoire ( occidentale ) des nombres prend source chez les 'egyp* *tiens et les babyloniens

Faccanoni, Gloria

159

Espace Populations Socits, numro spcial les temporalits des populations  

E-Print Network [OSTI]

-3 (2007) 305-316" #12;(Boulin et Mückenberger 2002). Des initiatives politiques, la mise en place de

Paris-Sud XI, Université de

160

Digestion des glucides chez le monogastrique Martine CHAMP  

E-Print Network [OSTI]

Digestion des glucides chez le monogastrique Martine CHAMP Laboratoire de Techno%gie des Aliments des Animaux, /. N. R.A., Rue de la Graudire, 44072 Nantes Cedex. Summary. Carbohydrate digestion digested in the small intestine of monogastric animals by enzymes of the salivary glands, pancreas

Paris-Sud XI, Universit 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.


161

PLC IMPLEMENTATION OF A DES SUPERVISOR FOR A MANUFACTURING  

E-Print Network [OSTI]

PLC IMPLEMENTATION OF A DES SUPERVISOR FOR A MANUFACTURING TESTBED: AN IMPLEMENTATION PERSPECTIVE Copyright by Ryan James Leduc 1996 #12;Title: PLC Implementation of A DES Supervisor for a Manufacturing, and issues involved in implementing DES supervisors on programmable logic controllers (PLC). A PLC based

Leduc, Ryan

162

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

SciTech Connect (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 (<4%), while carbon-rich AGB stars (especially the so-called extreme AGB stars) account for 87%-89% of the total dust input from cool evolved stars. We also estimate the dust input from hot stars and supernovae (SNe), and find that if SNe produce 10{sup -3} M{sub Sun} of dust each, then the total SN dust input and AGB input are roughly equivalent. We consider several scenarios of SN dust production and destruction and find that the interstellar medium (ISM) dust can be accounted for solely by stellar sources if all SNe produce dust in the quantities seen around the dustiest examples and if most SNe explode in dense regions where much of the ISM dust is shielded from the shocks. We find that AGB stars contribute only 2.1% of the ISM dust. Without a net positive contribution from SNe to the dust 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

163

Discovery of a peculiar Cepheid-like star towards the northern edge of the Small Magellanic Cloud  

E-Print Network [OSTI]

For seven years, the EROS-2 project obtained a mass of photometric data on variable stars. We present a peculiar Cepheid-like star, in the direction of the Small Magellanic Cloud, which demonstrates unusual photometric behaviour over a short time interval. We report on data of the photometry acquired by the MARLY telescope and spectroscopy from the EFOSC instrument for this star, called EROS2 J005135-714459(sm0060n13842), which resembles the unusual Cepheid HR 7308. The light curve of our target is analysed using the Analysis of Variance method to determine a pulsational period of 5.5675 days. A fit of time-dependent Fourier coefficients is performed and a search for proper motion is conducted. The light curve exhibits a previously unobserved and spectacular change in both mean magnitude and amplitude, which has no clear theoretical explanation. Our analysis of the spectrum implies a radial velocity of 104 km s$^{-1}$ and a metallicity of -0.4$\\pm$0.2 dex. In the direction of right ascension, we measure a proper motion of 17.4$\\pm$6.0 mas yr$^{-1}$ using EROS astrometry, which is compatible with data from the NOMAD catalogue. The nature of EROS2 J005135-714459(sm0060n13842) remains unclear. For this star, we may have detected a non-zero proper motion for this star, which would imply that it is a foreground object. Its radial velocity, pulsational characteristics, and photometric data, however, suggest that it is instead a Cepheid-like object located in the SMC. In such a case, it would present a challenge to conventional Cepheid models.

J. B. Marquette; P. Tisserand; P. Francois; J. P. Beaulieu; V. Doublier; E. Lesquoy; A. Milsztajn; J. Pritchard; A. Schwarzenberg-Czerny; C. Afonso; J. N. Albert; J. Andersen; R. Ansari; E. Aubourg; P. Bareyre; X. Charlot; C. Coutures; R. Ferlet; P. Fouque; J. F. Glicenstein; B. Goldman; A. Gould; D. Graff; M. Gros; J. Haissinski; C. Hamadache; J. de Kat; L. Le Guillou; C. Loup; C. Magneville; E. Maurice; A. Maury; M. Moniez; N. Palanque-Delabrouille; O. Perdereau; Y. R. Rahal; J. Rich; M. Spiro; A. Vidal-Madjar; S. Zylberajch

2008-05-29T23:59:59.000Z

164

VARIABILITY OF THE PULSED RADIO EMISSION FROM THE LARGE MAGELLANIC CLOUD PULSAR PSR J0529-6652  

SciTech Connect (OSTI)

We have studied the variability of PSR J0529-6652, a radio pulsar in the Large Magellanic Cloud (LMC), using observations conducted at 1390 MHz with the Parkes 64 m telescope. PSR J0529-6652 is detectable as a single pulse emitter, with amplitudes that classify the pulses as giant pulses. This makes PSR J0529-6652 the second known giant pulse emitter in the LMC, after PSR B0540-69. The fraction of the emitted pulses detectable from PSR J0529-6652 at this frequency is roughly two orders of magnitude greater than it is for either PSR B0540-69 or the Crab pulsar (if the latter were located in the LMC). We have measured a pulse nulling fraction of 83.3% {+-} 1.5% and an intrinsic modulation index of 4.07 {+-} 0.29 for PSR J0529-6652. The modulation index is significantly larger than values previously measured for typical radio pulsars but is comparable to values reported for members of several other neutron star classes. The large modulation index, giant pulses, and large nulling fraction suggest that this pulsar is phenomenologically more similar to these other, more variable sources, despite having spin and physical characteristics that are typical of the unrecycled radio pulsar population. The large modulation index also does not appear to be consistent with the small value predicted for this pulsar by a model of polar cap emission outlined by Gil and Sendyk. This conclusion depends to some extent on the assumption that PSR J0529-6652 is exhibiting core emission, as suggested by its simple profile morphology, narrow profile width, and previously measured profile polarization characteristics.

Crawford, F.; Altemose, D.; Li, H. [Department of Physics and Astronomy, Franklin and Marshall College, P.O. Box 3003, Lancaster, PA 17604 (United States)] [Department of Physics and Astronomy, Franklin and Marshall College, P.O. Box 3003, Lancaster, PA 17604 (United States); Lorimer, D. R. [Department of Physics, West Virginia University, Morgantown, WV 26506 (United States)] [Department of Physics, West Virginia University, Morgantown, WV 26506 (United States)

2013-01-10T23:59:59.000Z

165

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

166

soleil, parce que les pinceaux lumineux qui forment les images sont moins dlis et les foyers moins prcis.  

E-Print Network [OSTI]

AU PHNOMNE DE PELTIER; PAR M. BOUTY. 1. On sait que, quand on dcompose par la pile un sel dissous les phnomnes observs soit l'action chimique principale, soit une cause analogue celle qui part la pro- duction du courant que celle-l seule se distrib

Boyer, Edmond

167

Modlisation des meta-donnes bibliographiques : une contribution ins-trumente destine amliorer la circulation des usagers dans les  

E-Print Network [OSTI]

Modlisation des meta-donnes bibliographiques : une contribution ins- trumente destine .fr fabrice.papy@univ-paris8.fr Rsum La gestion des connaissances au sein des biblio- thques sociologue Francis Pav [Pav 89] a montr partir de cas concrets que ces prsupposs relevaient d'un forme

Boyer, Edmond

168

Phenomene couple thermo-hydro-mecanique des roches fracturees: Recents developpements des methodes de modelisation et tests de validation  

E-Print Network [OSTI]

95-54 Phenomene couple thermo-hydro-mecanique des roches fracturees: Recents developpements des methodes de modelisation et tests de validation Coupled thermo-hydro-mechanical phenomena in fractured fracture.La deuxiemequestion concemela modelisation des phenomenes couples thenno-hydro-mecaniques. L

Paris-Sud XI, Université de

169

Amtsblatt des Thringer Kultusministeriums und des Thringer Ministeriums fr Wissenschaft, Forschung und Kunst N r. 9/2002 Friedrich-Schiller-Universitt Jena  

E-Print Network [OSTI]

tritt am ersten Tage des auf ihre Veröffentlichung im Gemeinsamen Amtsblatt des Thüringer, Festkörperphysik, Kern- und Elementarteilchenphysik) an." 3. Diese ?nderung tritt am ersten Tage des auf ihre

Knüpfer, Christian

170

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

E-Print Network [OSTI]

tes dans les Annual Energy Outlook contrat en contrat etde 10 dans son Annual Energy Outlook de % par rapport aules prix son Annual Energy Outlook de 2003. terme pour des

Bolinger, Mark; Wiser, Ryan; Golove, William

2003-01-01T23:59:59.000Z

171

New Magellanic Cloud R Coronae Borealis and DY Per type stars from the EROS-2 database: the connection between RCBs, DYPers and ordinary carbon stars  

E-Print Network [OSTI]

R Coronae Borealis stars (RCB) are a rare type of evolved carbon-rich supergiant stars that are increasingly thought to result from the merger of two white dwarfs, called the Double degenerate scenario. This scenario is also studied as a source, at higher mass, of type Ia Supernovae (SnIa) explosions. Therefore a better understanding of RCBs composition would help to constrain simulations of such events. We searched for and studied RCB stars in the EROS Magellanic Clouds database. We also extended our research to DY Per type stars (DYPers) that are expected to be cooler RCBs (T~3500 K) and much more numerous than their hotter counterparts. The light curves of ~70 millions stars have been analysed to search for the main signature of RCBs and DYPers: a large drop in luminosity. Follow-up optical spectroscopy was used to confirm each photometric candidate found. We have discovered and confirmed 6 new Magellanic Cloud RCB stars and 7 new DYPers, but also listed new candidates: 3 RCBs and 14 DYPers. We estimated a...

Tisserand, P; Marquette, J B; Afonso, C; Albert, J N; Andersen, J; Ansari, R; Aubourg, E; Bareyre, P; Beaulieu, J P; Charlot, X; Coutures, C; Ferlet, R; Fouqu, P; Glicenstein, J F; Goldman, B; Gould, A; Gros, M; De Kat, J; Lesquoy, E; Loup, C; Magneville, C; Maurice, E; Maury, A; Milsztajn, A; Moniez, M; Palanque-Delabrouille, Nathalie; Perdereau, O; Rich, J; Schwemling, P; Spiro, M; Vidal-Madjar, A

2009-01-01T23:59:59.000Z

172

The VMC Survey - XIV. First results on the look-back time star-formation rate tomography of the Small Magellanic Cloud  

E-Print Network [OSTI]

We analyse deep images from the VISTA survey of the Magellanic Clouds in the YJKs filters, covering 14 sqrdeg (10 tiles), split into 120 subregions, and comprising the main body and Wing of the Small Magellanic Cloud (SMC). We apply a colour--magnitude diagram reconstruction method that returns their best-fitting star formation rate SFR(t), age-metallicity relation (AMR), distance and mean reddening, together with 68% confidence intervals. The distance data can be approximated by a plane tilted in the East-West direction with a mean inclination of 39 deg, although deviations of up to 3 kpc suggest a distorted and warped disk. After assigning to every observed star a probability of belonging to a given age-metallicity interval, we build high-resolution population maps. These dramatically reveal the flocculent nature of the young star-forming regions and the nearly smooth features traced by older stellar generations. They document the formation of the SMC Wing at ages <0.2 Gyr and the peak of star formation ...

Rubele, Stefano; Kerber, Leandro; Cioni, Maria-Rosa L; Piatti, Andres E; Zaggia, Simone; Bekki, Kenji; Bressan, Alessandro; Clementini, Gisella; de Grijs, Richard; Emerson, Jim P; Groenewegen, Martin A T; Ivanov, Valentin D; Marconi, Marcella; Marigo, Paola; Moretti, Maria-Ida; Ripepi, Vincenzo; Subramanian, Smitha; Tatton, Benjamin L; van Loon, Jacco Th

2015-01-01T23:59:59.000Z

173

Multi-Frequency Study of Supernova Remnants in the Large Magellanic Cloud. The case of LMC SNR J0530-7007  

E-Print Network [OSTI]

Context: The Supernova Remnants (SNRs) known in the Large Magellanic Cloud (LMC) show a variety of morphological structures in the different wavelength bands. This variety is the product of the conditions in the surrounding medium with which the remnant interacts and the inherent circumstances of the supernova event itself. Aims: This paper performs a multi-frequency study of the LMC SNR J0530-7007 by combining Australia Telescope Compact Array (ATCA), Molonglo Observatory Synthesis Telescope (MOST), R\\"ontgensatellit (ROSAT) and Magellanic Clouds Emission Line Survey (MCELS) observations. Methods: We analysed radio-continuum, X-ray and optical data and present a multi-wavelength morphological study of LMC SNR J0530-7007. Results We find that this object has a shell-type morphology with a size of 215"x180" (52 pc x 44 pc); a radio spectral index (alpha=-0.85+-0.13); with [Sii]/Halpha > 0.4 in the optical; and the presence of non-thermal radio and X-ray emission. Conclusions: We confirmed this object as a bona...

De Horta, A Y; Bozzetto, L M; Maggi, P; Haberl, F; Crawford, E J; Sasaki, M; Urosevi?, D; Pietsch, W; Gruendl, R; Dickel, J; Tothill, N F H; Chu, Y -H; Payne, J L; Collier, J D

2012-01-01T23:59:59.000Z

174

Plan d'action rgional pour la conservation des chimpanzs et des gorilles en Afrique Centrale Plan d'action rgional pour la conservation des chimpanzs  

E-Print Network [OSTI]

les lacunes en connaissances qu'il faut combler, à travers l'amélioration des méthodes de recensement par les chercheurs suggérant qu'ils avaient eu peu de contacts avec des humains auparavant. ©Nick gorilles de plaine d'Afrique Centrale. ©NickNichols,NGS #12;Plan d'action régional pour la conservation des

175

Studienordnung des Masterstudiengangs ,,Health Care Management"  

E-Print Network [OSTI]

1 Studienordnung des Masterstudiengangs ,,Health Care Management" an der Ernst-Moritz-Arndt-Universitt Greifswald die folgende Studienordnung fr den Masterstudiengang ,,Health Care Management" als Satzung Master- studiengang (M.Sc.) ,,Health Care Management" an der Ernst-Moritz-Arndt-Universitt Greifswald

Greifswald, Ernst-Moritz-Arndt-Universitt

176

Studienordnung des Masterstudiengangs ,,Health Care Management"  

E-Print Network [OSTI]

Studienordnung des Masterstudiengangs ,,Health Care Management" an der Ernst-Moritz-Arndt-Universitt Greifswald die fol- gende Studienordnung fr den Masterstudiengang ,,Health Care Manage- ment" als Satzung Masterstudiengang (M.Sc.) ,,Health Care Management" an der Ernst-Moritz- Arndt-Universitt Greifswald vom 15. Mrz

Greifswald, Ernst-Moritz-Arndt-Universitt

177

Service des finances Le saviez-vous ?  

E-Print Network [OSTI]

. La certification ISO 9001 atteste qu'une organisation a développé des pratiques de gestion qui responsable Penser autrement, acheter mieux ! L' Organisation internationale de normalisation (ISO) a publié durable dans une organisation : ISO 26 000 Responsabilité sociétale. Une organisation engagée envers le

178

Direction des bibliothques Bibliothque de chimie  

E-Print Network [OSTI]

lien suivant : https://origin-scifinder.cas.org/registration #12;6 N.B : II est obligatoire de s.ca. #12;7 Pour débuter: Cliquer sur le lien suivant et suivre les étapes : https « Search ». #12;10 La zone, ci-dessous contient des champs pour limiter ou affiner votre recherche. Les

Leclercq, Remi

179

INRA Laboratoire Croissance et Mtabolisme des Herbivores  

E-Print Network [OSTI]

'origine du mouvement, capable de transformer ' l'énergie des nutriments en force motrice. Enfin, c'est le sque- lette, et constituent le relais de la force motrice développée par le muscle. Ces différents

Paris-Sud XI, Université de

180

INSTABILITS DYNAMIQUES ET HYSTRSIS DES TRANSITIONS RSISTIVES  

E-Print Network [OSTI]

TYPE II A L'TAT MIXTE (*) F. P. PELTIER et J. BAIXERAS Laboratoire de Gnie Electrique des Universits monte du courant. (*) Ce travail fait partie de la Thse de Troisime Cycle soutenue par F. P. Peltier #12;68 toujours infrieure celle correspondant l'tat normal de l'chantillon et dans ce dernier

Paris-Sud XI, Universit 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.


181

Revue internationale des technologies en pdagogie universitaire  

E-Print Network [OSTI]

complexes ds que l'on s'affranchit de l'hypothse trs limitative des gaz parfaits. Il en rsulte que les simplement une turbine, un compresseur,une pompe,un changeur de chaleur,etc.,sans crire une seule quation

Paris-Sud XI, Universit de

182

THE INSIDIOUS BOOSTING OF THERMALLY PULSING ASYMPTOTIC GIANT BRANCH STARS IN INTERMEDIATE-AGE MAGELLANIC CLOUD CLUSTERS  

SciTech Connect (OSTI)

In the recent controversy about the role of thermally pulsing asymptotic giant branch (TP-AGB) stars in evolutionary population synthesis (EPS) models of galaxies, one particular aspect is puzzling: TP-AGB models aimed at reproducing the lifetimes and integrated fluxes of the TP-AGB phase in Magellanic Cloud (MC) clusters, when incorporated into EPS models, are found to overestimate, to various extents, the TP-AGB contribution in resolved star counts and integrated spectra of galaxies. In this paper, we call attention to a particular evolutionary aspect, linked to the physics of stellar interiors, that in all probability is the main cause of this conundrum. As soon as stellar populations intercept the ages at which red giant branch stars first appear, a sudden and abrupt change in the lifetime of the core He-burning phase causes a temporary 'boost' in the production rate of subsequent evolutionary phases, including the TP-AGB. For a timespan of about 0.1 Gyr, triple TP-AGB branches develop at slightly different initial masses, causing their frequency and contribution to the integrated luminosity of the stellar population to increase by a factor of ?2. The boost occurs for turn-off masses of ?1.75 M{sub ?}, just in the proximity of the expected peak in the TP-AGB lifetimes (for MC metallicities), and for ages of ?1.6 Gyr. Coincidently, this relatively narrow age interval happens to contain the few very massive MC clusters that host most of the TP-AGB stars used to constrain stellar evolution and EPS models. This concomitance makes the AGB-boosting particularly insidious in the context of present EPS models. As we discuss in this paper, the identification of this evolutionary effect brings about three main consequences. First, we claim that present estimates of the TP-AGB contribution to the integrated light of galaxies derived from MC clusters are biased toward too large values. Second, the relative TP-AGB contribution of single-burst populations falling in this critical age range cannot be accurately derived by approximations such as the fuel consumption theorem, which ignore, by construction, the above evolutionary effect. Third, a careful revision of AGB star populations in intermediate-age MC clusters is urgently demanded, promisingly with the aid of detailed sets of stellar isochrones.

Girardi, Lo [Osservatorio Astronomico di Padova-INAF, Vicolo dell'Osservatorio 5, I-35122 Padova (Italy); Marigo, Paola [Dipartimento di Fisica e Astronomia Galileo Galilei, Universit di Padova, Vicolo dell'Osservatorio 3, I-35122 Padova (Italy); Bressan, Alessandro [SISSA, via Bonomea 365, I-34136 Trieste (Italy); Rosenfield, Philip [Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195 (United States)

2013-11-10T23:59:59.000Z

183

Influence of the cosmological constant on the motion of Magellanic Clouds in the gravitational field of Milky Way  

SciTech Connect (OSTI)

Using the pseudo-Newtonian (PN) potential reflecting properties of the Schwarz-schild-de Sitter spacetime, we estimate the influence of the repulsive cosmological constant ? ? 1.3 10{sup ?56}cm{sup ?2} implied by recent cosmological tests onto the motion of both Small and Large Magellanic Clouds (SMC and LMC) in the gravitational field of the Milky Way. Considering detailed modelling of the gravitational field of the Galaxy disc, bulge and cold dark matter halo, the trajectories of SMC and LMC constructed for the PN potential with the cosmological constant are confronted to those given for ? = 0. In the realistic model of the extended cold dark matter halo its edge and related total mass are taken at typical values reflecting recent diversity in the total Galaxy mass estimates. In all cases, strong influence of the cosmological constant, on 10% level or higher, has been found for motion of both SMC and LMC. Inside the halo, the Newtonian part of the PN potential is exact enough, while outside the halo the PN potential can give relevant relativistic corrections. The role of the cosmological constant is most conspicuous when binding mass is estimated for the satellite galaxies. We have found a strong influence of cosmic repulsion on the total binding mass for both galaxies. For SMC there is the binding mass M{sub SMC}{sup ?=0} = 7.07 10{sup 11}M{sub ?} and M{sub SMC}{sup ?>0} = 8.61 10{sup 11}M{sub ?}, while even much higher increase is found for LMC, where M{sub LMC}{sup ?=0} = 1.50 10{sup 12}M{sub ?} and M{sub LMC}{sup ?} {sup >0} = 2.21 10{sup 12}M{sub ?}, putting serious doubts on the possibility that the LMC is bounded by the Milky Way. However, the estimates of binding masses are strongly influenced by initial velocity of SMC and LMC; we took the values inferred for the IAU MW rotation velocity ? 220 km/s. Our results indicate very important role of the cosmic repulsion in the motion of interacting galaxies, clearly demonstrated in the case of the satellite SMC and LMC galaxies moving in the field of Milky Way. In some cases, the effect of the cosmic repulsion can be even comparable to the effects of the dynamical friction and the Andromeda Galaxy.

Stuchlk, Zden?k; Schee, Jan, E-mail: zdenek.stuchlik@fpf.slu.cz, E-mail: jan.schee@fpf.slu.cz [Institute of Physics, Faculty of Philosophy and Science, Silesian University in Opava, Bezrucovo nm. 13, Opava (Czech Republic)

2011-09-01T23:59:59.000Z

184

Division de la gestion de documents et des archives Marie-Victorin au Qubec  

E-Print Network [OSTI]

Communiqu Division de la gestion de documents et des archives Marie-Victorin au Qubec Le 10 septembre 2011 -- La Division de la gestion de documents et des archives et la Direction des bibliothques s y verrez des paysages de la Gaspsie ou des photographies d'autochtones de la Cte-Nord ou de

Montral, Universit de

185

tude de la morbidit maternelle des populations rurales du Haut Atlas occidental marocain  

E-Print Network [OSTI]

dans le monde (UNICEF, 2008, p. 6). Au Maroc, le taux de mortalité maternelle demeure élevé et stable vulnérabilité au Maroc, Abdelmounaim ABOUSSAD, Mohamed CHERKAOUI et Patrice VIMARD (Ed.) (2010) 135-154" #12;M élevés dans les familles et les communautés les moins riches et les plus marginalisées. Au Maroc, malgré

Boyer, Edmond

186

rencontre du non-lineaire 2009 101 Effets d'un forcage spatial sur la dynamique des fronts  

E-Print Network [OSTI]

. Haudin1 , R. G. El´ias2 , M. G. Clerc2 ,, U. Bortolozzo1 , & S. Residori1 1 Institut Non Lin´eaire de´eris´ee par une propagation du front visant `a diminuer la taille du domaine le moins stable ´energ

Gavilan, Marcel G. Clerc

187

E-Print Network 3.0 - au calcul des Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

calcul des Search Powered by Explorit Topic List Advanced Search Sample search results for: au calcul des Page: << < 1 2 3 4 5 > >> 1 Les parties colores correspondent des actions...

188

E-Print Network 3.0 - avec des agents Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

agents Search Powered by Explorit Topic List Advanced Search Sample search results for: avec des agents Page: << < 1 2 3 4 5 > >> 1 Direction des Ressources Humaines Service des...

189

E-Print Network 3.0 - au cours des Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

des Search Powered by Explorit Topic List Advanced Search Sample search results for: au cours des Page: << < 1 2 3 4 5 > >> 1 HORAIRE DES COURS DU CERTIFICAT EN HORTICULTURE ET...

190

UNIVERSITE IBN TOFAIL FACULTE DES SCIENCES THESE DE DOCTORAT  

E-Print Network [OSTI]

Professeur à la Faculté des Sciences de Rabat - Maroc Président Mr . A. GAUDRY Ingénieur de recherche au de Meknès - Maroc Rapporteur Mr . A. CHOUKRI Professeur à la Faculté des Sciences de Kénitra - Maroc Examinateur Mr. S. CHAKIRI Professeur à la Faculté des Sciences de Kénitra - Maroc Examinateur Mr . M

Paris-Sud XI, Université de

191

Section des Units de recherche Rapport de l'AERES  

E-Print Network [OSTI]

Section des Unités de recherche Rapport de l'AERES sur l'unité : ELLIADD (?dition, Langages : Université de Franche-Comté Janvier 2011 #12;Section des Unités de recherche Rapport de l'AERES sur l Délégué scientifique représentant de l'AERES : M. Franck NEVEU Représentant(s) des établissements et

Jeanjean, Louis

192

PRINCIPALES CARACTERISTIQUES PHYSIONOMIQUES FLORISTIQUES DES FORMATIONS FORESTIERES  

E-Print Network [OSTI]

(MOYENNE COTE D'IVOIRE) par J.L. DEVINEAU SOMMAIRE RESUME/SUMMARY 275 INTRODUCTION 275 Les lambeaux scleroxylon. Dans la plupart des cas plusieurs strates peuvent y être distinguées. Les profils présentés ici°13' de latitude Nord, place la région de Lamto sous l'influence d'un climat équatorial de transition

Paris-Sud XI, Université de

193

The DES-Model and Its Applications  

E-Print Network [OSTI]

.3. Demand forecast models G 1.4. The European DESS-Model 8 2. ESSENTIALS OF THE DES-MODEL 10 2.1. Energy systems 58 6. PRIMARY ENERGY DEMAND AND ENERGY SYSTEM COSTS 59 6. 1. Energy demand forecasts 59 6.2. Fuel-pects of the technical and economic behaviour of existing and future energy systems, e.g. forecasting of energy demand

194

SECRETARIAT GENERAL Direction des ressources humaines  

E-Print Network [OSTI]

affaires générales, délégation Ile-de-France Ouest et Nord, - Séverine Rollet, responsable ressources des travaux de réhabilitation a débuté durant l'été - IDF Ouest et Nord : réorganisation entre restaurant de Meudon et celui de Verrières, plus d'autonomie du gérant de Verrières - Nord Est : lancement

Canet, Léonie

195

au seisme des: Topics by E-print Network  

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XI, Universit de 69 L'intgration des Supply chains Internationales impliques au Maroc : Le rle du contexte culturel. Physics Websites Summary: -organisationnelle occupe une...

196

au developpement des: Topics by E-print Network  

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XI, Universit de 96 L'intgration des Supply chains Internationales impliques au Maroc : Le rle du contexte culturel. Physics Websites Summary: -organisationnelle occupe une...

197

au traitement des: Topics by E-print Network  

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XI, Universit de 165 L'intgration des Supply chains Internationales impliques au Maroc : Le rle du contexte culturel. Physics Websites Summary: -organisationnelle occupe une...

198

au christianisme des: Topics by E-print Network  

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XI, Universit de 73 L'intgration des Supply chains Internationales impliques au Maroc : Le rle du contexte culturel. Physics Websites Summary: -organisationnelle occupe une...

199

au stockage des: Topics by E-print Network  

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XI, Universit de 82 L'intgration des Supply chains Internationales impliques au Maroc : Le rle du contexte culturel. Physics Websites Summary: -organisationnelle occupe une...

200

au respect des: Topics by E-print Network  

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XI, Universit de 71 L'intgration des Supply chains Internationales impliques au Maroc : Le rle du contexte culturel. Physics Websites Summary: -organisationnelle occupe une...

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201

au suivi des: Topics by E-print Network  

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MYCOPLASMA BOVIS : SUIVI PIDMIOLOGIQUE ET CLINIQUE DANS DES LEVAGES BOVINS LAITIERS AU MAROC Physics Websites Summary: INFECTION ? MYCOPLASMA BOVIS : SUIVI ?PID?MIOLOGIQUE...

202

au point des: Topics by E-print Network  

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XI, Universit de 99 L'intgration des Supply chains Internationales impliques au Maroc : Le rle du contexte culturel. Physics Websites Summary: -organisationnelle occupe une...

203

au niveau des: Topics by E-print Network  

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XI, Universit de 170 L'intgration des Supply chains Internationales impliques au Maroc : Le rle du contexte culturel. Physics Websites Summary: -organisationnelle occupe une...

204

au moyen des: Topics by E-print Network  

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205

au sein des: Topics by E-print Network  

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XI, Universit de 163 L'intgration des Supply chains Internationales impliques au Maroc : Le rle du contexte culturel. Physics Websites Summary: -organisationnelle occupe une...

206

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XI, Universit de 72 L'intgration des Supply chains Internationales impliques au Maroc : Le rle du contexte culturel. Physics Websites Summary: -organisationnelle occupe une...

207

au titre des: Topics by E-print Network  

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XI, Universit de 142 L'intgration des Supply chains Internationales impliques au Maroc : Le rle du contexte culturel. Physics Websites Summary: -organisationnelle occupe une...

208

au service des: Topics by E-print Network  

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XI, Universit de 116 L'intgration des Supply chains Internationales impliques au Maroc : Le rle du contexte culturel. Physics Websites Summary: -organisationnelle occupe une...

209

au voisinage des: Topics by E-print Network  

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210

au conditionnement des: Topics by E-print Network  

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XI, Universit de 74 L'intgration des Supply chains Internationales impliques au Maroc : Le rle du contexte culturel. Physics Websites Summary: -organisationnelle occupe une...

211

application des methodes: Topics by E-print Network  

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et entreprises connaissent un fort dveloppement des normes socio-techniques : norme ISO 9001, norme ISO 14000 etc ...Ces normes sont issues de travaux de rflexion...

212

applications des radioelements: Topics by E-print Network  

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occurs along the epitaxial direction. The comparison Silicium Sur Isolant (SSI, ou SOS : Silicon On Sapphire), matriau privilgi des circuits suhmi-...

213

application des isotopes: Topics by E-print Network  

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occurs along the epitaxial direction. The comparison Silicium Sur Isolant (SSI, ou SOS : Silicon On Sapphire), matriau privilgi des circuits suhmi-...

214

application diagnostic des: Topics by E-print Network  

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occurs along the epitaxial direction. The comparison Silicium Sur Isolant (SSI, ou SOS : Silicon On Sapphire), matriau privilgi des circuits suhmi-...

215

applications des procedes: Topics by E-print Network  

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occurs along the epitaxial direction. The comparison Silicium Sur Isolant (SSI, ou SOS : Silicon On Sapphire), matriau privilgi des circuits suhmi-...

216

application clinique des: Topics by E-print Network  

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occurs along the epitaxial direction. The comparison Silicium Sur Isolant (SSI, ou SOS : Silicon On Sapphire), matriau privilgi des circuits suhmi-...

217

application des fantomes: Topics by E-print Network  

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occurs along the epitaxial direction. The comparison Silicium Sur Isolant (SSI, ou SOS : Silicon On Sapphire), matriau privilgi des circuits suhmi-...

218

application des chargeurs: Topics by E-print Network  

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occurs along the epitaxial direction. The comparison Silicium Sur Isolant (SSI, ou SOS : Silicon On Sapphire), matriau privilgi des circuits suhmi-...

219

Jasper Johns in der Nachfolge des Ready-mades.  

E-Print Network [OSTI]

??Die Arbeit untersucht, wie die Einfhrung des Ready-mades in die Kunstwelt die Arbeitsweise von Knstlern sowie die Produktion und Wahrnehmung von Kunstwerken beeinflusst hat. Dies (more)

Mayer, Lynette Mildred

2013-01-01T23:59:59.000Z

220

aupres des piles: Topics by E-print Network  

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taient placs les dtecteurs. ?talonnage des canaux exprimentaux de la pile peuventtre . obturs compltement l'aide de blocs de graphite (dimen...

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,
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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


221

A L'INSTITUT NATIONAL DES SCIENCES APPLIQUEES DE ROUEN  

E-Print Network [OSTI]

PREMELANGE PAUVRE A HAUTE PRESSION APPLIQUEES AUX TURBINES A GAZ tel-00009334,version1-30May2005 #12;tel................................................................................................................... 15 I. 4 - DIMENSIONNEMENT DES TURBINES A GAZ

Paris-Sud XI, Universit de

222

Evaluierung geoelektrischer Tiefensondierungen im Neogen und Pleistozn des nrdlichen Burgenlandes.  

E-Print Network [OSTI]

??Im Rahmen der Diplomarbeit wurden nach einer Modellierung geoelektrischer Widerstandsmodelle mit dem Programm RES2DMOD vier geologisch unterschiedliche Bereiche des nrdlichen Burgenlandes mit der Methode der (more)

Kardeis, Gerald Ludwig

2009-01-01T23:59:59.000Z

223

ENTRE LIBRE INSCRIPTION OBLIGATOIRE 8 alle des platanes, 64100 Bayonne  

E-Print Network [OSTI]

EUROP?ENNES #12;MERCREDI 23 SEPTEMBRE 16H ACCUEIL DES PARTICIPANTS Jean-Louis GOUT, Président de l

Dambrine, Marc

224

!"#$%&'()&"*'+,"('+(-.'(/'(01$2,'+,%$+( !"#$%&!'#!'#()*+'"%#!'#,-cole des Mines de Nantes  

E-Print Network [OSTI]

-Marc Menaud, HdR, cole des Mines de Nantes M. Jean-Pierre Gudon, Professeur, cole Polytechnique de Nantes M

Paris-Sud XI, Université de

225

E-Print Network 3.0 - auftrag des bundesministeriums Sample Search...  

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und Arbeit... gefrdert sowie weiters mit Mitteln des Bundesministeriums fr Verkehr, Innovation und Technologie, des... - Live-Prsentation vor der ... Source: Breu, Ruth -...

226

E-Print Network 3.0 - association des physiologistes Sample Search...  

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des physiologistes Search Powered by Explorit Topic List Advanced Search Sample search results for: association des physiologistes Page: << < 1 2 3 4 5 > >> 1 Physiological systems...

227

E-Print Network 3.0 - arithmtiques des suites Sample Search Results  

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arithmtiques des suites Search Powered by Explorit Topic List Advanced Search Sample search results for: arithmtiques des suites Page: << < 1 2 3 4 5 > >> 1 TORSEURS ARITHMTIQUES...

228

E-Print Network 3.0 - analyse multidimensionnelle des Sample...  

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multidimensionnelle des Search Powered by Explorit Topic List Advanced Search Sample search results for: analyse multidimensionnelle des Page: << < 1 2 3 4 5 > >> 1 Seance 1:...

229

E-Print Network 3.0 - amelioration des performances Sample Search...  

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des performances Search Powered by Explorit Topic List Advanced Search Sample search results for: amelioration des performances Page: << < 1 2 3 4 5 > >> 1 Motivation Amelioration...

230

E-Print Network 3.0 - au comite des Sample Search Results  

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Collection: Computer Technologies and Information Sciences 2 Le 16 juin 2011 Curriculum Vitae Summary: des professeurs des universites) a l'Universite de Toulouse III du...

231

E-Print Network 3.0 - analyse des conceptions Sample Search Results  

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Centre de mathmatiques Collection: Mathematics 2 Ecole du dveloppement durable module 4 efficacit nergtique des btiments Efficacit et matrise nergtique des btiments...

232

E-Print Network 3.0 - adduits des produits Sample Search Results  

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de cyclisations radicalaires ...99 IV.2.1. Cyclisations radicalaires sur des adduits de Ugi ...100... 'addition-cyclisation base de thiophnol sur des adduits de Ugi contenant...

233

E-Print Network 3.0 - angulaire des particules Sample Search...  

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de fission... distributions de masse et de la distribution angulaire des fragments de fis- sion des noyaux lourds a t... - eurs expriences de la distribution ... Source:...

234

E-Print Network 3.0 - agricole geothermie des Sample Search Results  

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agricole geothermie des Search Powered by Explorit Topic List Advanced Search Sample search results for: agricole geothermie des Page: << < 1 2 3 4 5 > >> 1 CCOOLLEE...

235

DUSTY OB STARS IN THE SMALL MAGELLANIC CLOUD. II. EXTRAGALACTIC DISKS OR EXAMPLES OF THE PLEIADES PHENOMENON?  

SciTech Connect (OSTI)

We use mid-infrared Spitzer spectroscopy and far-infrared Herschel photometry for a sample of 20 main sequence O9-B2 stars in the Small Magellanic Cloud (SMC) with strong 24 {mu}m excesses to investigate the origin of the mid-IR emission. Either debris disks around the stars or illuminated patches of dense interstellar medium (ISM) can cause such mid-IR emission. In a companion paper, Paper I, we use optical spectroscopy to show that it is unlikely for any of these sources to be classical Be stars or Herbig Ae/Be stars. We focus our analysis on debris disks and cirrus hot spots. The local, prototype objects for these models are the debris disk around Vega and the heated dust cloud surrounding the stars in the Pleiades, also known as a cirrus hot spot. These two cases predict different dust masses, radii, origins, and structures, but the cleanest classification tools are lost by the poor physical resolution at the distance of the SMC. We also consider transition disks, which would have observable properties similar to debris disks. We begin classification by measuring angular extent in the highest resolution mid-IR images available. We find 3 out of 20 stars to be significantly extended, establishing them as cirrus hot spots. We then fit the IR spectral energy distributions to determine dust temperatures and masses. Analysis yields minimum grain sizes, thermal equilibrium distances, and the resultant dust mass estimates. We find the dust masses in the SMC stars to be larger than for any known debris disks. The difference in inferred properties is driven by the SMC stars being hotter and more luminous than known debris disk hosts and not in any directly observed dust properties, so this evidence against the debris disk hypothesis is circumstantial. Finally, we created a local comparison sample of bright mid-IR OB stars in the Milky Way (MW) by cross-matching the Wide-field Infrared Survey Explorer (WISE) and Hipparcos catalogs. We find that of the thousands of nearby ({<=}1 kpc) hot stars in the MW that show a mid-IR excess, only a small fraction (few percent) match the high mid-IR luminosities of the SMC stars. All such local stars in the appropriate luminosity range that can be unambiguously classified are young stars with optical emission lines or are spatially resolved by WISE with sizes too large to be plausible debris disk candidates. We conclude that the very strong mid-IR flux excesses are most likely explained as cirrus hot spots, although we cannot rigorously rule out that a small fraction of the sample is made up of debris disks or transition disks. We present suggestive evidence that bow-shock heating around runaway stars may be a contributing mechanism to the interstellar emission. These sources, interpreted as cirrus hot spots, offer a new localized probe of diffuse interstellar dust in a low metallicity environment.

Adams, Joshua J.; Simon, Joshua D. [Observatories of the Carnegie Institution of Science, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Bolatto, Alberto D. [Department of Astronomy, University of Maryland, College Park, MD 20742 (United States); Sloan, G. C. [Department of Astronomy, Cornell University, 222 Space Sciences Bldg., Ithaca, NY 14853-6801 (United States); Sandstrom, Karin M.; Schmiedeke, Anika [Max-Planck Institut fuer Astronomie, Koenigstuhl 17, D-69117, Heidelberg (Germany); Van Loon, Jacco Th.; Oliveira, Joana M. [School of Physical and Geographical Sciences, Lennard-Jones Laboratories, Keele University, Staffordshire, ST5 5BG (United Kingdom); Keller, Luke D., E-mail: jjadams@obs.carnegiescience.edu [Department of Physics, Ithaca College, Ithaca, NY 14850 (United States)

2013-07-10T23:59:59.000Z

236

Review of Discrete X-Ray Sources in the Small Magellanic Cloud: Summary of the ASCA Results and Implication on the Recent Star Forming Activity  

E-Print Network [OSTI]

We made 22 observations on the Small Magellanic Cloud (SMC) and covered full regions by the end of the ASCA mission. We detected 106 discrete sources with a criterion of S/N > 5 and performed systematic analyses on all of the sources. We determined the source positions with an ~40'' error radius (90% confidence) for sources detected in the central 20' radius of the GIS. We detected coherent pulsations from 17 sources. Among them, eight were newly discovered during this study. We classified most of these pulsars as X-ray binary pulsars (XBPs) based on their properties, such as the flux variability and the existence of an optical counterpart. We detected X-ray emission from eight supernova remnants (SNRs). Among them, five SNRs showed emission lines in their spectra, hence we regarded the five as thermal SNRs. We found that XBPs and thermal SNRs in the SMC can be clearly separated by their spectral hardness ratio. Applying this empirical law to faint (thus unclassified) sources, we found 19 XBP candidates and four thermal SNR candidates. We also found several tens of candidates for active galactic nuclei, both from the hardness ratio and the logN--logS relation of extragalactic sources. Based on these ASCA results and further information from other sattelites, we compiled comprehensive catalogues of discrete X-ray sources in the Small Magellanic Cloud. Using the catalogues, we derived the spatial distributions of XBPs and SNRs. XBPs and SNRs were found to be concentrated in the main body and eastern wing, which resembles the distribution of young stars with ages of ~2e7yr. By comparing the source populations in the SMC and our Galaxy, we suggest that the star-forming rate (per unit mass) in the SMC was much higher than the Galaxy 1e7yr ago. We also discuss the recent change of the star-forming rate in the SMC.

Jun Yokogawa; Kensuke Imanishi; Masahiro Tsujimoto; Katsuji Koyama; Mamiko Nishiuchi

2003-02-09T23:59:59.000Z

237

Unit de recherche Intelsig (Exploitation des signaux et des images) Dpartement d'Electricit, Electronique et Informatique  

E-Print Network [OSTI]

'installation des parcs éoliens marins, l'enfoncement des pylônes dans le fond marin génère des niveaux sonores très source. Tester et valider le code en propagation 2D et 3D en eaux profondes et peu profondes. Tester et valider le code par rapport à un ensemble de mesures in-situ qui seront mises à la disposition de l

Embrechts, Jean-Jacques

238

Sonie directionnelle en basse frquence Effet sur des sons purs latraliss uniquement par des diffrences de temps  

E-Print Network [OSTI]

Sonie directionnelle en basse fréquence Effet sur des sons purs latéralisés uniquement par des varie elle aussi en fonction de l'azimut. Ce phénomène est connu en tant que sonie directionnelle et variation de sonie observée pour différents azimuts était supérieure à ce qui pouvait être attendu des

Paris-Sud XI, Université de

239

ABSORPTION PHOTOLECTRIQUE DES RAYONS 03B3 DANS LA COUCHE L DES ATOMES Par Mme NADINE MARTY.  

E-Print Network [OSTI]

401. ABSORPTION PHOTO?LECTRIQUE DES RAYONS 03B3 DANS LA COUCHE L DES ATOMES Par Mme NADINE MARTY la suite, comme la section efficace totale d'absorption photoélectrique par atome. Les résultats de. Laboratoire dé Chimie nucléaire, Collège de France. Sommaire. - On rappelle la valeur des sections efficaces d'absorption

Boyer, Edmond

240

LA CAVITATION A L'ORIGINE DES BRUITS DU COEUR ET DES ACCIDENTS DE DCOMPRESSION EN PLONGE.  

E-Print Network [OSTI]

1 LA CAVITATION A L'ORIGINE DES BRUITS DU COEUR ET DES ACCIDENTS DE D?COMPRESSION EN PLONG?E. R'un phénomène de cavitation à l'origine des bruits de Korotkoff. Encouragés par l'aphorisme de MacDonald comme quoi le phénomène de cavitation est plus fréquent qu'on peut le penser dans le système cardio

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

La gestion des ports par une entit publique: aspects europens et environnementaux La gestion des ports par une entit publique  

E-Print Network [OSTI]

La gestion des ports par une entité publique: aspects européens et environnementaux « La gestion des ports par une entité publique: aspects européens et environnementaux » Thèse pour le Doctorat en,version1-25Apr2014 #12;La gestion des ports par une entité publique: aspects européens et environnementaux

Paris-Sud XI, Université de

242

Magellan Final Report  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: VegetationEquipment Surfaces and InterfacesAdministration -Lowell L.FallU . S . DMagellan Report on Cloud

243

Magellan-Tutorial.pptx  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: VegetationEquipment Surfaces and InterfacesAdministration -Lowell L.FallU . S . DMagellan Report

244

Mot du directeur Des ingnieurs humanistes, a existe!  

E-Print Network [OSTI]

des bacs de recyclage enfin réglé, l'adoption du Code de conduite des usagers de la Bibliothèque, et'aime plus particulièrement parce qu'il s'éloigne du strict bulletin de nouvelles. Les sujets que nous

Skorobogatiy, Maksim

245

Profils des entreprises en matire de RSE et innovation technologique  

E-Print Network [OSTI]

la nature de la relation entre la Responsabilité Sociale des Entreprises (RSE) et l'innovation : Innovation, PME, Responsabilité Sociale des Entreprises (RSE) Rachel BOCQUET - Caroline MOTHE hal-00950166 : Corporate Social Responsibility (CSR), Innovation, SME's hal-00950166,version1-25Feb2014 #12;3 Introduction

Boyer, Edmond

246

UNIVERSITE HASSAN I Settat Maroc FACULTE DES SCIENCES ET TECHNIQUES  

E-Print Network [OSTI]

UNIVERSITE HASSAN I ­ Settat ­ Maroc FACULTE DES SCIENCES ET TECHNIQUES ECOLE DOCTORALE DES Hassan I, Settat, Maroc Président du jury et Rapporteur M'hammed Said EL KEBBAJ Université Hassan II, Ben M'Sick, Casablanca, Maroc Examinateur Abdelaziz SOUKRI Université Hassan II, Ain Chock, Casablanca

Paris-Sud XI, Université de

247

presentee a L'ECOLE DES MINES DE PARIS  

E-Print Network [OSTI]

cette etude soit mis en valeur en m'initiant aux problemes speci ques de thermique des chercheurs du Centre d'Energetique de l'Ecole des Mines. Je les remercie de participer a ce jury. Parce qu'il a dechi

Paris-Sud XI, Université de

248

Explorer : des cls pour mieux comprendre la matire  

ScienceCinema (OSTI)

Le LHC va-t-il bouleverser les thories de l'infiniment petit ? Les physiciens aimeraient que l'acclrateur fasse trembler le modle standard. Cette thorie des particules lmentaires et des forces laisse de nombreuses zones d'ombre. Le LHC et ses expriences ont t conus pour les clairer.

None

2011-10-06T23:59:59.000Z

249

LIMITE SEMI-CLASSIQUE DES EQUATIONS DE SCHRODINGERPOISSON  

E-Print Network [OSTI]

. Introduction On s'int´eresse, pour ]0, 1] et x Rn , `a l'analyse BKW des ´equations : itu + 2 2 u = Vext(t, x´eveloppement BKW des ´equations de Schr¨odinger non-lin´eaires d´elicate. 1 #12;N´eanmoins, on dispose de nombreux

Alazard, Thomas

250

LES OUTILS DE CONTROLE DE GESTION DANS LE CONTEXTE DES  

E-Print Network [OSTI]

LES OUTILS DE CONTROLE DE GESTION DANS LE CONTEXTE DES PME : CAS DES PMI AU LIBAN Numro d diffrents outils de contrle de gestion utiliss dans les PMI libanaises et plus prcisment, d gestion outil de contrle calcul de cot Key words: SME - management control - cost control

Boyer, Edmond

251

Utilisation des Protocoles HARQ pour la Radio Cognitive  

E-Print Network [OSTI]

Utilisation des Protocoles HARQ pour la Radio Cognitive Romain Tajan encadré/01/2012 #12;Plan 1 Introduction 2 La Radio Cognitive Techniques de la Radio Cognitive Méthodes d'accès 3 performances du protocole IR-HARQ 4 Utilisation des protocoles HARQ pour la Radio Cognitive Utilisation de l

Dobigeon, Nicolas

252

PREVENTION DES EXPLOSIONS DE POUSSIERES ET PROTECTION CONTRE LEURS EFFETS  

E-Print Network [OSTI]

of prevention and protection of explosible atmospheres, including dust air mixtures. On the framework95-27 PREVENTION DES EXPLOSIONS DE POUSSIERES ET PROTECTION CONTRE LEURS EFFETS DIRECTIVES aujourd'hui des problemes de prevention et de protection en ce qui concerne les explosions d

Paris-Sud XI, Université de

253

Cours d't de franais 2013 PARC DES BASTIONS  

E-Print Network [OSTI]

RIVE JONCTION L'Arve M B D S PARC DES BASTIONS VIEILLE VILLE CIMETI?RE PLAINE DE PLAINPALAIS PONT HANS des périodes scolaires habituelles. Il s'agis- sait également du premier exemple de formation continue

Citi, Sandra

254

Valorisation des MIOM3 en technique routiere : suivi environnemen-  

E-Print Network [OSTI]

de MIOM de la gamme Scormat®. 1. INTRODUCTION Le Mächefer d'Incineration d'Ordures Menageres est l'incineration des ordures menageres, represente 25 ä 30 % en masse des dechets menagers incineres an (caicule sur la masse totale de dechets incineres - source ADEME 1999). ·3 MIOM : Mächefer d'Incineration d

Paris-Sud XI, Université de

255

INSTITUT DES SCIENCES ET TECHNOLOGIES cole doctorale nO  

E-Print Network [OSTI]

) Les performances des moteurs combustion interne sont limites par la quantit de gaz que leur tudes de cas : un turbocompresseur gomtrie fixe sur un moteur essence, une turbine gomtrie variable sur un moteur Diesel avec deux circuits de recirculation des gaz brls, et un turbocompresseur

Paris-Sud XI, Universit de

256

APPLICATION DES PALIERS A GAZ AUX GYROSCOPES Par G. GOBERT,  

E-Print Network [OSTI]

43 APPLICATION DES PALIERS A GAZ AUX GYROSCOPES Par G. GOBERT, Centre d'tudes Nuclaires de Saclay. Rsum. 2014 L'tude des frottements dans les paliers lubrification par gaz permet de cons- truire un avec, au centre, une turbine raction. Ces rotors sont placs entre deux butes coniques mtalliques

Paris-Sud XI, Universit de

257

Direktion des Innern Amt fr Wald und Wild  

E-Print Network [OSTI]

Direktion des Innern Amt für Wald und Wild Veranstaltungsreihe Forum Wild "Projet Lac Zugersee" Im Zug Aabachstrasse 5, Zug Veranstaltungsreihe Forum Wild "Projet Lac Zugersee" Im August 2013 hat ein, Zug Direktion des Innern Amt für Wald und Wild #12;

Wehrli, Bernhard

258

Ouverture des portes : Plonge dans le Grand Bleu... Activits libres  

E-Print Network [OSTI]

Ouverture des portes : Plongée dans le Grand Bleu... Activités libres : · Présentations de nos ... Fermeture des portes 10h En Continu 17h 10h - 12h 14h - 15h 17h 15h - 17h Samedi 10 mai 2014 Portes ouvertes

259

Dgradabilit compare dans le rumen des diffrentes fractions azotes des feuilles  

E-Print Network [OSTI]

bout de 1, 3, 6, 9, 15, 24 et 48 h. Après lavage et séchage à 60 °C, on a dosé dans le résidu l dégradation des fractions NDF et AFD du foin sont prati- quement identiques. Les cinétiques de dégradation de

Boyer, Edmond

260

Traitement Automatique des Langues Naturelles, Marseille, 2014 RENAM: Systme de Reconnaissance des Entits Nommes Amazighes  

E-Print Network [OSTI]

1 (1) LRIT, Unité Associée au CNRST (URAC 29), Faculté des Sciences, Mohammed V-Agdal, Rabat, Maroc (2) IRCAM, Avenue Allal El Fassi, Madinat Al Irfane, Rabat-Instituts, Maroc meriem 1989) qu'on soit au Maroc ou ailleurs. La langue Amazighe est maintenant une langue qui possède tous

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

LA REGULATION DU STATIONNEMENT ET DES CIRCULATIONS AUTOMOBILES EN VILLE : DES POLITIQUES SOUTERRAINES D'ATTRACTIVIT AU COTS  

E-Print Network [OSTI]

LA REGULATION DU STATIONNEMENT ET DES CIRCULATIONS AUTOMOBILES EN VILLE : DES POLITIQUES circulations automobiles en ville et sur les ambitions partagées de ces politiques urbaines. Alors qu de l'automobile, nous souhaitons aborder la manière dont ces politiques urbaines prennent en compte

Paris-Sud XI, Université de

262

Proposition de sujet de Thse de Doctorat Caractrisation multi chelle des proprits hydro-go-physiques des  

E-Print Network [OSTI]

Proposition de sujet de Thèse de Doctorat Caractérisation multi échelle des propriétés hydro structurales et ainsi développer des méthodologies d'acquisition hydro-géo-physique en ce milieu complexe

Naud Frédéric

263

Reseaux des groupes de Lie (Version preliminaire)  

E-Print Network [OSTI]

Cartan. - Exemples de r´eseaux. - M´elange. Th´eor`eme de Howe-Moore. - Comptage de points dans les r´eseaux. Th´eor`eme d'Eskin-McMullen. - Vari´et´e drapeau. Th´eor`eme de Furstenberg. - Repr´esentation des r´eseaux. Th´eor`eme de superrigidit´e de Margulis. - Corps locaux. Th´eor`eme d'arithm´eticit´e de Margulis

Wienhard, Anna

264

Utilisations thrapeutiques des interfaces cerveau-ordinateur  

E-Print Network [OSTI]

motrice (contrôle par la pensée d'une orthèse, d'une prothèse ou d'un robot). Il apparaît aujourd'hui que'aide à la rééducation motrice par un patient atteint d'une hémiplégie du coté droit. Index Terms supplémentaire vers l'extérieur, par le biais de l'activité cérébrale, pour : restaurer des fonctions motrices

Paris-Sud XI, Université de

265

Un modle formel pour la gestion des connaissances J.-L. Ermine  

E-Print Network [OSTI]

- 1 - Un modle formel pour la gestion des connaissances J.-L. Ermine Management et ingnierie des connaissances, modles et mthodes Trait IC2, Srie Management et Gestion des STIC Hermes-Lavoisier, 2008 hal'alignement stratgique de la gestion des connaissances 1. Introduction Pendant de nombreuses annes, la recherche en

Boyer, Edmond

266

La gestion du manque d'eau structurel et des scheresses en France  

E-Print Network [OSTI]

La gestion du manque d'eau structurel et des scheresses en France La France est rgulirement et demande en eau se sont crs. Des politiques et dispositifs de gestion des scheresses et du politiques. Il propose des adaptations qui incluent une meilleure gestion de crise, l'introduction de droits

Boyer, Edmond

267

TRAITEMENT COMPTABLE DES DEPENSES DE R&D ET MOTIVATIONS DE GESTION  

E-Print Network [OSTI]

1 TRAITEMENT COMPTABLE DES DEPENSES DE R&D ET MOTIVATIONS DE GESTION DES RESULTATS : UNE ETUDE EMPIRIQUE SUR DES ENTREPRISES FRAN?AISES COTEES Sana TRIKI DAMAK, Doctorante en comptabilité, UR : COFFIT développement (R&D) est un sujet controversé qui pourrait être, dans certains cas, motivé par des incitations à

Paris-Sud XI, Université de

268

Institut de Chimie et des Matriaux Paris-Est UMR 7182  

E-Print Network [OSTI]

prparation des chantillons ; Patrick Ochin, Christian Jolivet Michel Parise et Jean-Louis Bonnentien pour l

269

Quelle est l'attitude actuelle des PMI franaises l'gard  

E-Print Network [OSTI]

Quelle est l'attitude actuelle des PMI franaises l'gard des pratiques de planification? Cette cadre d'analyse pertinent susceptible de faciliter l'observation des pratiques dans les PMI. partir d'article dbouche sur un essai de classification typologique des PMI en fonction de leurs attitudes et de leurs

Boyer, Edmond

270

Variations des stratgies d'anticipation visuelle en fonction de la rgle dans un jeu vido  

E-Print Network [OSTI]

partagées avec l'ensemble des environnements virtuels (Stanney, Mollaghasemi, Reeves, Breaux, & Graeber

Paris-Sud XI, Université de

271

GROUPES DE SYMETRIE EN PHYSIQUE (des hautes energies). Approfondissement PHY 575  

E-Print Network [OSTI]

´ematique et une partie physique. 1 #12;Plan des cours: ´EL´EMENTS DE TH´EORIE DES GROUPES POUR PHYSICIENSGROUPES DE SYM´ETRIE EN PHYSIQUE (des hautes ´energies). Approfondissement PHY 575 Denis Bernard et David Renard Le but de cet enseignement est de reprendre certains th`emes du cours de physique des

Renard, David

272

Impacts historiques de la colonisation  

E-Print Network [OSTI]

of Europeans. #12; Holocene extinction of 19 species of birds. PNAS (1987) 84: 2350-2354 #12;Colonisation majorit des espces n'appartiennent aucun des groupes actuels ou ancestraux connus ! #12;Extinction L'extinction de nouvelles espces #12;Au moins 5 extinctions Extinction des dinosaures Extinction de 76-96% des

Blouin-Demers, Gabriel

273

Peltier A., 2008, La cartographie rglementaire des risques naturels en Suisse, en Italie et en France , La mise en carte des risques naturels, Diversit des approches, Montpellier : Presses Universitaires de la Mditerrane,  

E-Print Network [OSTI]

Peltier A., 2008, La cartographie rglementaire des risques naturels en Suisse, en Italie et en (2008) 61-67" #12;Peltier A., 2008, La cartographie rglementaire des risques naturels en Suisse, en

Paris-Sud XI, Universit de

274

RINNERVATION D'UN MUSCLE STRI PAR DES FIBRES PRGANGLIONNAIRES PARASYMPATHIQUES.  

E-Print Network [OSTI]

du lieu d'émer- gence du nerf récurrent, le diaphragme a été réinnervé par des fibres motrices des plaques motrices sur ce muscle ;J 3) ces plaques motrices sont fonctionnelles ; 4) l'activité des sur des fibres musculaires striées. L'activité électrique des unités motrices réinnervées peut être

Boyer, Edmond

275

Les marchands orientaux et les langues occidentales au XVIIe sicle : l'exemple des Choffelins de Marseille  

E-Print Network [OSTI]

1 Les marchands orientaux et les langues occidentales au XVIIe siècle : l'exemple des « Choffelins » de Marseille La question des marchands et des langues à l'époque moderne est loin d'être un domaine la question des marchands et des langues dans le commerce de moyenne et longue distances. Le but de

Paris-Sud XI, Université de

276

Conservatoire national des Arts et Mtiers Prsente au Conservatoire national des Arts et Mtiers  

E-Print Network [OSTI]

cellulaire et l'apoptose (cytométrie de flux) dans les lignées cellulaires de cancer du sein MCF-7 (RE+, RE cellules (transactivation) et dans des cellules négatives pour les REs nucléaires SKBr3 (GPR30+) (études de les cellules MCF-7 et MDA-MB-231 associés à une inhibition de la prolifération et un arrêt du cycle

Paris-Sud XI, Université de

277

Linarisation des amplificateurs de puissance par pr-distorsion avec prise en compte des effets mmoire  

E-Print Network [OSTI]

mémoire Geneviève BAUDOIN1, Pascale JARDIN1, Roman MARSALEK1,2 1ESYCOM - ESIEE - Laboratoire des Signaux effets de mémoire. Abstract ­ We present a baseband adaptive pre-distorion technique to linearize power-distortion system that is applied as a pre-distortion. The form of the pre-distorter is a polynomial with memory

Baudoin, Geneviève

278

Dtermination du rgime des bovins exploitant des parcours agropastoraux soudano-sahliens (Sngal)  

E-Print Network [OSTI]

the proportion of plant epiderms in the faeces. The proportions plants epiderms in faeces of cattle were found «traces» avec une contribution spécifique présence (CSP : proportion en pourcentage du nombre total de'une plante donnée varie avec la méthode de préparation des lames (fig 1): les monocotylédones appa- raissent

Boyer, Edmond

279

Mathmatiques et interactions des mathmatiques Participation des lus C aux valutations de l'AERES  

E-Print Network [OSTI]

évalutations de l'AERES La section 41 du comité national, lors de sa première réunion du nouveau mandat, demande par cette motion aux présidents de comités d'AERES d'intégrer systématiquement dans les comités de, directeur de la section des unités à l'AERES. #12;

Pouyanne, Nicolas

280

HYPOTHSES SUR L'ORIGINE DES BRUITS DU COEUR ET DES ACCIDENTS DE DCOMPRESSION EN PLONGE : LA CAVITATION.  

E-Print Network [OSTI]

CAVITATION. HYPOTH?SE SUR L'ORIGINE DE LA FERMETURE DES VALVES CARDIAQUES : LE RETARD ? LA FERMETURE DES un travail antérieur, l'hypothèse d'un phénomène de cavitation à l'origine des bruits de Korotkoff. Encouragés par l'aphorisme de MacDonald comme quoi le phénomène de cavitation est plus fréquent qu'on peut le

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.


281

Optical and X-ray variability of two Small Magellanic Cloud X-ray binary pulsars - SXP46.6 and SXP6.85  

E-Print Network [OSTI]

We present long-term optical and RXTE data of two X-ray binary pulsars in the Small Magellanic Cloud, SXP46.6 and SXP6.85. The optical light curves of both sources show substantial (~0.5-0.8 mag) changes over the time span of the observations. While the optical data for SXP6.85 do not reveal any periodic behaviour, by detrending the optical measurements for SXP46.6 we find an orbital period of ~137 days, consistent with results from the X-ray data. The detection of Type I X-ray outbursts from SXP46.6, combined with the fact that we also see optical outbursts at these times, implies that SXP46.6 is a high orbital eccentricity system. Using contemporaneous optical spectra of SXP46.6 we find that the equivalent width of the H_alpha emission line changes over time indicating that the size of the circumstellar disc varies. By studying the history of the colour variations for SXP6.85 we find that the source gets redder as it brightens which can also be attributed to changes in the circumstellar disc. We do not find any correlation between the X-ray and optical data for SXP6.85. The results for SXP6.85 suggest that it is a low eccentricity binary and that the optical modulations are due to the Be phenomenon.

K. E. McGowan; M. J. Coe; M. P. E. Schurch; R. H. D. Corbet; J. L. Galache; A. Udalski

2007-11-26T23:59:59.000Z

282

Multi-frequency study of Local Group Supernova Remnants The curious case of the Large Magellanic Cloud SNR J0528-6714  

E-Print Network [OSTI]

Aims. Recent ATCA, XMM-Newton and MCELS observations of the Magellanic Clouds (MCs) cover a number of new and known SNRs which are poorly studied, such as SNR J0528-6714 . This particular SNR exhibits luminous radio-continuum emission, but is one of the unusual and rare cases without detectable optical and very faint X-ray emission (initially detected by ROSAT and listed as object [HP99] 498). We used new multi-frequency radio-continuum surveys and new optical observations at H{\\alpha}, [S ii] and [O iii] wavelengths, in combination with XMM-Newton X-ray data, to investigate the SNR properties and to search for a physical explanation for the unusual appearance of this SNR. Methods. We analysed the X-ray and Radio-Continuum spectra and present multi-wavelength morphological studies of this SNR. Results. We present the results of new moderate resolution ATCA observations of SNR J0528-6714. We found that this object is a typical older SNR with a radio spectral index of {\\alpha}=-0.36 \\pm 0.09 and a diameter of D...

Crawford, E J; Haberl, F; Pietsch, W; Payne, J L; De Horta, A Y

2010-01-01T23:59:59.000Z

283

Design, implementation, and on-sky performance of an advanced apochromatic triplet atmospheric dispersion corrector for the Magellan adaptive optics system and VisAO camera  

E-Print Network [OSTI]

We present the novel design, laboratory verification, and on-sky performance of our advanced triplet atmospheric dispersion corrector (ADC), an important component of the Magellan Adaptive Optics system (MagAO), which recently achieved first light in December 2012. High-precision broadband (0.5-1.0 microns) atmospheric dispersion correction at visible wavelengths is essential both for wavefront sensing (WFS) on fainter guide stars, and for performing visible AO science using our VisAO science camera. At 2 airmasses (60 degrees from zenith) and over the waveband 500-1000 nm, our triplet design produces a 57% improvement in geometric rms spot size, a 33% improvement in encircled energy at 20 arcsec radius, and a 62% improvement in Strehl ratio when compared to a conventional doublet design. This triplet design has been fabricated, tested in the lab, and integrated into the MagAO WFS and the VisAO science camera. We present on-sky results of the ADC in operation with the MagAO system. We also present a zero-beam...

Kopon, Derek; Males, Jared R; Gasho, Victor

2013-01-01T23:59:59.000Z

284

Etude des interactions entre services des cosystmes Rives, F.; Antona, M.; Aubert, S.;Carrire, S.;Ichaou, A.; Montagne, P; Peltier R.; Sibelet, N.  

E-Print Network [OSTI]

.;Ichaou, A.; Montagne, P; Peltier R.; Sibelet, N. ISDA 2010, Montpellier, June 28-30, 2010 1 ETUDE DES , Aboubacar ICHAOU5 , Pierre MONTAGNE6 , Rgis PELTIER7 , Nicole SIBELET8 1 Unit de recherche Gestion des services des cosystmes Rives, F.; Antona, M.; Aubert, S.;Carrire, S.;Ichaou, A.; Montagne, P; Peltier R

Paris-Sud XI, Universit de

285

Votre t petit prix !!! Depuis 60 ans au service des vacances familles et enfants, Vacances Pour Tous propose une autre ide des vacances !  

E-Print Network [OSTI]

4 Mai 2012 Votre été à petit prix !!! Depuis 60 ans au service des vacances familles et enfants, Vacances Pour Tous propose une autre idée des vacances ! Nos équipes vous proposent des vacances en villages vacances, locations, campings en France et à l'étranger mais aussi le plus grand choix de

Arleo, Angelo

286

IMPORTANCE DE LA PARAMETRISATION HYDRODYNAMIQUE DES PREMIERS CENTIMETRES DU SOL  

E-Print Network [OSTI]

'une saison sèche et d'une saison des pluies. Au cours de la saison sèche, le vent dominant est l'Harmattan

287

eefnparticipants Academie Royale des Sciences de Su`ede  

E-Print Network [OSTI]

.grazzini@inria.fr Ph.D. student: image processing, meteorological and pollution models. AIR Project, INRIA Rocquencourt`ere. Jean Serra, ´Ecole des Mines. serra@cmm.ensmp.fr Professor, Member of the Organizing Committee, Invited

Kiselman, Christer

288

Amlioration des plantes Une contribution la slection simultane  

E-Print Network [OSTI]

Amlioration des plantes Une contribution la slection simultane sur plusieurs caractres : l programmation linaire, outil mathmatique souvent utilis en recherche oprationnelle, permet de complter l Summary A contribution to multitrait selection: the use of linear programming. Linear programming

Boyer, Edmond

289

Contribution phytocologique et dynamique l'tude des cosystmes forestiers.  

E-Print Network [OSTI]

Contribution phytocologique et dynamique l'tude des cosystmes forestiers. Applications aux forts du Nord-Est de la France J.-C. RAMEAU Phytocologie forestire l'E.N.GProfesseur de

Boyer, Edmond

290

au test des: Topics by E-print Network  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

au test des First Page Previous Page 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 Next Page Last Page Topic Index 1 INSTITUTNATIONALDESSCIENCESAPPLIQUESDELYON...

291

"Sauver la nuit" : empreinte lumineuse, urbanisme et gouvernance des territoires.  

E-Print Network [OSTI]

??Notre socit entretient une relation complexe avec la nuit, espace-temps souvent hors des cadences diurnes qui favorise la rflexion, limaginaire, la cration, lcoute et le (more)

Challat, Samuel

2010-01-01T23:59:59.000Z

292

Teilnehmer des deutsch-ukrainisch-polnischen Seminars in Tscherniwzi 2012  

E-Print Network [OSTI]

Teilnehmer des deutsch-ukrainisch-polnischen Seminars in Tscherniwzi 2012 BAYHOST & die Ukraine. Gefördert durch den DAAD veranstaltete BAYHOST zwei Deutsch - Ukrainische Seminare, die sich dem Thema

Schubart, Christoph

293

Nr. 142 / 2011 // 28. Juli 2011 Gewinner des Malwettbewerbs der  

E-Print Network [OSTI]

Bayreuth, Dr. Markus Zanner, Angela Danner, der persönlichen Referentin des Präsidenten, Professor Anno. Markus Zanner und Angela Danner) 737 Zeichen 15 Zeilen ca. 60 Anschläge/Zeile Abdruck honorarfrei #12;

Ullmann, G. Matthias

294

Valley wins High School Science Bowl | The Ames Laboratory  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Valley wins High School Science Bowl West Des Moines Valley defeated Bettendorf 72-32 in the championship match to win the 25th Ames LaboratoryIowa State University Regional High...

295

Labsolu rugissement dbraill dune absence insense de la mtaphore Poetry, photography, eroticism  

E-Print Network [OSTI]

capacit sexuelle)). Des reprsentations porno doivent donc maner quelques stimuli qui nous touchent en sorte quon soit comme aspirs (au moins momentanment) vers une vrit matrielle, phnomnale et qui transcende la reprsentation, sort delle et...

Khalfa, Jean

2014-01-01T23:59:59.000Z

296

E-Print Network 3.0 - apollo landing sites Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

2004 12;20 CHAPITRE 1. LES MISSIONS D'EXPLORATION DE LA LUNE Fig. 1.4 - Carte des sites Luna, Apollo... dans la region du cratere Fra Mauro, a moins de 200 km du site ......

297

Ecole Polytechnique de Bruxelles -Facult des Sciences SOLVAY AWARDS 2013  

E-Print Network [OSTI]

Ecole Polytechnique de Bruxelles - Faculté des Sciences SOLVAY AWARDS 2013 Informations sur le dossier à transmettre et la procédure à suivre Objectif Le Groupe Solvay décerne annuellement un Prix, dénommé « SOLVAY AWARDS » à des diplômés scientifiques clôturant un deuxième cycle universitaire (Master

Cerf, Nicolas

298

Des frontires du corps aux frontires de l'identit  

E-Print Network [OSTI]

incapacités motrices majeures Thèse soutenue le 21 octobre 2013 devant le jury composé de : David LE BRETON'une vie au quotidien avec des incapacités motrices majeures - 2013 tel-00904373,version1-14Nov2013 #12'EXPERIENCE D'UNE VIE AU QUOTIDIEN AVEC DES INCAPACITES MOTRICES MAJEURES Thèse de Doctorat Discipline

Paris-Sud XI, Université de

299

Cryptanalysis of S-DES Dr. K. S. Ooi  

E-Print Network [OSTI]

recovery. Other forms of security threat do exist, for example: identity theft, cyber stalking and cyber-DES Results 8.8 Difference Pair Table of S0 8.9 Difference Pair Table of S1 8.10 Difference Distribution Table of S0 8.11 Difference Distribution Table of S1 8.12 Differential Characteristic of S-DES 8.13 I/0 Table

Babinkostova, Liljana

300

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

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

Commande des liaisons HVDC dans un contexte reseau  

E-Print Network [OSTI]

Commande des liaisons HVDC dans un contexte r´eseau Leyla Arioua , Bogdan Marinescu , Eric´esum´e : Maintes solutions ont ´et´e propos´ees afin de contr^oler les liaisons `a courant continu (HVDC Matlab ainsi qu'Eurostag pour des syst`emes de grande dimension. Mots-cl´es: HVDC, stabilit´e transitoire

Paris-Sud XI, Université de

302

Inventaire des documents F.1 Documents d'archives  

E-Print Network [OSTI]

´epartements (1834­1839). F7 3842 - rapports g´en´eraux de surveillance de la police (an IV - 1827). F18 I - 146 - enregistrement des journaux non caution- n´es (no 4 et no 285). F18 1 `a 119 - d´eclarations de divers imprimeurs, entre 1817 et 1834, sur le tirage des journaux. F18 355­383 - d´eclarations de divers ´editeurs de jour

Kleinert, Hagen Michael

303

Les incidents lis la protection juridique des investissements trangers en Chine : effectivit des voies de recours.  

E-Print Network [OSTI]

??Ce travail de recherche a pour objectif d'apporter un clairage et une comprhension sur l'volution du droit des affaires en Chine et plus particulirement sur (more)

Davant, Jrme

2010-01-01T23:59:59.000Z

304

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

305

Comptes Rendus des JNC 17 -Poitiers 2011 Simulation par lments finis des procds par infusion de rsine  

E-Print Network [OSTI]

Comptes Rendus des JNC 17 - Poitiers 2011 Simulation par éléments finis des procédés par infusion de résine Finite Simulation of the liquid infusion processes G. Pacquaut, J. Bruchon, N. Moulin, S permettant de simuler par éléments finis les procé- dés par infusion de résine au travers de renforts fibreux

Paris-Sud XI, Université de

306

Hommes et milieux : volution, interactions Participation des elus C aux comits de visite des units par l'AERES  

E-Print Network [OSTI]

de visite des unités par l'AERES La section 31 du comité national, lors de la session d'automne 2012, demande par cette motion à la direction de l'AERES d'intégrer systématiquement dans les comités de visite que leur opinion puisse s'exprimer et être prise en compte au cours de l'évaluation des unités par l'AERES

van Tiggelen, Bart

307

HYPOTHSES SUR L'ORIGINE DES BRUITS DU COEUR ET DES ACCIDENTS DE DCOMPRESSION EN PLONGE : LA CAVITATION.  

E-Print Network [OSTI]

CAVITATION. HYPOTH?SE SUR L'ORIGINE DE LA FERMETURE DES VALVES CARDIAQUES : LE PH?NOM?NE DE VENTOUSE. Dr. R'un phénomène de cavitation à l'origine des bruits de Korotkoff. Encouragés par l'aphorisme de MacDonald comme quoi le phénomène de cavitation est plus fréquent qu'on peut le penser dans le système cardio

308

ULTRA-DEEP HUBBLE SPACE TELESCOPE IMAGING OF THE SMALL MAGELLANIC CLOUD: THE INITIAL MASS FUNCTION OF STARS WITH M {approx}< 1 M {sub Sun}  

SciTech Connect (OSTI)

We present a new measurement of the stellar initial mass function (IMF) based on ultra-deep, high-resolution photometry of >5000 stars in the outskirts of the Small Magellanic Cloud (SMC) galaxy. The Hubble Space Telescope (HST) Advanced Camera for Surveys observations reveal this rich, cospatial population behind the foreground globular cluster 47 Tuc, which we targeted for 121 HST orbits. The stellar main sequence of the SMC is measured in the F606W, F814W color-magnitude diagram down to {approx}30th magnitude, and is cleanly separated from the foreground star cluster population using proper motions. We simulate the SMC population by extracting stellar masses (single and unresolved binaries) from specific IMFs and converting those masses to luminosities in our bandpasses. The corresponding photometry for these simulated stars is drawn directly from a rich cloud of 4 million artificial stars, thereby accounting for the real photometric scatter and completeness of the data. Over a continuous and well-populated mass range of M = 0.37-0.93 M {sub Sun} (e.g., down to a {approx}75% completeness limit at F606W = 28.7), we demonstrate that the IMF is well represented by a single power-law form with slope {alpha} = -1.90 ({sup +0.15} {sub -0.10}) (3{sigma} error) (e.g., dN/dM{proportional_to} M {sup {alpha}}). This is shallower than the Salpeter slope of {alpha} = -2.35, which agrees with the observed stellar luminosity function at higher masses. Our results indicate that the IMF does not turn over to a more shallow power-law form within this mass range. We discuss implications of this result for the theory of star formation, the inferred masses of galaxies, and the (lack of a) variation of the IMF with metallicity.

Kalirai, Jason S.; Anderson, Jay; Dotter, Aaron; Reid, I. Neill [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States)] [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Richer, Harvey B. [Department of Physics and Astronomy, University of British Columbia, Vancouver, BC (Canada)] [Department of Physics and Astronomy, University of British Columbia, Vancouver, BC (Canada); Fahlman, Gregory G. [National Research Council, Herzberg Institute of Astrophysics, Victoria, BC (Canada)] [National Research Council, Herzberg Institute of Astrophysics, Victoria, BC (Canada); Hansen, Brad M. S.; Rich, R. Michael [Division of Astronomy and Astrophysics, University of California at Los Angeles, Los Angeles, CA 90095 (United States)] [Division of Astronomy and Astrophysics, University of California at Los Angeles, Los Angeles, CA 90095 (United States); Hurley, Jarrod [Center for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn VIC 3122 (Australia)] [Center for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn VIC 3122 (Australia); Shara, Michael M., E-mail: jkalirai@stsci.edu, E-mail: jayander@stsci.edu, E-mail: dotter@stsci.edu, E-mail: richer@astro.ubc.ca, E-mail: greg.fahlman@nrc-cnrc.gc.ca, E-mail: hansen@astro.ucla.edu, E-mail: rmr@astro.ucla.edu, E-mail: jhurley@swin.edu.au, E-mail: mshara@amnh.org [Department of Astrophysics, American Museum of Natural History, Central Park West and 79th Street, New York, NY 10024 (United States)

2013-02-15T23:59:59.000Z

309

E-Print Network 3.0 - analyse quantitative des Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

de Lyon 1A -Approfondissement Summary: Dellandra - 2008-2009 TD 1 - Introduction Matlab et codage des donnes en vue de leur analyse L... raliser un codage des donnes,...

310

E-Print Network 3.0 - aspects des complications Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

des complications Search Powered by Explorit Topic List Advanced Search Sample search results for: aspects des complications Page: << < 1 2 3 4 5 > >> 1 L.-E. JEWELL. 2014 The...

311

E-Print Network 3.0 - au temps des Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

temps des Search Powered by Explorit Topic List Advanced Search Sample search results for: au temps des Page: << < 1 2 3 4 5 > >> 1 Bases de Donnes -TD6 Licence Informatique...

312

E-Print Network 3.0 - appauvri chez des Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

appauvri chez des Search Powered by Explorit Topic List Advanced Search Sample search results for: appauvri chez des Page: << < 1 2 3 4 5 > >> 1 Perception, plasticit et vie...

313

E-Print Network 3.0 - appliques des lyon Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

des lyon Search Powered by Explorit Topic List Advanced Search Sample search results for: appliques des lyon Page: << < 1 2 3 4 5 > >> 1 Center for Turbulence Research Proceedings...

314

E-Print Network 3.0 - au secteur des Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

secteur des Search Powered by Explorit Topic List Advanced Search Sample search results for: au secteur des Page: << < 1 2 3 4 5 > >> 1 Mathmatiques l'industrie et le Summary:...

315

Accelerated Publications Three-Dimensional Structure of DesVI from Streptomyces Venezuelae: A Sugar  

E-Print Network [OSTI]

Accelerated Publications Three-Dimensional Structure of DesVI from Streptomyces Venezuelae: A Sugar for the biosynthesis of dTDP-desosamine in Streptomyces Venezuelae, with the last step catalyzed by DesVI, an N

Holden, Hazel

316

Molecular architecture of DesV from Streptomyces venezuelae: A PLP-dependent transaminase involved in  

E-Print Network [OSTI]

Molecular architecture of DesV from Streptomyces venezuelae: A PLP-dependent transaminase involved are required for its biosynthesis in Streptomyces venezuelae. The focus of this article is DesV, which

Holden, Hazel

317

MICRO-CAPTEURS POUR LA GESTION DURABLE DE LA QUALITE DES EAUX Namour Philippe1 *  

E-Print Network [OSTI]

1 MICRO-CAPTEURS POUR LA GESTION DURABLE DE LA QUALITE DES EAUX Namour Philippe1 * , Khadro Basma 2 besoins tant réglementaires (DCE, LEMA) que cognitifs, (exploration du fonctionnement des hydro

Boyer, Edmond

318

Les Bons Ingredients pour un Haut Niveau de Performance des Installations Climatiques  

E-Print Network [OSTI]

DE POST-RECEPTION DES SERVICES ADAPTES AUX BESOINS, CONTRACTUELS DES SERVICES ADAPTES AUX BESOINS, CONTRACTUELS 1 an RECEPTION RECEPTION ICEBO ? C ommiss 7 Le dossier technique Le dossier technique usage, maintenance, exploitation, usage, maintenance..., exploitation, selon le contratselon le contrat DOSSIER DOEFichesNotices d?usageMAP Ajustements des r?glages, fonctions DIUO de la GTB, nettoyages sanitaires? P.V.COPREC RECEPTION DOSSIER DOEFichesNotices d?usageMAPAjustements des r?glages, DIUO Fonctions de...

Rougnon, J.

2004-01-01T23:59:59.000Z

319

E-Print Network 3.0 - analysis untersuchung des Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

mithilfe der o.g. Zuverlssigkeitsanalyse... -orientierten Modellierungssprache Modelica vorgesehen. Als Beispiel ist in der Abbildung die Nicksteuerung des ... Source:...

320

Comptes rendus l'Acadmie des Sciences Special issue on nanosciences/nanotechnologies  

E-Print Network [OSTI]

Comptes rendus à l'Académie des Sciences Special issue on nanosciences/nanotechnologies March 1st manuscript, published in "Comptes rendus à l'Académie des Sciences (2011) Special issue on nanosciences/ nanotechnologies" #12;Comptes rendus à l'Académie des Sciences Special issue on nanosciences/nanotechnologies March

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.


321

L'ACCUEIL DES NAVIRES DE PLAISANCE EN BRETAGNE DANS LA PERSPECTIVE D'UNE GESTION  

E-Print Network [OSTI]

L'ACCUEIL DES NAVIRES DE PLAISANCE EN BRETAGNE DANS LA PERSPECTIVE D'UNE GESTION INTGRE DES ZONES prconisations de l'Union Europenne en faveur d'une gestion intgre des zones ctires (GIZC), dclinaison du, au cas par cas, d'estimer au mieux les retombes et la pertinence de chaque projet. Ceux-ci doivent

Boyer, Edmond

322

Licence Professionnelle, CISI 2009-2010 Cours 9 : Gestion des exceptions  

E-Print Network [OSTI]

cas o une exception a t leve http://www710.univ-lyon1.fr/~ecoquery #12;6 Gestion des exceptions1 Java Licence Professionnelle, CISI 2009-2010 Cours 9 : Gestion des exceptions Entree/Sortie #12;2 Gestion des exceptions Introduction : qu'est-ce qu'une exception ? - De nombreux langages de

Belad, Abdel

323

Gestion stratgique des comptences en PME : les enseignements d'une recherche-action  

E-Print Network [OSTI]

1 Gestion stratgique des comptences en PME : les enseignements d'une recherche-action Jean, France Introduction Si pendant longtemps, le besoin des entreprises n'allait pas au-del d'une gestion proccupation croissante autour de la gestion des comptences (Dfelix, 2003 ; Le Boterf, 2000), de sorte que

Boyer, Edmond

324

LeTemps.ch I Des robots pour mieux comprendre l,volution 08011217:49  

E-Print Network [OSTI]

LeTemps.ch I Des robots pour mieux comprendre l,volution LE TEMPs 08011217:49 biologie Vendredi6 janvier 2012 Des robots pour mieux comprendre l'6volution Par L'aldatoire entrerait en jeu Le d6'y parvenir en employant comme cobayes... des robots. Etude qu,ils publient cette semaine dans une

Alvarez, Nadir

325

Certification des structures d'hospitalisation domicile VS certification ISO 9000  

E-Print Network [OSTI]

Certification des structures d'hospitalisation domicile VS certification ISO 9000 RYM BEN comparative entre la certification ISO 9000 (International Organisation for Standardization) et la certification des HAD. Il s'agit de comparer la certification ISO 9000 celle des tablissements de sant et

Paris-Sud XI, Universit de

326

Des Plaines, Illinois: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump to:52c8ff988c1Dering Harbor, New York: Energy Resources JumpDes PlainesDes

327

Aussi avons-nous ensuite 6tudi6 des cristaux fabriqu6s au laboratoire (creusets de platine) [4],  

E-Print Network [OSTI]

- lement les deux pics P1 et P2. Apr6s avoir dope des cristaux de fluorure de lithium avec des ions Mn, irradiation et corrosion par des gaz). Puis on traite des phnomnes qui se produisent pendant et aprs

Paris-Sud XI, Universit de

328

TUDE DES CIBLES MINCES CHARGES DE TRITIUM UTILISES DANS LES ACCLRATEURS PRODUISANT DES NEUTRONS RAPIDES PAR LA RACTION D-T  

E-Print Network [OSTI]

61 ?TUDE DES CIBLES MINCES CHARG?ES DE TRITIUM UTILIS?ES DANS LES ACC?L?RATEURS PRODUISANT DES [titane-tritium]préparées par le Département des Radioéléments de Saclay. Dix sept cibles ont été ainsi rendement. Abstract. 2014 This study permits the determination of the efficiency of titan-tritium targets

Paris-Sud XI, Université de

329

THE CLUSTERED NATURE OF STAR FORMATION. PRE-MAIN-SEQUENCE CLUSTERS IN THE STAR-FORMING REGION NGC 602/N90 IN THE SMALL MAGELLANIC CLOUD  

SciTech Connect (OSTI)

Located at the tip of the wing of the Small Magellanic Cloud (SMC), the star-forming region NGC 602/N90 is characterized by the H II nebular ring N90 and the young cluster of pre-main-sequence (PMS) and early-type main-sequence stars NGC 602, located in the central area of the ring. We present a thorough cluster analysis of the stellar sample identified with Hubble Space Telescope/Advanced Camera for Surveys in the region. We show that apart from the central cluster low-mass PMS stars are congregated in 13 additional small, compact sub-clusters at the periphery of NGC 602, identified in terms of their higher stellar density with respect to the average background density derived from star counts. We find that the spatial distribution of the PMS stars is bimodal, with an unusually large fraction ({approx}60%) of the total population being clustered, while the remaining is diffusely distributed in the intercluster area, covering the whole central part of the region. From the corresponding color-magnitude diagrams we disentangle an age difference of {approx}2.5 Myr between NGC 602 and the compact sub-clusters, which appear younger, on the basis of comparison of the brighter PMS stars with evolutionary models, which we accurately calculated for the metal abundance of the SMC. The diffuse PMS population appears to host stars as old as those in NGC 602. Almost all detected PMS sub-clusters appear to be centrally concentrated. When the complete PMS stellar sample, including both clustered and diffused stars, is considered in our cluster analysis, it appears as a single centrally concentrated stellar agglomeration, covering the whole central area of the region. Considering also the hot massive stars of the system, we find evidence that this agglomeration is hierarchically structured. Based on our findings, we propose a scenario according to which the region NGC 602/N90 experiences an active clustered star formation for the last {approx}5 Myr. The central cluster NGC 602 was formed first and rapidly started dissolving into its immediate ambient environment, possibly ejecting also massive stars found away from its center. Star formation continued in sub-clusters of a larger stellar agglomeration, introducing an age spread of the order of 2.5 Myr among the PMS populations.

Gouliermis, Dimitrios A.; Gennaro, Mario [Max Planck Institute for Astronomy, Koenigstuhl 17, 69117 Heidelberg (Germany); Schmeja, Stefan [Zentrum fuer Astronomie der Universitaet Heidelberg, Institut fuer Theoretische Astrophysik, Albert-Ueberle-Str. 2, 69120 Heidelberg (Germany); Dolphin, Andrew E. [Raytheon Company, P.O. Box 11337, Tucson, AZ 85734 (United States); Tognelli, Emanuele; Prada Moroni, Pier Giorgio [Dipartimento di Fisica 'Enrico Fermi', Universita di Pisa, largo Pontecorvo 3, Pisa I-56127 (Italy)

2012-03-20T23:59:59.000Z

330

Salon International des Energies (SIDE), International Energy Exhibition & Conference Oil, Gas, Mining, RnE, October 2 -5, 2012 Palais des Congrs -Marrakech, Maroc.  

E-Print Network [OSTI]

, Mining, RnE, October 2 - 5, 2012 Palais des Congrès - Marrakech, Maroc. Potential source rocks of Late

Olsen, Paul E.

331

PERTES CARACTRISTIQUES DES LECTRONS DANS TlCl, TlBr, Tl I ET CALCUL DES FONCTIONS OPTIQUES ENTRE 3 ET 25 eV  

E-Print Network [OSTI]

diffèrent des halogé- nures alcalins notamment par leur grande constante diélectrique optique et par un

Paris-Sud XI, Université de

332

L'expertise en conduite automobile peut-elle moduler le phnomne d'extension des limites ?  

E-Print Network [OSTI]

L'expertise en conduite automobile peut-elle moduler le phénomène d'extension des limites'observateur vis-à-vis de la scène perçue, est sensible aux connaissances expertes. Des conducteurs automobiles automobile peut-elle moduler le phénomène d'extension des limites ? L'un des aspects les plus intrigants des

Jeanjean, Louis

333

Direction des immeubles Prparation du courrier prioritaire pour le Canada  

E-Print Network [OSTI]

Direction des immeubles Préparation du courrier prioritaire pour le Canada Comment faire? 1 requis ainsi que le code postal Pour expédier du courrier par Postes Canada · Vous pouvez utiliser une adresse civique et/ou une case postale. · Pour recevoir du courrier par Postes Canada, vous devez utiliser

Charette, André

334

VOLUTION DES FERRITES DOUX POUR TLCOMMUNICATIONS ET TLVISION  

E-Print Network [OSTI]

837 ?VOLUTION DES FERRITES DOUX POUR T?L?COMMUNICATIONS ET T?L?VISION R. SIBILLE Directeur Technique de L. C. C. Division Ferrites (COFELEC) Thomson C. S. F., 74 Route de Savigny, 21204 Beaune deuxième guerre mondiale), les ferrites doux sont encore en pleine évolution et nombreux sont ceux qui leur

Boyer, Edmond

335

LES DETERMINANTS DES DISCOURS MANAGERIAUX : APPLICATION AUX CAS  

E-Print Network [OSTI]

-techniques : norme ISO 9001, norme ISO 14000 etc ...Ces normes sont issues de travaux de réflexion réalisés certaines, entre autres la norme ISO 9001, des responsables qualité ayant une autre formation d'origine. Ceci s'explique par le fait que la norme ISO 9001 organise la circulation documentaire au sein de l

Paris-Sud XI, Université de

336

Facult des Lettres INSTITUT D' ETlil{OLOGIE  

E-Print Network [OSTI]

'OIBE D' EII HHO-BOTANIQUE ET DI ETHNO-ZOOLOGIE PARIS LE COMPORTEMENT ALI~OENTAlRE DES A1~IV~UX SAUVAGES Eusum IJational d 'Histoire--Naturelle LABOiLAC[tOIJ_-U:~; D' ET'HHO-B01\\AFfIQE ET DI ETHNO

Paris-Sud XI, Universit de

337

LES DETERMINANTS DES COMPETENCES DE LA FONCTION GESTION-FINANCE  

E-Print Network [OSTI]

LES DETERMINANTS DES COMPETENCES DE LA FONCTION GESTION-FINANCE Pierre-Laurent, Bescos Professeur'enjeu est de donner alors aux étudiants et professionnels de la fonction gestion-finance une formation de, les aptitudes et les grades au sein de la fonction gestion-finance. Mots clés : compétences, enquête

Paris-Sud XI, Université de

338

Bestimmung des ep{Wirkungsquerschnittes von Beauty-Quarks  

E-Print Network [OSTI]

Bestimmung des ep{Wirkungsquerschnittes von Beauty-Quarks durch ihren semileptonischen Zerfall in Myonen mit dem H1-Detektor bei HERA Determination of the ep Cross Section for Beauty Quarks via werden die sichtbaren ep-Wirkungsquerschnitte fur schwere Quarks in dem kinematischen Bereich Q2

339

Bernard CALMETTES Contribution l'tude des curriculums.  

E-Print Network [OSTI]

1 Bernard CALMETTES Contribution l'tude des curriculums. Le cas de l'enseignement de l le dveloppement d'une "culture" : Au niveau d'excution, mme fort lev dans la hirarchie-00278552,version1-13May2008 #12;4 dans l'enseignement une culture scientifique gnrale, apparemment

Boyer, Edmond

340

prsente L'cole Nationale Suprieure des Mines de Paris  

E-Print Network [OSTI]

la thèse: ESTIMATION ET CONTR?LE D'UN MOTEUR DIESEL HCCI. ESTIMATION DES SYST?MES P?RIODIQUES Examinateur #12;#12;Jonathan CHAUVIN ESTIMATION AND CONTROL OF A DIESEL HCCI ENGINE. ESTIMATION FOR TIME.chauvin@ifp.fr Url : www.cas.ensmp.fr/chauvin Key words and phrases. -- Engine control, HCCI, air path control

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.


341

Consommer des produits alimentaires locaux : comment et pourquoi ?1  

E-Print Network [OSTI]

redécouverte des saveurs, la volonté de consommer responsable et la recherche de lien social. L'analyse s, produit local, circuits courts, marketing agroalimentaire, lien producteur-consommateur. Local food: how for sustainable consumption and the search for social relationships. The analysis is based on a qualitative study

Paris-Sud XI, Université de

342

TUDE DES PHOTODSINTGRATIONS. , II. QUELQUES RSULTATS EXPRIMENTAUX SUR LES PHOTODSINTGRATIONS  

E-Print Network [OSTI]

était inférieur à ceux observés, en général, par Hirzel et Wâffler. Toms, Halpern et Stephens [5], [6 les iso- topes du magnésium, dont certaines conduisent à des nuclides stables. Byerly et Stephens [7

Paris-Sud XI, Université de

343

ATLAS-Experiment Abbildung 50: Aufbau des ATLAS Detektors.  

E-Print Network [OSTI]

ATLAS-Experiment Abbildung 50: Aufbau des ATLAS Detektors. 98 #12;ATLAS-Experiment ATLAS, LHC, zu unterst¨utzen. Die DESY Gruppe wurde formal im Juli 2006 in die ATLAS Kollaboration aufgenom Beteiligung an ATLAS erfolgt in enger Koope- ration mit einer Gruppe der Humboldt Universit¨at zu Berlin und

344

Arbeitspapiere des SFB 340 Bericht Nr. 132, September 1999  

E-Print Network [OSTI]

Arbeitspapiere des SFB 340 Bericht Nr. 132, September 1999 AN RSRL FORMALIZATION OF SERBO-CROATIAN . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 177 2. Clitic Placement in Serbo-Croatian . . . . . . . . . . . . . . . . . . . . . . . . . . . . 178. Such is the case in Serbo-Croatian where prosodic constituency plays a role on a par with syntactic constituency

Toronto, University of

345

Stphane Couturier EVALUATION DES ERREURS DE CARTES DE  

E-Print Network [OSTI]

guide de Chan Laguna près de Calakmul, Campeche, Pedro Zamora et ses étudiants biologistes de l'Université Autonome de Campeche. Merci à l'ensemble des membres de l'équipe DART, qui m'ont infailliblement soutenu en

Paris-Sud XI, Université de

346

Diplomanden-und Doktorandenseminar des Instituts fr Informatik  

E-Print Network [OSTI]

Diplomanden- und Doktorandenseminar des Instituts für Informatik Six Sigma im Im üblichen Sinne wird Six Sigma insbesondere in Fertigungsindustrien wie zum Beispiel in der ist Six Sigma nicht nur eine Managementstrategie, die sich ausschlie?lich auf die Fertigungsindustrie

Zachmann, Gabriel

347

LE JOURNAL DE PHYSIQUE L'COULEMENT DES MTAUX (1)  

E-Print Network [OSTI]

exemple, les pales d'une turbine vapeur tournant grande vitesse; si ces pales s'allongent de quelques millimes elles risqueront de toucher le corps de l'appareil, avec un danger vident. Dans les turbines gaz employes danse les avions les plus rcents, le danger est de beaucoup augment cause des

Paris-Sud XI, Universit de

348

Simulations of the OzDES AGN Reverberation Mapping Project  

E-Print Network [OSTI]

As part of the OzDES spectroscopic survey we are carrying out a large scale reverberation mapping study of $\\sim$500 quasars over five years in the 30 deg$^2$ area of the Dark Energy Survey (DES) supernova fields. These quasars have redshifts ranging up to 4 and have apparent AB magnitudes between $16.8DES reverberation mapping campaign and its possible extensions. We expect to recover lags for $\\sim$35-45\\% of the quasars. AGN with shorter lags and greater variability are more likely to yield a lag, and objects with lags $\\lesssim$6 month or $\\sim$1 year are expected be recovered the most accurately. The baseline OzDES reverberation mapping campaign is predicted to produce an ...

King, Anthea L; Davis, Tamara M; Denney, K D; Kochanek, C S; Peterson, Bradley M; Skielboe, Andreas; Vestergaard, Marianne; Huff, Eric; Watson, Darach; Banerji, Manda; McMahon, Richard; Sharp, Rob; Lidman, C

2015-01-01T23:59:59.000Z

349

Dossier d'Habilitation Diriger des Recherches Jacques Dverchre  

E-Print Network [OSTI]

: Géométrie et modes d'évolution des rifts dans le temps et l'espace B. DEMARCHE: de la "sismo-géologie" à l la « sismo-géologie » dans un ensemble d'observations géophysiques et géologiques 3. Les propriétés

Déverchère, Jacques

350

Centre Europen de Recherche et d'Enseignement des  

E-Print Network [OSTI]

informations diffusées par l'Isotope Geology Laboratory de Boise (Idaho, USA) et par le Lamont-Doherty Earth informations sur des éléments couramment analysés avec la technique TIMS : strontium, néodyme, plomb, uranium

Paris-Sud XI, Université de

351

La ville comme lieu d'mergence de nouvelles formes d'urbanit. Cas des quartiers rsidentiels de la ville de Constantine  

E-Print Network [OSTI]

La ville comme lieu d'émergence de nouvelles formes d'urbanité. Cas des quartiers résidentiels de supprime le monopole des communes sur le patrimoine foncier et autorise la création des lotissements par l;Mais, si l'Etat ne dispose plus des droits absolus sur la gestion des sols, il restera toujours l

Boyer, Edmond

352

Comptes Rendus des JNC 17 -Poitiers 2011 OSIRHYS IV Qualification des codes pour la prdiction du comportement  

E-Print Network [OSTI]

comportements. Abstract The hydrogen storage stays a key issue for the high scale deployment of fuel cell locaux. Les résultats montrent que l'analyse en statique linéaire utilisant des modèles 3D et nowadays. But it is necessary to reach a significant cost reduction of these storage systems

Paris-Sud XI, Université de

353

Travail, stress et sant : des modles thoriques un mta-modle Recension critique des modles thoriques reliant environnement  

E-Print Network [OSTI]

être stressée au travail (Milczarek, Schneider, & González, 2009).Toujours en 2005, 56 % des travailleurs européens estimaient que leur santé était affectée par leur activité professionnelle (Milczarek

Paris-Sud XI, Université de

354

Espaces Socits et Territoires Participation des lus C aux comits de visite des laboratoires par l'AERES  

E-Print Network [OSTI]

des laboratoires par l'AERES La section 39 du comité national, lors de sa première réunion du nouveau dans chaque comité de visite AERES un membre élu C de la section compétente du comité national. Les

van Tiggelen, Bart

355

conomie et Gestion Participation des lus C aux comits de visite des laboratoires par l'AERES  

E-Print Network [OSTI]

laboratoires par l'AERES La section 37 du comité national demande par cette motion à la direction de l'AERES d-Benoît Zimmermann Destinataires : Pierre GLAUDES, Directeur de la section des unités de recherche AERES Alain

van Tiggelen, Bart

356

LISTE DES MEMBRES DU CONSEIL DES ETUDES ET DE LA VIE UNIVERSITAIRE Collge ou catgorie Secteur Statut Nom Prnom Fonction Affectation  

E-Print Network [OSTI]

langues, sciences humaines et sociales Titulaire FRANCALANZA Eric Professeurs des Universités UFR Lettres et Sciences Humaines Art, littérature et langues, sciences humaines et sociales Titulaire AGOSTO Marie-Christine Professeurs des Universités UFR Lettres et Sciences Humaines Droit, économie, gestion

Brest, Université de

357

Des six projets de recherche en concurrence, Graphene est l'un des deux slectionns par le programme FET (Future and emerging tech-  

E-Print Network [OSTI]

Des six projets de recherche en concurrence, Graphene est l'un des deux slectionns par le reconnu en nano-lectronique et en matriaux et reprsentant suisse du projet Graphene (Graphene agship). Aujourd'hui l'Europe lance un projet de recherche d'une envergure sans prcdent ( agship). Graphene

Halazonetis, Thanos

358

Programme des 3mes Rencontres de l'ESS en Vaucluse le 18 octobre 2012 08h30 Accueil et visite des stands AT 04  

E-Print Network [OSTI]

Programme des 3èmes Rencontres de l'ESS en Vaucluse le 18 octobre 2012 du film sur l'ESS en Vaucluse dans l'amphithéâtre 09h00 Amphithéâtre AT 04 Lancement des 3èmes rencontres de l'ESS en présence de

Naud Frédéric

359

Rappropriation des donnes et droit la rediffusion La rutilisation des donnes en dehors de la plateforme Facebook a t beaucoup discute selon l'angle de la  

E-Print Network [OSTI]

plateforme Facebook a t beaucoup discute selon l'angle de la vie prive et de la ncessit d donnes des utilisateurs des entreprises, la licence octroye Facebook tant transfrable. A force d'abus rpts sur le terrain de la vie prive, le dbat propos de Facebook ignore largement la question de l

Paris-Sud XI, Universit de

360

THE MASS-LOSS RETURN FROM EVOLVED STARS TO THE LARGE MAGELLANIC CLOUD. II. DUST PROPERTIES FOR OXYGEN-RICH ASYMPTOTIC GIANT BRANCH STARS  

SciTech Connect (OSTI)

We model multi-wavelength broadband UBVIJHK{sub s} and Spitzer IRAC and MIPS photometry and Infrared Spectrograph spectra from the SAGE and SAGE-Spectroscopy observing programs of two oxygen-rich asymptotic giant branch (O-rich AGB) stars in the Large Magellanic Cloud (LMC) using radiative transfer (RT) models of dust shells around stars. We chose a star from each of the bright and faint O-rich AGB populations found by earlier studies of the SAGE sample in order to derive a baseline set of dust properties to be used in the construction of an extensive grid of RT models of the O-rich AGB stars found in the SAGE surveys. From the bright O-rich AGB population, we chose HV 5715, and from the faint O-rich AGB population we chose SSTISAGE1C J052206.92-715017.6 (SSTSAGE052206). We found the complex indices of refraction of oxygen-deficient silicates from Ossenkopf et al. and a power law with exponential decay grain size distribution like what Kim et al. used but with {gamma} of -3.5, a {sub min} of 0.01 {mu}m, and a {sub 0} of 0.1 {mu}m to be reasonable dust properties for these models. There is a slight indication that the dust around the faint O-rich AGB may be more silica-rich than that around the bright O-rich AGB. Simple models of gas emission suggest a relatively extended gas envelope for the faint O-rich AGB star modeled, consistent with the relatively large dust shell inner radius for the same model. Our models of the data require the luminosity of SSTSAGE052206 and HV 5715 to be {approx}5100 L {sub sun} and {approx}36,000 L {sub sun}, respectively. This, combined with the stellar effective temperatures of 3700 K and 3500 K, respectively, that we find best fit the optical and near-infrared data, suggests stellar masses of {approx}3 M {sub sun} and {approx}7 M {sub sun}. This, in turn, suggests that HV 5715 is undergoing hot-bottom burning and that SSTSAGE052206 is not. Our models of SSTSAGE052206 and HV 5715 require dust shells of inner radius {approx}17 and {approx}52 times the stellar radius, respectively, with dust temperatures there of 900 K and 430 K, respectively, and with optical depths at 10 {mu}m through the shells of 0.095 and 0.012, respectively. The models compute the dust mass-loss rates for the two stars to be 2.0 x 10{sup -9} M{sub sun} yr{sup -1} and 2.3 x 10{sup -9} M{sub sun} yr{sup -1}, respectively. When a dust-to-gas mass ratio of 0.002 is assumed for SSTSAGE052206 and HV 5715, the dust mass-loss rates imply total mass-loss rates of 1.0 x 10{sup -6} M{sub sun} yr{sup -1} and 1.2 x 10{sup -6} M{sub sun} yr{sup -1}, respectively. These properties of the dust shells and stars, as inferred from our models of the two stars, are found to be consistent with properties observed or assumed by detailed studies of other O-rich AGB stars in the LMC and elsewhere.

Sargent, Benjamin A.; Meixner, M.; Gordon, Karl D. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Srinivasan, S. [Institut d'Astrophysique de Paris, 98 bis, Boulevard Arago, Paris 75014 (France); Kemper, F.; Woods, Paul M. [Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13 9PL (United Kingdom); Tielens, A. G. G. M. [Leiden Observatory, P.O. Box 9513, NL-2300 RA Leiden (Netherlands); Speck, A. K. [Physics and Astronomy Department, University of Missouri, Columbia, MO 65211 (United States); Matsuura, M. [Institute of Origins, Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT (United Kingdom); Bernard, J.-Ph. [Centre d'Etude Spatiale des Rayonnements, 9 Av. du Colonel Roche, BP 44346, 31028 Toulouse Cedex 4 (France); Hony, S. [Laboratoire AIM, CEA/DSM-CNRS-Universite Paris Diderot DAPNIA/Service d'Astrophysique Bat. 709, CEA-Saclay F-91191 Gif-sur-Yvette Cedex (France); Indebetouw, R. [Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904 (United States); Marengo, M. [Department of Physics and Astronomy, Iowa State University, Ames, IA 50011 (United States); Sloan, G. C., E-mail: sargent@stsci.ed [Department of Astronomy, Cornell University, Ithaca, NY 14853 (United States)

2010-06-10T23:59:59.000Z

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
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361

Identits culturelles dans l'ge du Fer europen Notre connaissance des populations de l'ge du Fer europen permet aujourd'hui de dpasser  

E-Print Network [OSTI]

, spatiales, et typologiques, il est possible aujourd'hui d'identifier des contextes et des situations tenterons de faire des comparaisons interculturelles. Habitat : Groupé/isolé, ouvert/enclos/fortifié, plaine

362

Magellan Queues end November 30  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: VegetationEquipment Surfaces and InterfacesAdministration -Lowell L.FallU . S . DMagellan Report on Cloud

363

CONTAGION DES CRISES DE 1997 ET 2008 EN ASEAN+3: UN MODELE VAR STRUCTUREL  

E-Print Network [OSTI]

i CONTAGION DES CRISES DE 1997 ET 2008 EN ASEAN+3: UN MODELE VAR STRUCTUREL Marine Coupaud LAREFI possibilités d'analyses afin d'étudier l'impact de chocs monétaires et réels sur les pays de l'Asean. Cette étude vise à analyser les réactions des pays membres de l'Asean+3 face à des perturbations de grande

Paris-Sud XI, Université de

364

Rflexions autour des migrations forces en Afrique sub-saharienne1  

E-Print Network [OSTI]

réfugiés climatiques. Enfin, il insiste, à travers des études de cas, sur les territoires générés par ces, 2009). Ainsi, ce rapport remet en cause l'idée reçue concernant l'ampleur des migrations sud-nord alors recherche académique et des pouvoirs politiques au Nord. Ils accaparent l'attention et font l'objet d

Paris-Sud XI, Université de

365

Intgration d'outils scientifiques et techniques dans un processus de conception : modlisation des facteurs  

E-Print Network [OSTI]

objectif la caractérisation des activités motrices des acteurs concernés : les personnes en situation de handicap. Notre ambition est de caractériser et de modéliser les spécificités motrices de ces futurs motrices. Dans cet article, nous proposons une adaptation du processus de conception UCD en y intégrant des

Paris-Sud XI, Université de

366

Proprits des fibres musculaires squelettiques. 1. Influence de l'innervation motrice  

E-Print Network [OSTI]

Propriétés des fibres musculaires squelettiques. 1. Influence de l'innervation motrice F. BACOU, P'activité motrice. Elle contient, outre l'équipement enzymatique nécessaire à la couverture énergétique de la décrirons l'importance de l'innervation motrice dans la genèse et le maintien des propriétés des différents

Paris-Sud XI, Université de

367

Extraction et analyse automatiques des sinus de Valsalva partir de squences C. Blanchard1  

E-Print Network [OSTI]

Hospitalier Universitaire de Dijon, France Laboratoire Le2i, route des plaines de l'Yonne BP16, 89010 Auxerre- ment prometteuse pour l'étude des sinus de Valsalva (SV), il n'existe pas aujourd'hui de consensus pour les examens. De plus, sur l'ensemble des séquences, il y a d'excellentes corrélation et concor- dance

Boyer, Edmond

368

Approche compare du dveloppement des villes-ports l'chelle mondiale : problmes conceptuels et mthodologiques  

E-Print Network [OSTI]

1 Approche comparée du développement des villes-ports à l'échelle mondiale : problèmes conceptuels comparaison internationale des villes-ports se justifie par la similitude croissante des phénomènes spatiaux mécanismes que connaissent les villes-ports dans leur individualité et au sein de leur espace national, ce

Paris-Sud XI, Université de

369

Analyse morphomtrique des abeilles Quinze chantillons d'abeilles provenant  

E-Print Network [OSTI]

Analyse morphométrique des abeilles d'Uruguay Quinze échantillons d'abeilles provenant d'Uruguay venant d'Uruguay, d'Europe et d'Afri- que, montre une similitude étroite entre l'abeille ibérique (Apis mellifera iberica) et les échantillons d'Uruguay. L'autre, basé sur la méthode de Daly et Balling (1978) et

Paris-Sud XI, Université de

370

La rfraction des Matriaux : de Descartes Harry Potter  

E-Print Network [OSTI]

deuxième ordre Ions à paires libres R. D. Shannon et al. J. Phys. Chem Ref. Data 31, n° 4, (2002) 931 hal1 La réfraction des Matériaux : de Descartes à Harry Potter Gilles Le Flem ICMCB ( mars 2007)Gilles Descartes à Harry Potter (notes informelles et diapositives du séminaire de 16/03/07) En juin 2006 le groupe

Boyer, Edmond

371

cole Doctorale n 398 : Gestion des Ressources Naturelles AVANT PROPO  

E-Print Network [OSTI]

?cole Doctorale n° 398 : Gestion des Ressources Naturelles AVANT ­PROPO présentée et soutenue alternatives pour maximiser la récupération du métal. Cette étude a été appliquée au cas du gisement stratiforme de Cu et Ag de Mantos de la Luna situé dans le Nord du Chili. Elle comporte en particulier une

Paris-Sud XI, Université de

372

S'eparation des convexes J.Ch. Gilbert, Inria  

E-Print Network [OSTI]

S'eparation des convexes J.Ch. Gilbert, Inria Th'eor`eme de Hahn­Banach (forme analytique) ffl Soit. ffl Th'eor`eme de Hahn­Banach (forme analytique). Si \\Delta E est un espace vectoriel (non n toujours un f tel que l'on ait 'egalit'e. 1 #12; Th'eor`emes de Hahn­Banach (formes g'eom'etriques) ffl

373

Reprsentations crbrales des articulateurs de la parole Krystyna Grabski1  

E-Print Network [OSTI]

observé le déclenchement de mouvements spécifiques et ont ainsi établi une cartographie corticale motrice liée au contrôle de différentes parties du corps. Cette organisation corticale motrice, dite son organisation spatiale que de la taille des zones motrices associées à chaque partie du corps. Ce

Paris-Sud XI, Université de

374

DE QUELQUES FACTEURS DETERMINANT LE DEROULEMENT DES CARRIERES DE PRATIQUANTS  

E-Print Network [OSTI]

'Etude Sport et Actions Motrices CesamS EA 4260 ­ UFR STAPS Université de Caen Basse-Normandie Deux auteurs motrice spécialisée qui, dans l'immense majorité des cas, n'est pas en droit leur occupation principale en charge du sport, entendu au sens d'activités motrices codifiées sous forme compétitive et

Boyer, Edmond

375

Des quipements mutualiss Les systmes d'information  

E-Print Network [OSTI]

modernisation de la flotte. La rnovation et l'agrandissement du pavillon d'accueil du centre IRD d'le-de-France reprsentent l'essentiel de l'investissement en grands travaux. \\Un pavillon d'accueil au centre IRD le-de-France Pour renforcer les capacits de recherche des pays du Sud, l'IRD accueille au centre le-de-France une

376

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]

prati- que des Anuttarayogatantra, ainsi que dassurer, linstar du sens cach une conti- nuit ncessaire du point de vue psychologique, didactique et sotriologique, entre stra et tantra (V. P. Arnes, Un exemple dapplication un tantra, du... on the oral transmission, Oxford, Ox- ford Univ. Press, 1963, p.48), chez les bKa brgyud pa et les rNying ma pa, on dis- tingue entre gnas lugs quil traduit par being in itself et yin lugs quil traduit par being this or that, ces deux aspects tant la...

Arenes, Pierre

2002-01-01T23:59:59.000Z

377

INFORMALITS NORMALISES : FACTEURS D'INTEGRATION CONOMIQUE ET SOCIALE DES BRSILIENNES EN GUYANE  

E-Print Network [OSTI]

'Africains échappés du Surinam (1880), forment des villages le long du fleuve Maroni. Les descendants de ces

Boyer, Edmond

378

Centenaire de la Socit des Amis du Musum national d'histoire naturelle Enrichissement et valorisation  

E-Print Network [OSTI]

dessinatrice : « Ils sont d'une personne du même sexe que celle à qui nous devons ceux des insectes de Surinam

379

E-Print Network 3.0 - activities sachstandsbericht des Sample...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Weltklimarats eingesetzten Modellen errechnet wurde10 . Es gibt also keine Diskrepanz... solare Beeinflussung des Klimas. Eine aktivere Sonne knne ... Source: Stock, Manfred -...

380

UNIVERSITE SCIENTIFIQUE ET MEDICALE DE GRENOBLE U.E.R DES SCIENCES PHARMACEUTIQUES  

E-Print Network [OSTI]

personnel de l'AECL (Association des Etudiants pour la Culture et les Loisirs) et son Président Monsieur P

Note: This page contains sample records for the topic "magellan des moines" from the National Library of EnergyBeta (NLEBeta).
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they are not comprehensive nor are they the most current set.
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381

Correction-solution partielle des Feuilles 1 8 Exercice 1.1 : Solutions  

E-Print Network [OSTI]

STIA3 Correction-solution partielle des Feuilles 1 à 8 Exercice 1.1 : Solutions : Df = R+ Dg = Rn 5

Mas, André

382

E-Print Network 3.0 - alle hrtexte des Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Search Sample search results for: alle hrtexte des Page: << < 1 2 3 4 5 > >> 1 ADAPTING DATABASE IMPLEMENTATION TECHNIQUES TO MANAGE VERY LARGE KNOWLEDGE BASES Summary: history...

383

E-Print Network 3.0 - academies des sciences Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Collection: Mathematics 19 "Simion Stoilow" Institute of Mathematics of the Romanian Academy Le premier seminaire roumain-tunisien Summary: Belhaj Rhouma (Faculte des...

384

tude comparative des systmes verbaux du franais et du persan (mode, temps, aspect).  

E-Print Network [OSTI]

??Cette tude comparative des systmes verbaux du persan et du franais est constitue de trois chapitres. Nous consacrerons le dbut de cette thse au verbe (more)

Sadidi, Zahra

2012-01-01T23:59:59.000Z

385

E-Print Network 3.0 - analyse des risques Sample Search Results  

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les risques, ... Source: Ecole Polytechnique, Centre de mathmatiques Collection: Mathematics 2 POLLAK Catherine (2009), L impossible approche positive des risques sociaux ? ,...

386

Des plans-lumire nocturnes la chronotopie. Vers un urbanisme temporel.  

E-Print Network [OSTI]

??Cette thse s'intresse la prise en compte des rythmes urbains en urbanisme. Alors que les volutions conomiques, sociales et techniques ont progressivement transform nos (more)

Mallet, Sandra

2009-01-01T23:59:59.000Z

387

Effet des saponines strodiques de fe-nugrec sur l'hypercholestrolmie du  

E-Print Network [OSTI]

rat des sables diabétique et hypercholestérolémique. Y Dahmani 1,Y Dahmani J Catala F Fichaux C Azema

Boyer, Edmond

388

E-Print Network 3.0 - atlfastii implementierung des Sample Search...  

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Advanced Search Sample search results for: atlfastii implementierung des Page: << < 1 2 3 4 5 > >> 1 Implementierung von Algebren in Summary: Implementierung von Algebren in...

389

E-Print Network 3.0 - auswirkungen des klimas Sample Search Results  

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sind... Meteorologie, das Institut fr Kstenforschung des GKSS-Forschungszentrums Geesthacht und das Deutsche... Klimarechenzentrum beteiligt sind. Am Hamburger KlimaCampus...

390

E-Print Network 3.0 - aktuellen stand des Sample Search Results  

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des Monats Communicatorpreis-Preis 2011 an Gerd Gigerenzer Der Source: Manstein, Dietmar J. - Department of Biophysical Chemistry, Medizinische Hochschule Hannover Collection:...

391

E-Print Network 3.0 - automatique des reacteurs Sample Search...  

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des Materiaux et du Genie Physique (LMGP) en partenariat avec Schneider Electric dans le cadre... tempo lent les themes les plus reussis et nous amene a...

392

E-Print Network 3.0 - air depollution des Sample Search Results  

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Suprieure des Mines de Saint-Etienne Collection: Mathematics 15 Intertemporal Emissions Trading and Market Power: A Dominant Firm with Competitive Fringe Model Summary: with...

393

E-Print Network 3.0 - alloys etude des Sample Search Results  

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ALLOYS Summary: , Section de Physique du Solide, 85 X-38041 Grenoble Cedex, France Resume. - Une etude cxperimentalc des... JOLKhAL 1)t PHYSIQLI: INTERACTION OF ORDER WITH...

394

E-Print Network 3.0 - adaptation des fiches Sample Search Results  

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Catgorie Emploi Catgorie B BAP Emploi type Poste localis GMP IUT... MISSION OU RESUME DES FONCTIONS exercer sur ce poste Maintenance ... Source: Sart, Remi -...

395

E-Print Network 3.0 - artikel des frhrn Sample Search Results  

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17 Erste Satzung zur nderung der Zulassungsordnung der Universitt Stuttgart fr den Deutsch-Franzsischen Masterstudiengang Empirische Politik-und Sozialforschung Summary: des...

396

E-Print Network 3.0 - abschludatum des vorhabens Sample Search...  

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Antrag auf Zulassung zum Promotionsverfahren Summary: Vorlufiger Arbeitstitel (in Deutsch oder Englisch): Working title (in German or English): Beginn des... - see also 3...

397

E-Print Network 3.0 - absicherung des betriebsverhaltens Sample...  

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Lehre des Institutes mit eingebunden und knnen so spannende Erfahrungen im Bereich Deutsch... Finanzierung und Absicherung luft ber das Erasmus-Programm zwischen der...

398

E-Print Network 3.0 - als gegenstand des Sample Search Results  

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and Information Sciences 52 Fachprfungsordnung fr den Bachelor-Teilstudiengang Deutsch als Fremdsprache Summary: . 545). 2 Studium (1) Das Studium des Fachmoduls Deutsch...

399

Elektrische Charakterisierung und Modellierung von metallischen Interkonnektoren (MIC) des SOFC-Stacks.  

E-Print Network [OSTI]

??In dieser Arbeit wurde der Effekt des metallischen Interkonnektors (MIC) auf die Leistungsdichte der anodengesttzten Zelle (ASC) sowie die Wechselwirkung zwischen dem MIC und der (more)

Kornely, Michael

2012-01-01T23:59:59.000Z

400

Estimation des param`etres d'un moteur pas-`a-pas sans capteur mecanique  

E-Print Network [OSTI]

vitesse. L'estimation des param`etres du PMSM, ´etudi´ee par exemple dans Blauch et al. [1993], utilise

Boyer, Edmond

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401

ccsd-00003283,version1-24Nov2004 Des correctifs de scurit la mise jour  

E-Print Network [OSTI]

distribué et injection à chaud Nicolas Loriant - Marc Ségura-Devillechaise - Jean-Marc Menaud ?cole des

Paris-Sud XI, Université de

402

Untersuchungen zur diagnostischen Wertigkeit der urinbasierten Marker Zytologie, FISH, NMP22 und ImmunoCyt in Urinproben aus dem oberen Harntrakt zur Detektion von Urothelkarzinomen des oberen Harntraktes .  

E-Print Network [OSTI]

??Nierenbecken- und Harnleitertumoren ergeben ungefhr 5 - 10% aller Tumoren des Harntraktes. Da sich der berwiegende Teil der Tumoren des oberen Harntraktes bei Diagnosestellung bereits (more)

Esser, Michael

2015-01-01T23:59:59.000Z

403

tude multi-chelle du comportement thermo-hydro-mcanique des matriaux cimentaires : approche morphologique pour la prise en compte de la msostructure.  

E-Print Network [OSTI]

??L'tude du comportement du bton en temprature est un problme majeur qui vise in fine valuer le niveau de scurit des structures sous des (more)

Le, Thi Thu Huong

2011-01-01T23:59:59.000Z

404

Recherche de l'conomie des ressources naturelles par des tudes de conception de coeurs de racteurs eau et haut facteur de conversion combustibles mixtes Thorium / Uranium / Plutonium.  

E-Print Network [OSTI]

??Dans le cadre des tudes neutroniques d'innovation sur les curs de Racteurs Eau lgre Pressurise (REP) de 3me gnration, la recherche de l'conomie des (more)

Vallet, Vanessa

2012-01-01T23:59:59.000Z

405

Les liens de l'eau Les oasis abritent des villages et des jardins luxuriants dans les rgions  

E-Print Network [OSTI]

agriculteurs. Oasis de Figuig (Maroc). Le « gardien des eaux » mesure le volume d'eau du bassin grâce à une canne graduée et en déduit la part de chacun. Oasis de Figuig (Maroc). Un coup de houe ouvre la voie à l (Maroc). Pour approvisionner cette oasis tunisienne, un cours d'eau permanent a été en parti dévié par un

406

Publi dans: Hoffmann, Odile, 2001. Flux et reflux des catgories identitaires. Une lecture des politiques foncires au  

E-Print Network [OSTI]

, conditionnaient la reconnaissance de leurs droits fonciers en les situant dans les scènes de négociation acceptées redéfinir leurs relations dans des cadres largement préconstruits par les sociétés du Nord. RESUMEN Desde la nature multi-ethnique et pluri-culturelle de la nation. Elle confirme et amplifie les droits fonciers

Paris-Sud XI, Université de

407

Quels outils de gestion des prlvements en eau agricole pour faire face la rduction annonce des disponibilits en eau ?  

E-Print Network [OSTI]

Quels outils de gestion des prélèvements en eau agricole pour faire face à la réduction annoncée démographique. C'est notamment le cas dans la plaine du Roussillon, caractérisée par une forte croissance nécessitera l'instauration d'une gestion de l'eau, en particulier de l'eau destinée à l'irrigation. Nous avons

Paris-Sud XI, Université de

409

Die nderung tritt nach der Genehmigung des Rek-tors mit Wirkung vom 1. Oktober 2007 in Kraft.  

E-Print Network [OSTI]

Artikel 2 Die ?nderung tritt nach der Genehmigung des Rek- tors mit Wirkung vom 1. Oktober 2007 ?nderung tritt nach der Genehmigung des Rek- tors mit Wirkung vom 1. Oktober 2007 in Kraft. Bremen, den 10

Hoffmeister, Thomas S.

410

L. JANICKI.2014 Feinere Zerlegung der Spektrallinien von Quecksilber, Kadmium, Natrium, Zink, Thallium und Wasserstoff (Dcomposition des raies spectrales  

E-Print Network [OSTI]

, Thallium und Wasserstoff (Décomposition des raies spectrales du mercure, du cadmium, du sodium, du zinc, du

Boyer, Edmond

411

Synthse de la table ronde n 4 De la terre aux aliments, des valeurs aux rgles... Quelles solutions ?  

E-Print Network [OSTI]

directement à l'encontre des travaux d'Amartya Sen qui, dans son ouvrage Poverty and Famines: An Essay

Paris-Sud XI, Université de

412

STRUCTURE ET ENREGISTREMENT DES TRACES LATENTES D'IONS ARGON ET FER DANS L'OLIVINE ET LE MICA MUSCOVITE  

E-Print Network [OSTI]

attaque chimique : l'enre- gistrement des traces n'apparat pas li un mcanisme seuil nergtique

Boyer, Edmond

413

Alleaume, Denis, 1998, L'Egypte l'aube du XXe sicle : Pays, bourgs, cits en des temporalits divergentes,  

E-Print Network [OSTI]

Alleaume, Denis, 1998, L'Egypte l'aube du XXe sicle : Pays, bourgs, cits en des temporalits L'Egypte l'aube du XXe sicle : Pays, bourgs, cits en des temporalits divergentes Ghislaine), SEDET, universit Paris 7, 2009 Dans les travaux sur l'histoire rcente des villes d'Egypte, l

Boyer, Edmond

414

Le dynamisme des nouvelles places marchandes de l'Est algrien : reconfiguration urbaine et nouvelles donnes sociales  

E-Print Network [OSTI]

1 Le dynamisme des nouvelles places marchandes de l'Est algérien : reconfiguration urbaine et Dynamiques urbaines et accumulation marchande L'importance des politiques publiques dans les processus de libéralisation du marché à partir des années 1990, et l'importante accumulation marchande qui en découlera vont

Paris-Sud XI, Université de

415

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

E-Print Network [OSTI]

METAFOR et CMIP5 #12; Projet européen (EU-FP7) Initiative du European Network for Earth System Modelling (NOAA/NCAR/GFDL) CERA2 (MPI) BFG (Univ. Of Manchester) ESMF (Earth System Modeling Framework, NASA

416

Adsorption of the first layer of argon on graphite (*) Laboratoire des Composs non St0153chiomtriques,  

E-Print Network [OSTI]

]. The cooling bath is solid nitrogen obtained by pumping. The adsorption cell, enclosed in an aluminium blockL-9 Adsorption of the first layer of argon on graphite (*) F. Millot Laboratoire des Composés non déterminé des isothermes d'adsorption d'argon sur le graphite entre 55 et 62 K. Nous proposons une

Boyer, Edmond

417

Apprciation simple de la maturit des composts urbains en relation avec leurs effets sur la pro-  

E-Print Network [OSTI]

Apprciation simple de la maturit des composts urbains en relation avec leurs effets sur la pro54500 Vandceuvre RSUM Des composts prlevs dans diffrentes usines aprs divers temps de maturation de composts jeunes, puis cet effet s'attnue et devient mme positif aprs plusieurs mois de

Boyer, Edmond

418

Facult des Sciences de Bizerte Tl. (216)72591906-Fax. (216)72590566 Deuxime Colloque Maghrbin  

E-Print Network [OSTI]

(Université Casablanca, Maroc) A.ABOUQATEB (Université Marrakech, Maroc) A. AROUCHE (Université des Sciences et. BONATTI (Université de Bourgogne, France) M. BOUCETTA (Université Marrakech, Maroc) O. ECHI (Univ. El, Lyon I, France) A.IKHEMAKHEN (Université Marrakech, Maroc) I. LIOUSSE (Université des Sciences et Techn

El Kacimi, Aziz

419

Erste Satzung zur nderung der Fachprfungsordnung des Masterstudiengangs Health Care Management  

E-Print Network [OSTI]

1 Erste Satzung zur nderung der Fachprfungsordnung des Masterstudiengangs Health Care-Moritz-Arndt-Universitt Greifswald die folgende Satzung zur nderung der Fachprfungsordnung des Masterstudiengangs Health Care Masterstudiengangs Health Care Management vom 15. Mrz 2011 (Mittl.bl. BM M-V 2011 S. 288) wird wie folgt gendert

Greifswald, Ernst-Moritz-Arndt-Universitt

420

Direction gnrale des technologies de l'information et de la communication  

E-Print Network [OSTI]

(ITIL), qui lui permettra de revoir tout son processus de gestion des incidents et des requêtes et de sa première phase, l'implantation du référentiel ITIL touche surtout les processus nécessaires au bon

Charette, André

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

80 L'intelligence Cerveau & Psycho Une bonne mmoire, des qualits de raisonnement,  

E-Print Network [OSTI]

'entraînement, et être un pilote de ligne requiert d'avoir longuement piloté des avions. Cette caractéristique de l distingue par la façon dont les connaissances sont organisées dans sa mémoire. Des capacités acquises Ess_09

Jeanjean, Louis

422

Les dfis de l'valuation conomique du patrimoine urbain des pays en dveloppement  

E-Print Network [OSTI]

Les dfis de l'valuation conomique du patrimoine urbain des pays en dveloppement Methods for the economic valuation of urban heritage: a sustainability-based approach L. Dalmas, V. Geronimi, J.-F. Nol, J2013 #12;3 Les dfis de l'valuation conomique du patrimoine urbain des pays en dveloppement Methods

Boyer, Edmond

423

Systmes d'information centrs rseau : Contributions la gestion des situations de crise  

E-Print Network [OSTI]

Systmes d'information centrs rseau : Contributions la gestion des situations de crise Le cas d'information centrs rseau : Contributions la gestion des situations de crise Le cas d'une crise sanitaire chez'une crise sanitaire chez Leclerc Agns LANCINI Matre de confrences en Sciences de Gestion Universit Aix

Boyer, Edmond

424

Journes Scientifiques de l'Environnement La transition cologique des mgapoles, 12 -14 fvrier 2013  

E-Print Network [OSTI]

laquelle les ressources productives, dont le foncier, font l'objet d'usages en partie concurrentiels avec, fortement dans les pays du sud et de plus en plus dans les pays du nord, aux approvisionnements alimentaires des espaces agricoles proches des villes. C'est largement le cas en ?le-de-France par exemple, où plus

Paris-Sud XI, Université de

425

CAHIER DU CAMPUS LOGISTIQUE N2 Des carrefours intelligents pour une meilleure gestion du  

E-Print Network [OSTI]

CAHIER DU CAMPUS LOGISTIQUE N2 Des carrefours intelligents pour une meilleure gestion du gestion du trafic en milieu urbain ncessite le dploiement de solutions techniques innovantes pour Journal Europen des Systmes Automatiss. MOTS-CLS : gestion du trafic, rseau de Petri hybride, systme

Boyer, Edmond

426

GESTION DURABLE DES RISQUES D'AFFAISSEMENT MINIER : CHOIX DE STRATEGIES -CAS DE MOYEUVRE-GRANDE.  

E-Print Network [OSTI]

GESTION DURABLE DES RISQUES D'AFFAISSEMENT MINIER : CHOIX DE STRATEGIES - CAS DE MOYEUVRE abandonnes. La gestion des risques qui en dcoule peut se faire selon diffrentes stratgies et conduire un application l'tude du cas de la commune de Moyeuvre-Grande (57) travers une analyse cots

Boyer, Edmond

427

Intgration des mares dans la gestion du massif forestier de Snart (Essonne)  

E-Print Network [OSTI]

1 Intgration des mares dans la gestion du massif forestier de Snart (Essonne) Grard HERBUVEAUX1 la gestion ordinaire d'une fort domaniale, en prenant comme exemple la fort domaniale de Snart'homme, dans la majorit des cas la suite de l'extraction de meulire. Les comblements de mares ont t trs

Boyer, Edmond

428

LA CERTIFICATION FORESTIERE COMME NORME DE GESTION DURABLE DES FORETS TROPICALES : UNE LABORIEUSE APPLICATION EN AFRIQUE  

E-Print Network [OSTI]

LA CERTIFICATION FORESTIERE COMME NORME DE GESTION DURABLE DES FORETS TROPICALES : UNE LABORIEUSE sous l'effet de pressions du march europen que par souci cologique de gestion durable des forts nombreuses Organisations Non Gouvernementales Internationales (ONGI) bases dans les pays du Nord et militant

Boyer, Edmond

429

Gestion de la cohrence des rgles mtier dites partir d'ontologies OWL  

E-Print Network [OSTI]

Gestion de la cohrence des rgles mtier dites partir d'ontologies OWL Amina Chniti1,2 , Patrick Albert1 , Jean Charlet2,3 1 IBM, CAS France {amina.chniti,albertpa}@fr.ibm.com 2 INSERM UMRS 872 effectu propose une mthode pour la gestion des relations entre les ontologies et les rgles mtier en

Boyer, Edmond

430

treiben. Wenn die Intelligenz der Fahrzeuge in das Zentrum des wissenschaftlichen In-  

E-Print Network [OSTI]

öffnen wird. · ZUM GELEIT Geleitwort des Rektors Automobil- und Motorentechnik haben in Stuttgart und Baden-Württemberg eine lange Tradition, und Stuttgart gilt als Ge- burtsstadt des Automobils. Baden- när an der Universität Stuttgart mit dem Automobil beschäftigt, ist das Institut für

Möbius, Bernd

431

Enjeux des agrocarburants au Burkina Faso : le cas du Jatropha curcas L.  

E-Print Network [OSTI]

Enjeux des agrocarburants au Burkina Faso : le cas du Jatropha curcas L. Pierre JANIN, géographe. Dans ce domaine, une plante agroénergétique se distingue plus particulièrement ­ le Jatropha curcas L, souvent peu scientifiques, autour du Jatropha (et plus géné- ralement des agrocarburants), le besoin de

Paris-Sud XI, Université de

432

Zielsetzungen und Rahmenbedingungen fr die Gewhrung des Siemens-ZIB-Doktorandenstipendiums (inklusive Anlage)  

E-Print Network [OSTI]

Zielsetzungen und Rahmenbedingungen fr die Gewhrung des Siemens-ZIB-Doktorandenstipendiums (inklusive Anlage) Die Firma Siemens AG und das KonradZuseZentrum fr Informationstechnik Berlin (ZIB. Verantwortlich fr die Vergabe des SiemensZIBDoktorandenstipendiums und fr die Betreuung der Doktoranden sind

Andrzejak, Artur

433

Bielefelder Poet in Residence ist eine Veranstaltung des Fachs Germanistik der Fakultt fr Linguistik und Literatur-  

E-Print Network [OSTI]

Bielefelder Poet in Residence ist eine Veranstaltung des Fachs Germanistik der Fakultät für Studierenden die Werke des Poet, sie erfahren etwas vom ihrem/ seinem Schreiballtag ­ von Inspirationen öffentliche Lesungen. Den Auftakt der Reihe Bielefelder Poet in Residence macht 2012 Zoran Drvenkar. Er wurde

Moeller, Ralf

434

Institut des Nanotechnologies de Lyon UMR CNRS 5270 http://inl.cnrs.fr  

E-Print Network [OSTI]

Institut des Nanotechnologies de Lyon UMR CNRS 5270 http://inl.cnrs.fr 9 February 2012 / Vol.1, No.1 / INL COMMUNICATIONS: TOOLS FOR PHOTONICS 1 Propagation of an electromagnetic lightwave through *,1 * Université de Lyon, Institut des Nanotechnologies de Lyon (INL) UMR 5270 CNRS- INSA-ECL-UCBL 1

Paris-Sud XI, Université de

435

Successful Attack on an FPGA-based WDDL DES Cryptoprocessor Without Place and Route Constraints.  

E-Print Network [OSTI]

Successful Attack on an FPGA-based WDDL DES Cryptoprocessor Without Place and Route Constraints method to improve Side Channel Attacks (SCAs) on Dual-rail with Precharge Logic (DPL) countermeasure to perform advanced attacks. We have experimentally validated the proposed method by attacking a DES

Paris-Sud XI, Université de

436

TUDE EXPRIMENTALE PAR SPECTROMTRIE INFRAROUGE DE L'INFLUENCE DES FORCES DE SURFACE  

E-Print Network [OSTI]

rateur externe ou celui qui existe a la surface des cristaux d'halog6nures alcalins ou d'autres mat6riaux (halog6nures alcalins, teflon) ou n'en pr6sentant pas (polyethylene, polyisobutylene), il se produit des

Paris-Sud XI, Université de

437

Comptes Rendus des JNC 17 -Poitiers 2011 Elaboration et caractrisation mcanique de composites matrice cramique  

E-Print Network [OSTI]

ceramic matrix composites R. Etchart-Salas, S. Jacques, A. Coradi, E. Martin Laboratoire des Composites Keywords : ceramic matrix composite, mechanical testing, acoustic emission, damage, modeling 1 IntroductionComptes Rendus des JNC 17 - Poitiers 2011 1 Elaboration et caractérisation mécanique de composites

Paris-Sud XI, Université de

438

Approche micromcanique statistique-probabiliste de la multifissuration des fils transversaux d'un CMC tiss  

E-Print Network [OSTI]

presents the basis of a new stochastic approach to multiple cracking in transverse tows in ceramic matrix Pierre PINEAU, Jacques LAMON Laboratoire des Composites ThermoStructuraux 3 allée de la Boétie ­ 33600-probabiliste de la multi fissuration des fils transversaux au sein d'un composite tissé à matrice céramique (CMC

Boyer, Edmond

439

SUR L'ANALYSE THERMODYNAMIQUE DES FORCES LECTROMOTRICES. Par M. JEAN VILLEY.  

E-Print Network [OSTI]

'auteur éclaire et complète; par l'analyse des diverses forces électro- motrices capables d'entretenir un courant. Les conclusions principales auxquelles conduit l'analyse méthodique des forces électro- motrices

Paris-Sud XI, Université de

440

Une analyse des liens entre types de Green IT et stratgies RSE  

E-Print Network [OSTI]

: France (2013)" #12;ABSTRACT This communication addresses the issue of the adoption of green technologiesUne analyse des liens entre types de Green IT et stratégies RSE An analysis of links between Green/INSTEAD (Luxembourg), CREM R?SUM? Cette communication aborde la question de l'adoption des technologies vertes ou

Boyer, Edmond

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

Energie hydrolectrique et barrages Facult des Sciences Applique, Dpartement d'Hydraulique et de Transport  

E-Print Network [OSTI]

importante et produit une nergie propre et entirement renouvelable, sans aucune mission de gaz effet de'nergie renouvelable et propre Aprs avoir travers les turbines des barrages, les eaux rejoignent les rivires, puis renouvelable. Comme les ancestrales roues aubes tour- nant sous la simple action du courant, les turbines des

Lige, Universit de

442

Production d'nergie et environnement Facult des Sciences Appliques, Unit de recherche  

E-Print Network [OSTI]

des turbines gaz et vapeur et brlent quasi exclusivement du gaz naturel, verront leur rendement combustion du charbon, du gaz naturel et dans une moindre mesure du ptrole; Les centrales nuclaires qui moulins vent), les turbines hydro-lectriques qui font la mme chose avec l'nergie de l'eau des cours d

Lige, Universit de

443

Section des Units de recherche Rapport de l'AERES sur l'unit  

E-Print Network [OSTI]

Section des Unités de recherche Rapport de l'AERES sur l'unité : Groupe d'études de l représentant de l'AERES : M. Daniel GUEDALIA Représentant(s) des établissements et organismes tutelles de l

Ribes, Aurélien

444

Satzung zur Streichung des Schwerpunkts Niederdeutsch in den Lehramtsstudiengngen Deutsch Gymnasium und Regionale Schule  

E-Print Network [OSTI]

1 Satzung zur Streichung des Schwerpunkts Niederdeutsch in den Lehramtsstudiengängen Deutsch Deutsch im Lehramtsstudiengang Gymnasium Die Prüfungs- und Studienordnung für den Teilstudiengang Deutsch: 1. § 2 Absatz 2 wird wie folgt gefasst: ,,(2) Für Lehramtsstudierende des Teilstudiengangs Deutsch

Greifswald, Ernst-Moritz-Arndt-Universität

445

Digestion des glucides cytoplasmiques de la fverole par le veau prruminant  

E-Print Network [OSTI]

Digestion des glucides cytoplasmiques de la fverole par le veau prruminant J. M. BESLE B. LASSALAS, P. THIVEND Laboratoire de la Digestion des Ruminants, LN.R.A. Theix 63110 Beaumont France. Summary. Digestion of field bean cytoplasmic carbohydrates by the preruminant calf. Three veal calves

Paris-Sud XI, Universit de

446

Article original Digestion des protines de pois et de soja chez le veau  

E-Print Network [OSTI]

Article original Digestion des protines de pois et de soja chez le veau prruminant. II partiellement dgrades puissent chapper la digestion dans l'intestin grle dans le cas des aliments pois et - digestion - ilon - veau prruminant Summary ― Digestion of pea and soya-bean proteins in preruminant

Paris-Sud XI, Universit de

447

Digestion des glucides de la levure d'alcanes par le veau prruminant  

E-Print Network [OSTI]

Digestion des glucides de la levure d'alcanes par le veau prruminant J. M. BESLE, Bernadette LASSALAS, P. THIVEND Laboratoire de la Digestion des Ruminanfs, 1.N.R.A., Theix, 63110 Beaumont France. Summary. Digestion of alkane yeast carbohydrates by the preruminant calf. Four 15-day old preruminant

Paris-Sud XI, Universit de

448

On hybrid control of complex systems: Sur la commande hybride des systmes  

E-Print Network [OSTI]

On hybrid control of complex systems: a survey Sur la commande hybride des syst·mes complexes a brief overview of hybrid control systems is given and an introduction to several approaches in hybrid to hybrid control. RESUME. L'objectif de cet article est de prZsenter un Ztat de l'art des travaux relatifs

Koutsoukos, Xenofon D.

449

STRUCTURE ET DYNAMIOUE DES RESEAUX DETERMINATION OF THE EIGENVECTORS OF SOFT MODES  

E-Print Network [OSTI]

Ble du deplacement des atomes dans le mode ferro- klectrique de KDzP04 a l'aide de la mkthode des dries be dropped, since we shall be dealing with only one optic mode at a time). Fourier transformation gives is proportional to b, u,, where b, is the coherent neutron scattering length for an atom of type K. For a phonon

Paris-Sud XI, Université de

450

MINISTERE DES AFFAIRES ETRANGERES ET EUROPEENNES AMBASSADE DE FRANCE AU KENYA  

E-Print Network [OSTI]

1 MINISTERE DES AFFAIRES ETRANGERES ET EUROPEENNES AMBASSADE DE FRANCE AU KENYA FICHE CURIE ENSEIGNEMENT SUPERIEUR KENYA I. Organisation de l'enseignement supérieur a. Management de l'enseignement technique Le Kenya compte de nombreuses institutions d'enseignement technique qui offrent en 1 à 4 ans des

Hélein, Frédéric - Institut de Mathématiques de Jussieu, Université Paris 7

451

colloque des Archives d'Agde. Agde, 11 juin 2005 Association pour la Promotion des Archives d'Agde et de sa Rgion  

E-Print Network [OSTI]

étangs dans les plaines périphériques de la Méditerranée fait qu'ils sont au coeur, en non en marge, de l. Il faut ajouter à ce besoin strictement alimentaire en céréales une recherche du profit et de pouvoir de la part des maîtres de la terre : les seigneurs, qu'il s'agisse des laïcs (nobles locaux et

Boyer, Edmond

452

La France et l'Iran, des nations si lointaines et si proches 197 La France et l'Iran, des nations  

E-Print Network [OSTI]

La France et l'Iran, des nations si lointaines et si proches 197 La France et l'Iran, des nations si lointaines et si proches Le recteur Gérard-François DUMONT* La France et l'Iran apparaissent comme'autre. Pour les Français, comme sans doute pour les autres Européens, penser ce pays asiatique qu'est l'Iran

Paris-Sud XI, Université de

453

L2-Logique, TD5 Calcul des propositions  

E-Print Network [OSTI]

L2-Logique, TD5 2007/08 Calcul des propositions 1 D´emonstrations Dans cette partie, utilisez le m´eta-th´eor standard. On interpr`ete ce syst`eme par l'alg`ebre de Boole standard. 2 - Est-ce que tout th´eor`eme de CP) (A B) | A, B FCP0 } 4 - Est-ce que toute tautologie est un th´eor`eme de CP0' ? 5 - Le m´eta-th´eor

Narboux, Julien

454

Des Plaines Landfill Biomass Facility | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump to:52c8ff988c1Dering Harbor, New York: Energy Resources JumpDes Plaines

455

Des Plaines, Illinois: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump to:52c8ff988c1Dering Harbor, New York: Energy Resources JumpDes Plaines

456

LA SARCOSPORIDIOSE DES RUMINANTS AU MAROC ETUDE EPIDEMIOLOGIQUE PAR DEUX TECHNIQUES HISTOLOGIQUES  

E-Print Network [OSTI]

LA SARCOSPORIDIOSE DES RUMINANTS AU MAROC ETUDE EPIDEMIOLOGIQUE PAR DEUX TECHNIQUES HISTOLOGIQUES Agronomique et Vétérinaire Hassan Il. B.P. 704 - Rabat - Agdal. Maroc &dquo; Département de Parasitologie

Boyer, Edmond

457

HYBRIDITES ARCHITECTURALES EN TUNISIE ET AU MAROC AU TEMPS DES PROTECTORATS  

E-Print Network [OSTI]

HYBRIDITES ARCHITECTURALES EN TUNISIE ET AU MAROC AU TEMPS DES PROTECTORATS : ORIENTALISME dans "Architectures au Maroc et en Tunisie à l'époque coloniale, Tunisie (2009)" #12;plus large. Pour

Boyer, Edmond

458

Modifications du travail de sortie des surfaces clives de GaAs, lies au refroidissement  

E-Print Network [OSTI]

les positions energetiques des etats de surface. Cette idee a ete reprise et developpee par L. K experimentaux ne posent pas de probleme majeur [6], 1'exp6rimentation, delicate, conduit a se poser la question

Boyer, Edmond

459

Zweite Satzung zur nderung der Studienordnung des Masterstudiengangs ,,Health Care Management" an der  

E-Print Network [OSTI]

1 Zweite Satzung zur nderung der Studienordnung des Masterstudiengangs ,,Health Care Management die folgende nderungssatzung der Studienordnung fr den Masterstudiengang ,,Health Care Management" (HCM) als Satzung: Artikel 1 Die Studienordnung fr den Masterstudiengang ,,Health Care Management" (M

Greifswald, Ernst-Moritz-Arndt-Universitt

460

Annual Report 2009 Eawag: Das Wasserforschungs-Institut des ETH-Bereichs  

E-Print Network [OSTI]

Annual Report 2009 Eawag: Das Wasserforschungs-Institut des ETH-Bereichs #12;Cover photo Kai Udert in the future. Pictured here, a microbiological fuel cell running on urine (for more details see p. 28). Photo

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.


461

DE LA RUE AU PALAIS MUNICIPAL. LA GESTION DES CONFLITS SOCIAUX  

E-Print Network [OSTI]

#12;DE LA RUE AU PALAIS MUNICIPAL. LA GESTION DES CONFLITS SOCIAUX PAR LE PARTI DE LA RVOLUTION parti politique3 . Pour cette raison, le cas du Parti de la Rvolution dmocratique (PRD), au Mexique

Boyer, Edmond

462

EURECOM 2229 Route des Crtes BP 193 F-06904 Sophia Antipolis cedex  

E-Print Network [OSTI]

EURECOM ­ 2229 Route des Crêtes ­ BP 193 F-06904 Sophia Antipolis cedex www.eurecom.fr Spatial, Sophia Antipolis, France http://www.openairinterface.org bassem.zayen@eurecom.fr 2. Cognitive Radio

Gesbert, David

463

E-Print Network 3.0 - avec des enfants Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

enfants Search Powered by Explorit Topic List Advanced Search Sample search results for: avec des enfants Page: << < 1 2 3 4 5 > >> 1 ANNEXE 1, Chapitre 5 : Diverses situations...

464

E-Print Network 3.0 - appendices inventaire des Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

VER... Extraire les documents des locaux d'archivage 5 CA Trier selon les procdures ad-hoc 6 CA Re... -conditionner les documents conserver 8 AP, RO, CA Modifier les...

465

pour obtenir le grade de Docteur des universits Paris-Est et Tunis El Manar  

E-Print Network [OSTI]

'oxydation avancée Degradation of pesticides chlortoluron, carbofuran and bentazone in aqueuos medium by advanced des pesticides chlortoluron, carbofurane et bentazone en milieux aqueux par les procédés d

Paris-Sud XI, Université de

466

E-Print Network 3.0 - approche smio-cognitive des Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

historique... centennale Vallon (Naulet, 2002) 12;19 1.4 Approche naturaliste Hydro-gomorphologie Analyse des units... maximale du champ d'inondation Garry G., et al....

467

tel-00651477,version1-13Dec2011 Problmatiques(s) des rapports soma/psych  

E-Print Network [OSTI]

atteinte fonctionnelle des fonctions motrices et/ou sensorielles sans que lon puisse en donner une plus particulièrement sur les paralysies motrices hystériques où les investigations neurologiques

Paris-Sud XI, Université de

468

Thse prpare au Laboratoire d'Analyse et d'Architecture des Systmes du CNRS  

E-Print Network [OSTI]

2007 Spécialité : Intelligence Artificielle par Nicolas Do Huu APPRENTISSAGE DE REPR?SENTATIONS SENSORI-MOTRICES . . . . . . . . . . . . . . . . . . . . . 19 I. La boucle sensori-motrice . . . . . . . . . . . . . . . . . . . . . . 19 II. Apprentissage des

Paris-Sud XI, Université de

469

E-Print Network 3.0 - apres radiotherapie des Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

des diffrents travaux. tel-00585878,version1-14Apr2011 12;41 Article n 2 - External irradiation... .vinchon-petit@unimedia.fr tel-00585878,version1-14Apr2011 12;43 ABSTRACT...

470

Universit Paris-Est-Crteil-Val de Marne Facult des Lettres, Langues et Sciences Humaines  

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philosophiques de la théorie du choix social à l'évaluation démocratique des capabilités d'Amartya Sen Directeur

Paris-Sud XI, Université de

471

Ecotoxicit des terres rares Les terres rares sont un groupe de mtaux qui  

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'automobile pour dpolluer les gaz d'chappement constituent le principal dbouch des terres rares (tout vhicules hybrides, les turbines d'oliennes ainsi que dans le nuclaire et l'armement. Les terres rares ont

Wehrli, Bernhard

472

CLASSIFICATION DES PHNOMNES OBSERVS comme chocs lastiques (p, p), 20 % probable-  

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. - L'examen de nos premiers ré- sultats montre que la chambre à bulles à propane peut être un que la simple pro- jection orthogonale. COURBES PARCOURS-?NERGIE DES PARTICULES 03B1 DANS L

Paris-Sud XI, Université de

473

Universit des Sciences et Technologies de Lille Numro d'Ordre: 3506 Anne: 2005  

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networks technologies are useless. Managing services consists in providing a reliable and easy wayifL Universit des Sciences et Technologies de Lille Numro d'Ordre: 3506 Anne: 2005 Thse

Paris-Sud XI, Universit de

474

AM ABEND DES 20. SEPTEMBER 2002 lste sich eine gigantische Eis-und Steinlawine vom Nord-  

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#12;AM ABEND DES 20. SEPTEMBER 2002 lste sich eine gigantische Eis- und Steinlawine vom Nord- hang Eis nur schwer aus- zumachen: ein Teil der Gletscherflchen ist stets mit Schutt bedeckt. ASTER hat

Kb, Andreas

475

Article de recherche Analyse pollinique des miels de l'Ontario, Canada  

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Article de recherche Analyse pollinique des miels de l'Ontario, Canada M.J. Feller-Demalsy J. Parent Université du Québecà Rimouski, 300, allée des Ursulines, Rimouski, OC, Canada, G5L 3A11 (reçu le plupart en 1983 et provenant du sud de l'Ontario (Canada) où est concentrée l'activité apicole. Les

Paris-Sud XI, Université de

476

MMOIRES ORIGINAUX A propos de l'origine de la contamination des laits  

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commerciales des PCE à cette époque [1] : · Emploi en systèmes clos contrôlables : les PCE sont utilisés comme: les PCE sont utilisés dans des systèmes hydrauliques et d'échange thermique et dans les petits systèmes non clos donc à produit perdu : les PCE sont utilisés dans la formulation d'huiles de

Paris-Sud XI, Université de

477

Droits fonciers des femmes au Maroc Entre complexit du systme foncier et discrimination  

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Droits fonciers des femmes au Maroc Entre complexité du système foncier et discrimination Fatiha Daoudi E & E, n° 4 Les Etudes et Essais du Centre Jacques Berque N° 4 ­ Octobre 2011 Rabat (Maroc) halshs-00694238,version1-3May2012 #12;halshs-00694238,version1-3May2012 #12;3 Droits fonciers des femmes au Maroc

Boyer, Edmond

478

Serge Marlet et Pierre Ruelle (diteurs scientifiques), 2002. Vers une matrise des impacts  

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de statistique appliquée, IAV Hassan II, Rabat, Maroc ** Département des sciences du sol, IAV Hassan II, Rabat, Maroc *** Unité de science du sol, INRA, Versailles, France Résumé Modélisation de l région des Doukkala au Maroc, a permis de prévoir avec une précision acceptable l'évolution à court terme

Boyer, Edmond

479

Mecanique des Milieux Continus I 18 \\ DCOUVERTE \\N 357 JUILLET-AOT 2008  

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´eformations, lois de comportement et probl`emes aux limites. Une fois tous les concepts introduits, on s'int´eressera `a la r´esolution des probl`emes obtenus et `a la mise en ´evidence des ph´enom`enes qui en d´ecoulent tant en statique qu'en dynamique, en petits qu'en grands d´eplacements. On ´etudiera ainsi les probl`emes

Boyer, Edmond

480

VALIDATION DE METHODE D'ETALONNAGE ET EVALUATION DES INCERTITUDES DE MESURE EN ANALYSE  

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'INERIS, organisme accrédité ISO/CEI/17025, certifié ISO 9001 et reconnu BPL, a pour mission la maîtrise des risques mesure exposés dans ce document. Abstract : INERIS, a certified (ISO 9001) and accredited (ISO/CEI 17025 norme NF ISO 17993 [5]. Le diagramme d'Ishikawa de l'analyse du processus de mesure des HAP par CLHP

Boyer, Edmond

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481

LA NATURE CONTRE LE TERRITOIRE : LES CONTRADICTIONS DE LA POLITIQUE DES AIRES PROTEGEES EN URUGUAY  

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URUGUAY Dorothée Capo. Université de Paris 1, Panthéon-Sorbonne. Pierre Gautreau Université des sciences'environnement est une réalité récente en Uruguay (Achkar et Domínguez, 2000). La création du ministère de l protection des « milieux naturels ». La première originalité tient à la situation écologique de l'Uruguay

Paris-Sud XI, Université de

482

Gestion des rsultats comptables et structure de l'actionnariat : le cas franais  

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1 Gestion des résultats comptables et structure de l'actionnariat : le cas français Yves MARD et gestion et management (CRCGM), Faculté de Sciences ?conomiques et de Gestion, IAE de Clermont Ferrand, E'étudier l'impact de la structure de l'actionnariat sur la gestion du résultat des sociétés cotées françaises

Paris-Sud XI, Université de

483

Notes et tudes conomiques n30, Mars 2008 LA GESTION DES RISQUES EN AGRICULTURE  

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33 Notes et études économiques ­ n°30, Mars 2008 LA GESTION DES RISQUES EN AGRICULTURE De la rurale et gestion, Agrocampus Rennes ** Chargés de mission au bureau de l'analyse économique et de la la gestion des risques en agriculture #12;34 Notes et études économiques ­ n°30, Mars 2008 L

Paris-Sud XI, Université de

484

LA DYNAMIQUE DES SYSTEMES COMME OUTIL D'AIDE A LA GESTION DU SOL URBAIN  

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LA DYNAMIQUE DES SYSTEMES COMME OUTIL D'AIDE A LA GESTION DU SOL URBAIN Monique DANTAS Doctorante qui le composent sont interreliées. Tel est le cas du sol urbain dont la complexité des interactions rend délicate la mise en place de politiques adaptées. La construction d'un modèle de gestion du sol

Paris-Sud XI, Université de

485

Colloque international " L'eau en montagne : gestion intgre des Hauts Bassins Versants "  

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Colloque international " L'eau en montagne : gestion intégrée des Hauts Bassins Versants " 5 et 6, comprenant la plaine située entre l'Atlas au sud et les Jbilet au nord et dont Marrakech est la capitale. L'organisation de la région. C'est le cas de l'agriculture de plaine avec la construction des premières khettara5

Paris-Sud XI, Université de

486

Siph-i Ispahn : devenir des groupes consonantiques initiaux moyen-perses en persan  

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Siph-i Ispahn : devenir des groupes consonantiques initiaux moyen-perses en persan Agnès Lenepveu persan contemporain n'a plus cette structure. On s'interrogera sur les raisons et l'époque de cette transformation. Lorsqu'on observe de près le lexique du persan des Xe -XIe siècles, on a rapidement une

Paris-Sud XI, Université de

487

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

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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

Boyer, Edmond

488

Paris, le 6 janvier 2014 Des rductions rgionales importantes de biomasse dans  

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1/2 Paris, le 6 janvier 2014 Des réductions régionales importantes de biomasse dans l'océan profond futures réductions régionales de biomasse dans l'océan profond à l'aide de modèles du climat de dernière pas à l'abri des impacts du changement climatique et que leur biomasse devrait connaître une forte

Canet, Léonie

489

JOURNEE DES DOCTORANTS DE LA FEDERATION DENIS POISSON 9`eme EDITION  

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JOURN´EE DES DOCTORANTS DE LA F´ED´ERATION DENIS POISSON 9`eme ´EDITION JEUDI 17 OCTOBRE 2013 #12;R´esum´es des expos´es Sylvain ARNT : Espace `a partitions pond´er´ees et actions isom´etriques affines sur un espace de Banach On consid`e le r´esultat suivant d^u `a Robertson-Steger et Cherix

d'Orléans, Université

490

DES NANDERTALIENS DANS LA TROISIME CAVERNE DE GOYET Hlne Rougier, Isabelle Crvecoeur, Patrick Smal & Michel Toussaint  

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DES N?ANDERTALIENS DANS LA TROISI?ME CAVERNE DE GOYET Hélène Rougier, Isabelle Crèvecoeur, Patrick 1870 à la troisième caverne par le géologue ?douard Dupont. La cinquantaine de vestiges mis au jour à). Il y a donc des restes humains récents dans la troisième caverne de Goyet mais, étant donné la

Boyer, Edmond

491

Amartya Kumar Sen, La dmocratie des autres. Pourquoi la libert n'est pas une invention  

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Amartya Kumar Sen, La démocratie des autres. Pourquoi la liberté n'est pas une invention de l'économiste et philosophe Amartya Sen. D'une part, sa foi en la démocratie apparaît comme la raison première de et public. Sen fait partie des auteurs qui défendent une conception de la « démocratie en termes de

Paris-Sud XI, Université de

492

ACROTERIASIS CONGENITA DANS LA RACE PIE NOIRE DES PLAINES EN POLOGNE  

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ACROTERIASIS CONGENITA DANS LA RACE PIE NOIRE DES PLAINES EN POLOGNE H. GERINGER Chaire de Pie noire des Plaines, le défaut héréditaire d'ampu- tation congénitale (Acroteriasis congenita) déjà montrent qu'il peut s'agir d'un déterminisme héréditaire mono- factoriel récessif. Bien qu'incomplets, les

Boyer, Edmond

493

Conflits, bruits et captation des flux : cls de l'organisation spatiale cerdane.  

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différenciations spatiales. Ils sont la réponse des Cerdans aux perturbations qui peuvent les affecter. La organisateur : dès lors, il est possible de dire qu'ils produisent du sens. L'ouverture des frontières, en pyrénéen axial (carte 1). Elle comprend une plaine limitée au nord par le massif du Carlit et de Puigpedros

Boyer, Edmond

494

Approche hybride par la modelisation electromagnetique des interactions en champ proche et en champ lointain  

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Approche hybride par la mod´elisation ´electromagn´etique des interactions en champ proche et en'expansion du champ ´electromagn´etique dans diff´erents rep`eres `a partir de la connaissance des conditions aux limites se trouvent d´ej`a dans Stratton [1]. Ainsi, la connaissance du champ ´electromagn´etique

Boyer, Edmond

495

| L'enqute CNRS I LE JOURNAL l'horizon 2020, la part des  

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on le souhai- tera ;c'estlatechniqueCAES(compressed air energy storage). « Pour le stockage à grande leur nombre, pour des raisons géographiques. Suivant la même logique, l'eau peut être remplacée par l'air- primerl'air,quipourraêtredétenduulté- rieurement dans des turbines afin de restituer l'électricité quand

van Tiggelen, Bart

496

PROCD RAPIDE POUR LA PHOTOMTRIE DES BECS A INCANDESCENCE PAR LE GAZ (1) ;  

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469 PROC?D? RAPIDE POUR LA PHOTOM?TRIE DES BECS A INCANDESCENCE PAR LE GAZ (1) ; Par P. LAURIOL. Les essais des becs à incandescence par le gaz destinés à l'éclai- rage public comportent un très pendant une série de mesures. On emploie une lampe à incandescence électrique dont on #12;471 maintint la

Paris-Sud XI, Université de

497

MESURE DU PARCOURS MOYEN DES RAYONS 03B1 DU THORIUM PAR LA MTHODE PHOTOGRAPHIQUE  

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MESURE DU PARCOURS MOYEN DES RAYONS 03B1 DU THORIUM PAR LA M?THODE PHOTOGRAPHIQUE Par Mme HENRIETTE thorium dans l'émulsion des plaques photo- graphiques, on déduit leur parcours moyen dans l'air à150 thorium a déjà fait l'objet de plusieurs mesures dont les résultats ne sont pas toujours concordants. Les

Paris-Sud XI, Université de

498

CONTRIBUTION A L'TUDE DES SOURCES DE THORIUM C ET DE THORIUM C'  

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583 CONTRIBUTION A L'?TUDE DES SOURCES DE THORIUM C ET DE THORIUM C' Par Marie ADER, Physique atomique, Collège de France. Un dépôt actif de thorium sur disque d'argent de 3 mm de diamètre, constitue plaques impressionnées par une solution de nitrate de thorium par la méthode de contact et la méthode des

Paris-Sud XI, Université de

499

Des bouffes clestes de rayons gamma IAGL : Institut d'Astrophysique et de Gophysique ULg  

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Gamma Ray Bursts). Ceux-ci sont produits lors d'énormes explosions révélées seulement (à l'origine) parDes bouffées célestes de rayons gamma IAGL : Institut d'Astrophysique et de Géophysique ULg Rédigé systèmes américains de surveillance militaire, les 'sursauts gamma' sont maintenant attribués à des

Liège, Université de

500

L'IDENTIT AU MIROIR DU DROIT LE STATUT DES PERSONNES EN EGYPTE,  

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L'IDENTIT? AU MIROIR DU DROIT LE STATUT DES PERSONNES EN EGYPTE, FIN DU XIXe - MILIEU DU XXe SI?CLE sur les statuts et les identités en Egypte, à l'époque où l'ordre ottoman, fondé sur l'abolition des capitulations (1937), privilèges conférés aux étrangers et devenus insupportables à l'Egypte

Paris-Sud XI, Université de