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1

Clean Cities: Lone Star Clean Fuels Alliance (Central Texas) coalition  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Lone Star Clean Fuels Alliance (Central Texas) Coalition Lone Star Clean Fuels Alliance (Central Texas) Coalition The Lone Star Clean Fuels Alliance (Central Texas) coalition works with vehicle fleets, fuel providers, community leaders, and other stakeholders to reduce petroleum use in transportation. Lone Star Clean Fuels Alliance (Central Texas) coalition Contact Information Stacy Neef 512-773-8794 stacy.neef@lonestarcfa.org Coalition Website Clean Cities Coordinator Stacy Neef Photo of Stacy Neef Stacy Neef has served as the coordinator for Lone Star Clean Fuels Alliance (Austin) (LSCFA) promoting and advancing the use of alternative fuel and vehicles for fleets in central Texas since 2000. The central Texas region includes Bastrop, Caldwell, Hays, Travis, Williamson Counties; Fort Hood and City of Temple, Texas. LSCFA works closely with other Texas Clean

2

Lone Star I (Q2) Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Q2) Wind Farm Q2) Wind Farm Jump to: navigation, search Name Lone Star I (Q2) Wind Farm Facility Lone Star I (Q2) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Horizon Developer RES/Horizon Energy Purchaser Direct Energy Location Callahan and Shackelford counties TX Coordinates 32.594885°, -99.506464° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":32.594885,"lon":-99.506464,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

3

Lone Star I (Q3) Wind Farm | Open Energy Information  

Open Energy Info (EERE)

I (Q3) Wind Farm I (Q3) Wind Farm Jump to: navigation, search Name Lone Star I (Q3) Wind Farm Facility Lone Star I (Q3) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Horizon Developer RES/Horizon Energy Purchaser Direct Energy Location Callahan and Shackelford counties TX Coordinates 32.594885°, -99.506464° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":32.594885,"lon":-99.506464,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

4

Lone Star Wind Alliance LSWA | Open Energy Information  

Open Energy Info (EERE)

Wind Alliance LSWA Wind Alliance LSWA Jump to: navigation, search Name Lone Star Wind Alliance (LSWA) Place Houston, Texas Sector Wind energy Product Texas-based research centres, focusing on large composite structures, wind engineering, electromechanical controls and power electronics. The organisation is led by the University of Houston. Coordinates 29.76045°, -95.369784° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":29.76045,"lon":-95.369784,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

5

Lone Star I (4Q07) Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Lone Star I (4Q07) Wind Farm Lone Star I (4Q07) Wind Farm Facility Lone Star I (4Q07) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Horizon Developer RES/Horizon Energy Purchaser Direct Energy Location Callahan and Shackleford Counties TX Coordinates 32.594885°, -99.506464° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":32.594885,"lon":-99.506464,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

6

Solar production of industrial process steam for the Lone Star Brewery. 80% review report  

DOE Green Energy (OSTI)

The solar steam system for the Lone Star Brewery is described in detail. It consists of a roof-mounted parabolic trough collector field heating Monsanto's Therminol T-55 heat transfer fluid, a solar-fired boiler, a heat transfer fluid circulation pump, and all the associated piping. The comparison of various collectors and heat transfer fluids surveyed is reviewed. Also included are discussions of the system performance analysis, economic analysis, safety analysis, data collection, and environmental impact assessment. Numerous drawings illustrate the system, particularly the parallel trough collectors. (LEW)

Deffenbaugh, D.M.; Watkins, P.V.; Hugg, S.B.; Kulesz, J.J.; Decker, H.E.; Powell, R.C.

1979-05-15T23:59:59.000Z

7

Lone Star II (1Q08) Wind Farm | Open Energy Information  

Open Energy Info (EERE)

1Q08) Wind Farm 1Q08) Wind Farm Facility Lone Star II (1Q08) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Horizon Developer RES/Horizon Energy Purchaser JAron Location Callahan and Shackelford counties TX Coordinates 32.594885°, -99.506464° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":32.594885,"lon":-99.506464,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

8

Lone Star II (4Q07) Wind Farm | Open Energy Information  

Open Energy Info (EERE)

4Q07) Wind Farm 4Q07) Wind Farm Facility Lone Star II (4Q07) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Horizon Wind Energy Developer RES/Horizon Energy Purchaser JAron Location Callahan and Shackleford Counties TX Coordinates 32.594885°, -99.506464° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":32.594885,"lon":-99.506464,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

9

Solar production of industrial process steam for the Lone Star Brewery. Final report  

DOE Green Energy (OSTI)

This report outlines the detailed design and system analysis of a solar industrial process steam system for the Lone Star Brewery. The industrial plant has an average natural gas usage of 12.7 MMcf per month. The majority of this energy goes to producing process steam of 125 psi and 353/sup 0/F at about 50,000 lb/h, with this load dropping to about 6000 lb/h on the weekends. The maximum steam production of the solar energy system is about 1700 lb/h. The climatic conditions at the industrial site give 50% of the possible amount of sunshine during the winter months and more than 70% during the summer months. The long-term yearly average daily total radiation on a horizontal surface is 1574 Btu/day-ft/sup 2/, the long-term yearly average daytime ambient temperature is 72/sup 0/F, and the percentage of clear day insolation received on the average day of the year is 62%. The solar steam system will consist of 9450 ft/sup 2/ of Solar Kinetics T-700 collectors arranged in fifteen 90-ft long rows through which 67.5 gpm of Therminol T-55 is pumped. This hot Therminol then transfers the heat collected to a Patterson-Kelley Series 380 unfired steam boiler. The solar-produced steam is then metered to the industrial process via a standard check valve. The thermal performance of this system is projected to produce about 3 million lbs of steam during an average weather year, which is approximately 3 billion Btu's. As with any prototype system, this steam system cannot be justified for purely economic reasons. It is estimated, however, that if the cost of the collectors can be reduced to a mass production level of $3 per lb then this type of system would be cost effective in about six years with the current government incentives and a fuel escalation rate of 10%. This period can be shortened by a combination of an increased investment tax credit and an accelerated depreciation.

Deffenbaugh, D.M.; Watkins, P.V.; Hugg, S.B.; Kulesz, J.J.; Decker, H.E.; Powell, R.C.

1979-06-29T23:59:59.000Z

10

Lone Star Transmission LLC | Open Energy Information  

Open Energy Info (EERE)

LLC Place Juno Beach, Florida Zip 33408 Product Wholly owned subsidiary of FPL Energy, developing transmission lines. First project is the DFW Express high voltage DC...

11

CA-TRIBE-PAIUTE-SHOSHONE INDIANS OF THE LONE PINE  

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

U.S. Department of Energy Categorical Exclusion Determination Form Program or Field Office: Energy Efficiency and Conservation Block Grant Program Project Title CA-TRIBE-PAIUTE-SHOSHONE INDIANS OF THE LONE PINE COMMUNITY Location: Tribe CA-TRIBE-PAIUTE- SHOSHONE INDIANS OF THE LONE PINE COMMUNITY CA American Recovery and Reinvestment Act: Proposed Action or Project Description The Paiute-Shoshone Indians of the Lone Pine Community propose to prepare a feasibility study for

12

Clean Cities: Lone Star Clean Fuels Alliance (Central Texas)...  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

case1": "Next video in 1", "other": "Next video in " This video is currently unavailable. Your browser does not currently recognize any of the video formats available. Click here...

13

Solar production of industrial process steam for the Lone Star Brewery. Conceptual design report  

DOE Green Energy (OSTI)

The project conceptual design activities are divided into six parts: Industrial Plant, Conceptual System Design, Collector Selection, Heat Transfer Fluid Selection, Site Fabrication, and Engineered Equipment. Included is an overview of the solar steam system and a brief discussion on the environmental impact of the project as well as the safety considerations of the system design. The effect of the solar system on the environment is negligible, and the safety analysis of the system indicates the considerations to be taken to minimize any potential safety hazard due to contamination of the food product or to fire. Both of these potential hazards are discussed in detail. Both the question of product contamination and the question of potential fire hazards will be presented to the industrial partner's safety committee so that the selection of the heat transfer fluid meets with their approval.

Deffenbaugh, D.M.

1978-12-29T23:59:59.000Z

14

User Developed Applications and Information Systems Success: A Test of DeLone and McLean's Model  

Science Conference Proceedings (OSTI)

DeLone and McLean's 1992 model of information systems success has received much attention amongst researchers. This study provides the first empirical test of an adaptation of DeLone and McLean's model in the user-developed application domain. The model ...

Tanya McGill; Valerie Hobbs; Jane Klobas

2003-01-01T23:59:59.000Z

15

Beyond the Lone-Pair Model for Structurally Distorted Metal Oxides  

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

Beyond the Lone-Pair Model for Structurally Distorted Metal Oxides Print Beyond the Lone-Pair Model for Structurally Distorted Metal Oxides Print "Ferroelectricity," by analogy to ferromagnetism, is defined as the presence of spontaneous electrical polarization in a material, often arising from distortions in the material's crystal structure. In oxides of the metals lead and bismuth, such distortions were for many years attributed to the existence of "lone pair" electrons: pairs of chemically inert, nonbonding valence electrons in hybrid orbitals that leave noticeable voids in the crystal structure. At the ALS, researchers from the U.K., Ireland, and the U.S. have now obtained definitive experimental evidence that this lone-pair model must be revised. High-resolution x-ray photoemission spectroscopy (XPS) and soft x-ray emission spectroscopy (XES) have clarified the subtle electronic origins of the prototypical distortions in these crystal structures. The results have important implications for the tantalizing possibility of spintronic or superconducting devices combining ferroelectric and ferromagnetic properties.

16

Beyond the Lone-Pair Model for Structurally Distorted Metal Oxides  

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

Beyond the Lone-Pair Model for Structurally Distorted Metal Oxides Print Beyond the Lone-Pair Model for Structurally Distorted Metal Oxides Print "Ferroelectricity," by analogy to ferromagnetism, is defined as the presence of spontaneous electrical polarization in a material, often arising from distortions in the material's crystal structure. In oxides of the metals lead and bismuth, such distortions were for many years attributed to the existence of "lone pair" electrons: pairs of chemically inert, nonbonding valence electrons in hybrid orbitals that leave noticeable voids in the crystal structure. At the ALS, researchers from the U.K., Ireland, and the U.S. have now obtained definitive experimental evidence that this lone-pair model must be revised. High-resolution x-ray photoemission spectroscopy (XPS) and soft x-ray emission spectroscopy (XES) have clarified the subtle electronic origins of the prototypical distortions in these crystal structures. The results have important implications for the tantalizing possibility of spintronic or superconducting devices combining ferroelectric and ferromagnetic properties.

17

Free stars  

E-Print Network (OSTI)

Free stars are certain subsets of a poset, first defined by me in [1]. Free stars are closely related with filters, namely free stars on a boolean lattice bijectively correspond to filters on this lattice. This article introduces consideration of free stars. Some questions are raised. Free stars are useful in my further (yet unpublished) research (in general topology).

Victor Porton; Shay Agnon

2012-01-01T23:59:59.000Z

18

STAR Search STAR Search5 30  

E-Print Network (OSTI)

STAR Search "" STAR STAR Search5 30 Tokyo Tech STAR STAR Search Tech OCW T2R2 Google Web T2R2 Tokyo Tech OCW Web #12; STAR STAR Search DB DB T2R2 Tokyo Tech OCW T2R2 Tokyo Tech OCW STAR Search STAR Search T2R2 Tokyo Tech OCW STAR

19

ENERGY STAR  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

20

ENERGY STAR Snapshot | ENERGY STAR  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

Note: This page contains sample records for the topic "waha lone star" 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

Work, poverty and welfare reform: welfare-to-work programmes for lone parents in depressed local labour markets  

E-Print Network (OSTI)

Appendix I: Interview questions for follow-up interviews with Buffalo lone parents Appendix J: Network view of 'Experience of employment' BIBLIOGRAPHY 220 220 224 225 229 231 232 235 245 247 247 254 258 262 265 267 275 278 279 283... and the US Lake . _~. ___ .J ;/ Ontario , I , ,.~. I , I I , I , I --I \\ , I I I I I I , I , , , "------~--------- I I I I I ~ - - - - - J-'" - ... - - ... -,'" _ ... I I New: ~.... York: ). C - ",,_ Ity.,~ o km 100 I I...

Casebourne, Joanna Jane

2002-02-12T23:59:59.000Z

22

ENERGY STAR in action | ENERGY STAR  

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

Benchmark energy use ENERGY STAR in action Programs and policies using ENERGY STAR Green buildings and ENERGY STAR Communicate and educate Find out who's partnered with...

23

ENERGY STAR  

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

the measurement and tracking of electricity, gas, and water data, through the use of the ENERGY STAR Portfolio Manager tool. Goals included completion rates for critical and...

24

ENERGY STAR  

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

and Other and Other Climate Protection Partnerships 2011 Annual Report CONTENTS Letter from the Administrator ............................................................................................................................................................................. 1 Executive Summary .............................................................................................................................................................................................. 2 Highlights of 2011 ......................................................................................................................................................................................... 4 ENERGY STAR Overview ......................................................................................................................................................................................

25

NIST Stars  

Science Conference Proceedings (OSTI)

... Weather and climate research satellites could use SI Stars for on orbit calibration of their spectroradiometers and astronomers ... Facilities/Tools Used ...

2012-11-16T23:59:59.000Z

26

ENERGY STAR  

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

such as: Choosing ENERGY STAR certified appliances and electronics. Maintaining home heating and cooling systems to improve efficiency. Ensuring homes are well sealed...

27

ENERGY STAR  

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

STAR certified buildings > photo of a room in the W Hotel, San Francisco, CA W HOTEL, San Francisco, Calif. In 2007, hotel employees submitted a petition asking management to...

28

Earn recognition | ENERGY STAR  

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

ENERGY STAR Partner of the Year Award ENERGY STAR plant certification ENERGY STAR Challenge for Industry Success stories: Industrial energy management Market impacts: Improvements...

29

ENERGY STAR  

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

Protection Agency program helping businesses and individuals fight global warming through superior energy efficiency. Bring Your Green to Work with ENERGY STAR ® 1 Give It a rest Use the ENERGY STAR power management settings on your computer and monitor so they go into power save mode when not in use. Also use a power strip as a central "turn off" point when you are using equipment to completely disconnect the power supply. 2 Unplug It Unplug electronics such as cell phones and laptops once they are charged. Adapters plugged into outlets use energy even if they are not charging. 3 Light Up Your Work Life Replace the light bulb in your desk lamp with an ENERGY STAR qualified bulb. It will last up to 10 times longer and use about 75 percent less energy. Turn off the lights when

30

Chameleon stars  

Science Conference Proceedings (OSTI)

We consider a gravitating spherically symmetric configuration consisting of a scalar field nonminimally coupled to ordinary matter in the form of a perfect fluid. For this system we find static, regular, asymptotically flat solutions for both relativistic and nonrelativistic cases. It is shown that the presence of the nonminimal interaction leads to substantial changes both in the radial matter distribution of the star and in the star's total mass. A simple stability test indicates that, for the choice of parameters used in the paper, the solutions are unstable.

Dzhunushaliev, Vladimir [Institute for Basic Research, Eurasian National University, Astana, 010008 (Kazakhstan); Institute of Physicotechnical Problems and Material Science of the NAS of the Kyrgyz Republic, 265 a, Chui Street, Bishkek, 720071 (Kyrgyzstan); Folomeev, Vladimir [Institute of Physicotechnical Problems and Material Science of the NAS of the Kyrgyz Republic, 265 a, Chui Street, Bishkek, 720071 (Kyrgyzstan); Singleton, Douglas [Institute for Basic Research, Eurasian National University, Astana, 010008 (Kazakhstan); Physics Department, CSU Fresno, Fresno, California 93740-8031 (United States)

2011-10-15T23:59:59.000Z

31

ENERGY STAR Challenge for Industry | ENERGY STAR  

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

ENERGY STAR plant certification ENERGY STAR Challenge for Industry See who has taken the Challenge See who has achieved the Challenge See who is promoting the Challenge ENERGY...

32

ENERGY STAR  

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

of Air and Radiation * For more information www.energystar.gov or call 1.888.STAR.YES (1.888.782.7937) * (6202J) EPA 430-H-08-002 * December 2008 * Recycled/Recyclable - Printed with Vegetable Oil Based Inks on Recycled Paper (Minimum 50% Post-consumer Content) of Air and Radiation * For more information www.energystar.gov or call 1.888.STAR.YES (1.888.782.7937) * (6202J) EPA 430-H-08-002 * December 2008 * Recycled/Recyclable - Printed with Vegetable Oil Based Inks on Recycled Paper (Minimum 50% Post-consumer Content) Enable power management settings so they automatically enter a low-power mode when not in use. monitor/computer Use a power strip as a central "turn off" point when you are done using office equipment to completely disconnect the power supply. power strip Unplug electronics

33

RHIC | STAR Detector  

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

The STAR Detector The STAR detector specializes in tracking the thousands of particles produced by each ion collision at RHIC. Weighing 1,200 tons and as large as a house, STAR is...

34

Home : ENERGY STAR  

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

STAR logo Skip directly to page content Energy Efficient Products Energy Efficient Products ENERGY STAR products are independently certified to save energy without sacrificing...

35

ENERGY STAR Challenge  

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

STAR Challenge for Industry Participant Handbook June 2013 ENERGY STAR is a U.S. Environmental Protection Agency Program helping organizations and individuals fight climate change...

36

Participation Form | ENERGY STAR  

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

application. Select the ENERGY STAR program you intend to participate in, and choose your primary contacts. Return this form to ENERGY STAR for consideration as a partner....

37

ENERGY STAR Certified New Homes : ENERGY STAR  

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

little label with a big message. Better is better. The blue ENERGY STAR label on a new home means: Peace of Mind Enduring Quality Wall-to-Wall Comfort Proven Value ENERGY STAR...

38

ENERGY STAR plant certification | ENERGY STAR  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

39

ENERGY STAR Congregations Handout | ENERGY STAR  

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

handout to learn a summary of ENERGY STAR offerings for congregations, quick tips for saving energy in religious worship facilities, and how to sign up for the ENERGY STAR...

40

ENERGY STAR industrial partnership | ENERGY STAR  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

Note: This page contains sample records for the topic "waha lone star" 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

ENERGY STAR communications toolkit | ENERGY STAR  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

42

The value of ENERGY STAR | ENERGY STAR  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

43

ENERGY STAR Challenge for Industry | ENERGY STAR  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

44

ENERGY STAR for existing buildings | ENERGY STAR  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

45

ENERGY STAR  

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

New Energy Technology 2754 Compass Drive, Grand Junction, CO 81506 Business: Energy Management Services/Consulting Sarah Faverman Phone: 970-243-0255 / Fax: 970-245-4268 Email: sarah@newenergytech.net Customer JCPenney Company, Inc. 6501 Legacy Drive, Plano, TX 75024 Business: Retail Rob Keller, P.E., Energy Management & Engineering Services Director Phone: 972-431-1788 / Fax: 972-531-1788 Email: rkeller@jcpenney.com New Energy Technology helped JCPenney earn the first ENERGY STAR labels for retail buildings and Partner of the Year Award. Project Scope New Energy Technology (NET) supports JCPenney's (JCP) energy conservation culture through three programs focused on high-quality energy data and energy management. Through its automated benchmarking

46

ENERGY STAR  

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

Green Team Checklist Green Team Checklist One person cannot do it all! So when it comes to making your workplace greener and more energy efficient, nothing beats a team. The Environmental Protection Agency (EPA) has learned from ENERGY STAR partners that forming a green team with coworkers is a great way to help increase energy efficiency and reduce office waste. Consider the following checklist of creative ideas from EPA to help your green team get started. Once you've formed your team, start by planting the seeds for success with small changes in individual workspaces. Then move through the list and help success bloom with bigger changes that can affect the whole organization. Together, these actions can help your green team build a better world! Start Off Right-Meet with management to get approval and buy-in for the idea of forming a green team. Not only does support

47

2014 ENERGY STAR Awards : ENERGY STAR  

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

Partner Resources Partner Resources Manufacturers Retailers New Home Industry Utilities/EEPS Residential & Commercial Products Programs Service & Product Providers Buildings & Plants Small Businesses Congregations For Contractors For Federal Agencies Join ENERGY STAR Home > Partner Resources > ENERGY STAR Awards 2014 ENERGY STAR Awards The application submission period for the 2014 ENERGY STAR Awards has closed. Each year, the ENERGY STAR program honors organizations that have made outstanding contributions to protecting the environment through energy efficiency. Please save the date for our awards ceremony on April 29, 2014. Ceremony registration information will be available on this website in January 2014. If you have any questions, please contact Rebecca Hudson, at

48

Building Technologies Program: ENERGY STAR  

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

ENERGY STAR on Twitter Bookmark Building Technologies Program: ENERGY STAR on Google Bookmark Building Technologies Program: ENERGY STAR on Delicious Rank Building...

49

Building Technologies Office: ENERGY STAR  

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

ENERGY STAR on Twitter Bookmark Building Technologies Office: ENERGY STAR on Google Bookmark Building Technologies Office: ENERGY STAR on Delicious Rank Building...

50

STAR Test Environment  

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

STAR Test Environment STAR Test Environment STAR Test Environment These instructions describe how to set up the STAR environment independent of the production environment in order to test different installations in $OPTSTAR and $GROUP_DIR. If you want to modify those installations you will need access to the starofl account. Bypass STAR envionment login Edit your ~/.pdsf_setup file changing the STAR_LINUX_SETUP to "use_none" and start a new session. You should not see all the STAR environmental variables defined when you do this (and it will probably be much quicker than usual, too). Do a manual STAR login If you want to modify what test environment you use copy the test login scripts to your own working area: cp -r /common/star/startest /path/to/myworkdir/. If you don't want to modify these files you can source them directly from

51

Become an ENERGY STAR partner | ENERGY STAR  

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Become an ENERGY STAR partner Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction...

52

Earn ENERGY STAR certification | ENERGY STAR  

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Earn ENERGY STAR certification Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction...

53

Sample ENERGY STAR performance documents | ENERGY STAR  

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Verify and document your savings Sample ENERGY STAR performance documents Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers...

54

Green buildings and ENERGY STAR | ENERGY STAR  

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Green buildings and ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction...

55

ENERGY STAR Building Upgrade Manual | ENERGY STAR  

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ENERGY STAR Building Upgrade Manual Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new...

56

ENERGY STAR for small business | ENERGY STAR  

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STAR, you can improve your small business's financial performance by reducing energy waste and energy costs, while protecting the environment. Join the network When you join...

57

NVLAP Recognized by ENERGY STAR  

Science Conference Proceedings (OSTI)

NVLAP Recognized by ENERGY STAR. For ... criteria. Details of the program can be found on the ENERGY STAR website. ...

2012-05-08T23:59:59.000Z

58

Competitor resources | ENERGY STAR  

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Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

59

Federal agencies | ENERGY STAR  

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Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

60

ENERGY STAR Challenge  

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

STAR Challenge STAR Challenge for Industry Participant Handbook June 2013 ENERGY STAR is a U.S. Environmental Protection Agency Program helping organizations and individuals fight climate change through superior energy efficiency. Learn more at energystar.gov/buildings. 2 Contents Overview ............................................................................................................................. 3 Participation Eligibility .......................................................................................................... 4 How to Participate ............................................................................................................... 5 Step 1: Establish an energy intensity metric ................................................................ 5

Note: This page contains sample records for the topic "waha lone star" 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

Cushman & Wakefield Environmental Challenge | ENERGY STAR  

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

STAR in action Communicate and educate ENERGY STAR communications toolkit Bring Your Green to Work with ENERGY STAR Motivate with a competition ENERGY STAR National Building...

62

ENERGY STAR Challenge for Architects | ENERGY STAR  

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

Race to Denver 2012 Race to DC 2011 Race to New Orleans 2010 Race to Miami 2009 Race to San Francisco 2008 Race to Boston 2007 Race to San Antonio ENERGY STAR Challenge for...

63

star-shaped polygon  

Science Conference Proceedings (OSTI)

NIST. star-shaped polygon. (definition). Definition: A polygon P in which there exists an interior point p such that all the boundary ...

2013-05-08T23:59:59.000Z

64

Energy Star Portfolio Manager  

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

May 2013 What's New in Portfolio Manager ? EPA's ENERGY STAR Portfolio Manager tool helps you measure and track energy use, water use, and greenhouse gas emissions of your...

65

Press room | ENERGY STAR  

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

improve their efficiency, and earn recognition. Learn more about the program Facts and statistics See who's partnered with ENERGY STAR Find certified buildings and plants...

66

Energy guides | ENERGY STAR  

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

track, and benchmark Improve energy performance ENERGY STAR industrial partnership Energy guides Energy efficiency and air regulation Plant energy auditing Industrial...

67

A Star on Earth  

Science Conference Proceedings (OSTI)

Jun 2, 2009 ... The world's highest-energy laser system, capable of creating temperatures and pressures that now only exist in the cores of stars, was unveiled...

68

Ten reasons to pursue ENERGY STAR certification | ENERGY STAR...  

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

substantial. For example, ENERGY STAR certified office buildings cost 0.50 less per square foot to operate than their peers. Currently, ENERGY STAR certified buildings are...

69

ENERGY STAR certification | ENERGY STAR Buildings & Plants  

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

ENERGY STAR certification ENERGY STAR certification Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Find out who's partnered with ENERGY STAR Become an ENERGY STAR partner Find ENERGY STAR certified buildings and plants ENERGY STAR certification Featured research and reports Facts and stats Climate change and buildings ENERGY STAR certification

70

EPA's ENERGY STAR National Building Competition | ENERGY STAR  

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

ENERGY STAR communications toolkit Motivate with a competition EPA's ENERGY STAR National Building Competition Secondary menu About us Press room Contact Us Portfolio...

71

ENERGY STAR Partner of the Year Award | ENERGY STAR  

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

Partner of the Year profiles in leadership ENERGY STAR plant certification ENERGY STAR Challenge for Industry Success stories: Industrial energy management Market impacts:...

72

Join ENERGY STAR as a partner | ENERGY STAR  

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

we help you? Build an energy program Improve building and plant performance Earn the ENERGY STAR and other recognition Benchmark energy use ENERGY STAR in action Communicate and...

73

EPA's ENERGY STAR National Building Competition | ENERGY STAR  

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

How can we help you? Communicate and educate ENERGY STAR communications toolkit Motivate with a competition EPA's ENERGY STAR National Building Competition...

74

The value of ENERGY STAR certification | ENERGY STAR  

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

building as ENERGY STAR. Below is a summary of several studies that evaluated the added market value of ENERGY STAR certified buildings. Chart showing price advantages of ENERGY...

75

ENERGY STAR Homes in the News : ENERGY STAR  

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

ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR products are...

76

STAR METRICS | Department of Energy  

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

STAR METRICS STAR METRICS May 4, 2011 - 4:47pm Addthis Energy continues to define Phase II of the STAR METRICS program, a collaborative initiative to track Research and Development...

77

ENERGY STAR Score for Offices  

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

July 2013 ENERGY STAR Score for Offices in the United States Page 1 ENERGY STAR Score for Offices in the United States Technical Reference OVERVIEW The ENERGY STAR Score for...

78

Commercial new construction | ENERGY STAR  

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

6: Complete the ENERGY STAR lifecycle See projects that have been Designed to Earn the ENERGY STAR 1 World Green Building Trends: Business Benefits Driving New and Retrofit...

79

Star Biomass | Open Energy Information  

Open Energy Info (EERE)

Biomass Jump to: navigation, search Name Star Biomass Place India Sector Biomass Product Plans to set up biomass projects in Rajasthan. References Star Biomass1 LinkedIn...

80

ENERGY STAR Score for Hospitals  

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

Hospitals in the United States Page 1 ENERGY STAR Score for Hospitals in the United States Technical Reference OVERVIEW The ENERGY STAR Score for Hospitals applies to general...

Note: This page contains sample records for the topic "waha lone star" 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

Home : ENERGY STAR  

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

Who dared imagine? Who dared imagine? Our newest video celebrates 20 years of success with our innovative ENERGY STAR partners. See the Video EPA Logo ENERGY STAR is a U.S. Environmental Protection Agency voluntary program that helps businesses and individuals save money and protect our climate through superior energy efficiency. Learn more about ENERGY STAR. A comprehensive review of ENERGY STAR and other EPA climate protection partnerships. See 2011 Annual Report. Basic information on climate change, greenhouse gas emissions, and climate change science. See Climate Change. With help from ENERGY STAR, by 2012, Americans had cumulatively prevented more than 1.8 billion metric tons of GHG emissions. See 2012 Achievements. Energy Efficiency For Your Home

82

Protoneutron Star Winds  

E-Print Network (OSTI)

Neutrino-driven winds are thought to accompany the Kelvin-Helmholtz cooling phase of nascent protoneutron stars in the first seconds after a core-collapse supernova. These outflows are a likely candidate as the astrophysical site for rapid neutron-capture nucleosynthesis (the r-process). In this chapter we review the physics of protoneutron star winds and assess their potential as a site for the production of the heavy r-process nuclides. We show that spherical transonic protoneutron star winds do not produce robust $r$-process nucleosynthesis for `canonical' neutron stars with gravitational masses of 1.4 M_sun and coordinate radii of 10 km. We further speculate on and review some aspects of neutrino-driven winds from protoneutron stars with strong magnetic fields.

Todd A. Thompson

2003-09-03T23:59:59.000Z

83

Electrically charged compact stars  

E-Print Network (OSTI)

We review here the classical argument used to justify the electrical neutrality of stars and show that if the pressure and density of the matter and gravitational field inside the star are large, then a charge and a strong electric field can be present. For a neutron star with high pressure (~ 10^{33} to 10^{35} dynes /cm^2) and strong gravitational field (~ 10^{14} cm/s^2), these conditions are satisfied. The hydrostatic equation which arises from general relativity, is modified considerably to meet the requirements of the inclusion of the charge. In order to see any appreciable effect on the phenomenology of the neutron stars, the charge and the electrical fields have to be huge (~ 10^{21} Volts/cm). These stars are not however stable from the viewpoint that each charged particle is unbound to the uncharged particles, and thus the system collapses one step further to a charged black hole

Subharthi Ray; Manuel Malheiro; Jose' P. S. Lemos; Vilson T. Zanchin

2006-04-17T23:59:59.000Z

84

What is Energy Star? ENERGY STAR  

E-Print Network (OSTI)

What is Energy Star? ENERGY STAR® qualified products and practices help you save money and reduce greenhouse gas emissions by meeting strict energy efficiency guidelines set by the U.S. Environmental Protection Agency (EPA) and the U.S. Department of Energy. You can help reduce electricity usage and its

van Tiggelen, Bart

85

Leading organizations choose ENERGY STAR | ENERGY STAR Buildings & Plants  

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

Leading organizations choose ENERGY STAR Leading organizations choose ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Why design to earn ENERGY STAR Leading organizations choose ENERGY STAR Sell others on the idea of ENERGY STAR An overview of the ENERGY STAR lifecycle Design to earn ENERGY STAR Leading organizations choose ENERGY STAR Facebook's data center achieved Designed to Earn the ENERGY STAR More than

86

Hypernuclear Physics for Neutron Stars  

E-Print Network (OSTI)

The role of hypernuclear physics for the physics of neutron stars is delineated. Hypernuclear potentials in dense matter control the hyperon composition of dense neutron star matter. The three-body interactions of nucleons and hyperons determine the stiffness of the neutron star equation of state and thereby the maximum neutron star mass. Two-body hyperon-nucleon and hyperon-hyperon interactions give rise to hyperon pairing which exponentially suppresses cooling of neutron stars via the direct hyperon URCA processes. Non-mesonic weak reactions with hyperons in dense neutron star matter govern the gravitational wave emissions due to the r-mode instability of rotating neutron stars.

Jurgen Schaffner-Bielich

2008-01-24T23:59:59.000Z

87

Service providers | ENERGY STAR  

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

buildings and industrial plants. Photo of a man with a clipboard. Verify applications for ENERGY STAR certification Find how-to guides and training for individuals who sign off on...

88

ENERGY STAR industrial partnership | ENERGY STAR Buildings & Plants  

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

ENERGY STAR industrial partnership ENERGY STAR industrial partnership Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Get started with ENERGY STAR Make the business case Build an energy management program Measure, track, and benchmark Improve energy performance ENERGY STAR industrial partnership New ENERGY STAR industrial partners Energy guides Energy efficiency and air regulation

89

Use ENERGY STAR benchmarking tools | ENERGY STAR Buildings & Plants  

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

Use ENERGY STAR benchmarking tools Use ENERGY STAR benchmarking tools Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Build an energy program Improve building and plant performance Earn the ENERGY STAR and other recognition Benchmark energy use Learn about benchmarking Use ENERGY STAR benchmarking tools ENERGY STAR in action Communicate and educate

90

ENERGY STAR | Open Energy Information  

Open Energy Info (EERE)

ENERGY STAR ENERGY STAR Jump to: navigation, search Logo: ENERGY STAR Name ENERGY STAR Year founded 1992 Notes Partnered with more than 20,000 public sector organizations. Website https://www.energystar.gov/ind References About ENERGY STAR[1] LinkedIn Connections Contents 1 About ENERGY STAR 1.1 For the Home 1.2 For Business 1.3 References About ENERGY STAR ENERGY STAR is a joint program of the U.S. Environmental Protection Agency and the U.S. Department of Energy helping us all save money and protect the environment through energy efficient products and practices. Results are already adding up. Americans, with the help of ENERGY STAR, saved enough energy in 2010 alone to avoid greenhouse gas emissions equivalent to those from 33 million cars - all while saving nearly $18 billion on their

91

ENERGY STAR Focus on Energy Efficiency in Printing | ENERGY STAR  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

92

ENERGY STAR certification for your building | ENERGY STAR  

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

that your building can earn ENERGY STAR certification just like a refrigerator or light bulb? The mark of efficiency No matter where you see it, the ENERGY STAR label means the...

93

ENERGY STAR Small Business Network List | ENERGY STAR  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

94

ENERGY STAR Guidelines for Energy Management | ENERGY STAR  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

95

ENERGY STAR Partner of the Year Awards | ENERGY STAR  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

96

Earn the ENERGY STAR and other recognition | ENERGY STAR  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

97

ENERGY STAR portfolio-wide recognition | ENERGY STAR  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

98

ENERGY STAR Commercial Buildings College Course | ENERGY STAR  

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

and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program...

99

Making Carbon in Stars  

E-Print Network (OSTI)

The triple alpha process plays an important role in the production of 12C in stars. Its rate is known with an accuracy of about 12%. We examine the corresponding uncertainties introduced in the description of pre-supernova stars, of nucleosynthesis in a core-collapse SN explosion, and of the production of 12C during the third dredge-up in asymptotic giant branch (AGB) stars. For the AGB case we consider also the effects of uncertainties in the 14N(p,gamma)15O rate. We conclude that the present accuracy of the triplr alpha rate is inadequate and describe new experiments that will lead to a more accurate value.

Sam M. Austin

2004-11-30T23:59:59.000Z

100

Barron Electric Cooperative - Energy Star Appliance & Energy...  

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

Barron Electric Cooperative - Energy Star Appliance & Energy Efficient Lighting Rebate Program Barron Electric Cooperative - Energy Star Appliance & Energy Efficient Lighting...

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


101

ENERGY STAR Score for Hotels  

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

Hotels in the United States Page 1 ENERGY STAR Score for Hotels in the United States Technical Reference OVERVIEW The ENERGY STAR Score for Hotels applies to properties renting...

102

Learn the benefits | ENERGY STAR  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

103

About the battle | ENERGY STAR  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

104

High-gravity central stars  

E-Print Network (OSTI)

NLTE spectral analyses of high-gravity central stars by means of state-of-the-art model atmosphere techniques provide information about the precursor AGB stars. The hydrogen-deficient post-AGB stars allow investigations on the intershell matter which is apparently exhibited at the stellar surface. We summarize recent results from imaging, spectroscopy, and spectropolarimetry.

Thomas Rauch

2006-07-11T23:59:59.000Z

105

ENERGY STAR service and product provider training series | ENERGY STAR  

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

service and product provider training series service and product provider training series Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can ENERGY STAR help your business? Get started Join ENERGY STAR as a partner ENERGY STAR service & product provider training series Service and product provider's marketing toolkit ENERGY STAR sales tools for service and product providers

106

ENERGY STAR plant certification | ENERGY STAR Buildings & Plants  

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

» ENERGY STAR plant certification » ENERGY STAR plant certification Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Get started with ENERGY STAR Make the business case Build an energy management program Measure, track, and benchmark Improve energy performance Industrial service and product providers Earn recognition ENERGY STAR Partner of the Year Award

107

Campaigns and incentive programs that incorporate ENERGY STAR | ENERGY STAR  

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

Campaigns and incentive programs that incorporate ENERGY STAR Campaigns and incentive programs that incorporate ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Policies that specify the use of ENERGY STAR tools Campaigns and incentive programs that incorporate ENERGY STAR Lead by example Gather support Develop programs and policies Host a competition Use financing vehicles

108

About ENERGY STAR for commercial and industrial buildings | ENERGY STAR  

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

ENERGY STAR for commercial and industrial buildings ENERGY STAR for commercial and industrial buildings Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Find out who's partnered with ENERGY STAR Become an ENERGY STAR partner Find ENERGY STAR certified buildings and plants ENERGY STAR certification Featured research and reports Facts and stats Climate change and buildings

109

Earn ENERGY STAR certification | ENERGY STAR Buildings & Plants  

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

Earn ENERGY STAR certification Earn ENERGY STAR certification Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Build an energy program Improve building and plant performance Earn the ENERGY STAR and other recognition Benchmark energy use ENERGY STAR in action Communicate and educate ENERGY STAR communications toolkit Bring Your Green to Work with ENERGY STAR

110

Leading firms choose ENERGY STAR | ENERGY STAR Buildings & Plants  

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

Leading firms choose ENERGY STAR Leading firms choose ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Why you should design to earn the ENERGY STAR Leading firms choose ENERGY STAR Why new doesn't always mean efficient Follow EPA's step-by-step process ENERGY STAR Challenge for Architects Leading firms choose ENERGY STAR Facebook data center Hundreds of leading A/E firms have already partnered

111

Window To The Stars  

E-Print Network (OSTI)

We present Window To The Stars, a graphical user interface to the popular TWIN single/binary stellar evolution code, for novices, students and professional astrophysicists. It removes the drudgery associated with the traditional approach to running the code, while maintaining the power, output quality and flexibility a modern stellar evolutionist requires. It is currently being used for cutting edge research and interactive teaching.

Robert G. Izzard; Evert Glebbeek

2006-07-27T23:59:59.000Z

112

Halo Star Evolution  

E-Print Network (OSTI)

In this review, I will discuss a few problems which point to the need for improved stellar evolution models of halo stars. Current stellar evolution models do not match the observed $^7$Li abundance patterns, suggesting that the input physics and/or the assumptions used in constructing the models are in need of revision. It appears that all halo stars have suffered some $^7$Li depletion, implying that the primordial $^7$Li abundance is higher than that presently observed in hot halo stars. Observations of abundances of various elements in globular cluster giant branch stars have suggested for some time now that some form of deep mixing, which is not present in theoretical models, occurs in halo stars. The driving mechanism for this mixing, and its incorporation into stellar models remain one of the key problems in stellar modeling. Current theoretical isochrones are able to provide a good match to observed colour-magnitude diagrams. However, there is some evidence that the theoretical luminosity functions are in disagreement with observations. This is an area which requires further study, as it suggests that the relative main sequence/giant branch lifetimes predicted by the models are incorrect. A discussion of some of the uncertainties involved in determining the ages of globular clusters is presented. The absolute ages of globular clusters provide a lower bound to the age of the universe, and so are of great interest to cosmologists. Unfortunately, present uncertainties in stellar models lead to a rather large range in the inferred ages of globular clusters of 11 -- 18 Gyr.

Brian Chaboyer

1995-09-08T23:59:59.000Z

113

Cerenkov radiation and scalar stars  

E-Print Network (OSTI)

We explore the possibility that a charged particle moving in the gravitational field generated by a scalar star could radiate energy via a recently proposed gravitational \\v{C}erenkov mechanism. We numerically prove that this is not possible for stable boson stars. We also show that soliton stars could have \\v{C}erenkov radiation for particular values of the boson mass, although diluteness of the star grows and actual observational possibility decreases for the more usually discussed boson masses. These conclusions diminish, although do not completely rule out, the observational possibility of actually detecting scalar stars using this mechanism, and lead us to consider other forms, like gravitational lensing.

S. Capozziello; G. Lambiase; Diego F. Torres

2000-06-23T23:59:59.000Z

114

Energy Star | Open Energy Information  

Open Energy Info (EERE)

Star Star Jump to: navigation, search Energystarlogo.jpg Contents 1 What's new 2 About ENERGY STAR 3 For the Home 4 For Business 5 History 6 References What's new On March 15, 2012, the EPA released a press release announcing 2012's ENERGY STAR award winners, and celebrating the 20 year anniversary of the award. Overall, the EPA estimates that American's have saved nearly $230 billion over two decades of the award. About ENERGY STAR ENERGY STAR is a joint program of the United States Environmental Protection Agency and the United States Department of Energy helping us all save money and protect the environment through energy efficient products and practices. Results are already adding up. Americans, with the help of ENERGY STAR, saved enough energy in 2009 alone to avoid greenhouse gas emissions

115

Detector limitations, STAR  

Science Conference Proceedings (OSTI)

Every detector has limitations in terms of solid angle, particular technologies chosen, cracks due to mechanical structure, etc. If all of the presently planned parts of STAR [Solenoidal Tracker At RHIC] were in place, these factors would not seriously limit our ability to exploit the spin physics possible in RHIC. What is of greater concern at the moment is the construction schedule for components such as the Electromagnetic Calorimeters, and the limited funding for various levels of triggers.

Underwood, D. G.

1998-07-13T23:59:59.000Z

116

Stable dark energy stars  

E-Print Network (OSTI)

The gravastar picture is an alternative model to the concept of a black hole, where there is an effective phase transition at or near where the event horizon is expected to form, and the interior is replaced by a de Sitter condensate. In this work, a generalization of the gravastar picture is explored, by considering a matching of an interior solution governed by the dark energy equation of state, $\\omega\\equiv p/ \\rhosolution at a junction interface. The motivation for implementing this generalization arises from the fact that recent observations have confirmed an accelerated cosmic expansion, for which dark energy is a possible candidate. Several relativistic dark energy stellar configurations are analyzed by imposing specific choices for the mass function. The first case considered is that of a constant energy density, and the second choice, that of a monotonic decreasing energy density in the star's interior. The dynamical stability of the transition layer of these dark energy stars to linearized spherically symmetric radial perturbations about static equilibrium solutions is also explored. It is found that large stability regions exist that are sufficiently close to where the event horizon is expected to form, so that it would be difficult to distinguish the exterior geometry of the dark energy stars, analyzed in this work, from an astrophysical black hole.

Francisco S. N. Lobo

2005-08-28T23:59:59.000Z

117

Find an ENERGY STAR service and product provider | ENERGY STAR  

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Find an ENERGY STAR service and product provider Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial...

118

Win ENERGY STAR Partner of the Year | ENERGY STAR  

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Win ENERGY STAR Partner of the Year Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new...

119

EPA's ENERGY STAR National Building Competition | ENERGY STAR  

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ENERGY STAR National Building Competition Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new...

120

How can ENERGY STAR help your business? | ENERGY STAR  

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ENERGY STAR help your business? Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction...

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to obtain the most current and comprehensive results.


121

Bring Your Green to Work with ENERGY STAR | ENERGY STAR  

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Bring Your Green to Work with ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new...

122

Join the ENERGY STAR Small Business Network | ENERGY STAR  

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Join the ENERGY STAR Small Business Network Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new...

123

Celebrating a Decade of ENERGY STAR Buildings | ENERGY STAR  

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Celebrating a Decade of ENERGY STAR Buildings Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new...

124

Verify applications for ENERGY STAR certification | ENERGY STAR  

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Verify applications for ENERGY STAR certification Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial...

125

ENERGY STAR Success Story: HEI Hotels & Resorts | ENERGY STAR  

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Story: HEI Hotels & Resorts HEI Hotels & Resorts is a growing hospitality company with 30 hotel properties in 13 states. Since launching its partnership with ENERGY STAR in 2006,...

126

ENERGY STAR SNAPSHOT - Spring 2009  

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0 0 Snapshot data runs through June 30, 2010. Summary By mid-year 2010, commercial and industrial organizations have almost exceeded activity levels reached throughout all of 2009. From January through June 30, 2010: More than 80,000 buildings have benchmarked their energy usage with ENERGY STAR, of which 63,000 buildings received an ENERGY STAR energy performance score-nearly equivalent to the amount for all of 2009. Close to 3,200 buildings earned the ENERGY STAR label-the highest amount earned through two quarters of any year, and 80% higher than mid-year 2009. The ENERGY STAR Snapshot provides an at-a-glance summary of the latest national ENERGY STAR metrics to help you, our partners, see the impact of your efforts. The ENERGY STAR Snapshot is

127

ENERGY STAR EEPS Partnership Agreement  

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Approval expires 02/29/2016 1 EPA Form No. 5900-33 ENERGY STAR Partnership Agreement Instructions for Partnering with ENERGY STAR ® As an Energy Efficiency Program Sponsor Organizations interested in partnering with ENERGY STAR as an Energy Efficiency Program Sponsor should take the following steps: 1. Review the Energy Efficiency Program Sponsors Program Definitions and Program Requirements documents. 2. Select the area(s) of interest for a new partnership on the Participation Form. Please

128

Snapshot (Spring 2012) | ENERGY STAR  

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resources Small business resources State and local government resources Snapshot (Spring 2012) The ENERGY STAR Snapshot provides an at-a-glance summary of the key performance...

129

Building Technologies Program: ENERGY STAR  

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with ENERGY STAR DOE conducts research, development, and deployment to improve the energy efficiency of existing homes using a whole-building approach, which results in the...

130

A Mosque Among the Stars  

E-Print Network (OSTI)

A Mosque Among The Stars was the first anthology that dealt with the subject of Muslim characters and/or Islamic themes and Science Fiction.

Ahmad, Muhammad Aurangzeb; Khan, Ahmad

2007-01-04T23:59:59.000Z

131

Snapshot (Fall 2009) | ENERGY STAR  

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to help ENERGY STAR partners see the impact of their efforts. It provides a look at: Trends in the energy performance rating of commercial and institutional buildings...

132

Snapshot (Spring 2009) | ENERGY STAR  

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to help ENERGY STAR partners see the impact of their efforts. It provides a look at: Trends in the energy performance rating of commercial and institutional buildings...

133

Snapshot (Fall 2008) | ENERGY STAR  

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to help ENERGY STAR partners see the impact of their efforts. It provides a look at: Trends in the energy performance rating of commercial and institutional buildings...

134

Snapshot (Spring 2008) | ENERGY STAR  

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to help ENERGY STAR partners see the impact of their efforts. It provides a look at: Trends in the energy performance rating of commercial and institutional buildings...

135

Industries in focus | ENERGY STAR  

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ENERGY STAR Energy Performance Indicators for plants Industries in focus Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers...

136

Plant energy auditing | ENERGY STAR  

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track, and benchmark Improve energy performance ENERGY STAR industrial partnership Energy guides Energy efficiency and air regulation Plant energy auditing Industrial...

137

Improve energy performance | ENERGY STAR  

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track, and benchmark Improve energy performance ENERGY STAR industrial partnership Energy guides Energy efficiency and air regulation Plant energy auditing Industrial...

138

ENERGY STAR Petroleum Energy Guide  

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183 ERNEST ORLANDO LAWRENCE BERKELEY NATIONAL LABORATORY Energy Efficiency Improvement and Cost Saving Opportunities For Petroleum Refineries An ENERGY STAR Guide for Energy and...

139

Energy Star Building Upgrade Manual  

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program helping businesses and individuals fight global warming through superior energy efficiency. ENERGY STAR Building Upgrade Manual United States Environmental Protection...

140

Portable Data loggers | ENERGY STAR  

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short list of companies that sell the products. Download more information about Portable Data Loggers here. Energy Efficient Products Learn about ENERGY STAR Products Save Energy...

Note: This page contains sample records for the topic "waha lone star" 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

Star Products for Relativistic Quantum Mechanics  

E-Print Network (OSTI)

The star product formalism has proved to be an alternative formulation for nonrelativistic quantum mechanics. We want introduce here a covariant star product in order to extend the star product formalism to relativistic quantum mechanics in the proper time formulation.

P. Henselder

2007-05-24T23:59:59.000Z

142

ENERGY STAR Score for Medical Offices  

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

July 2013 ENERGY STAR Score for Medical Offices in the United States Page 1 ENERGY STAR Score for Medical Offices in the United States Technical Reference OVERVIEW The ENERGY STAR...

143

TRIGGERED STAR FORMATION SURROUNDING WOLF-RAYET STAR HD 211853  

SciTech Connect

The environment surrounding Wolf-Rayet (W-R) star HD 211853 is studied in molecular, infrared, as well as radio, and H I emission. The molecular ring consists of well-separated cores, which have a volume density of 10{sup 3} cm{sup -3} and kinematic temperature {approx}20 K. Most of the cores are under gravitational collapse due to external pressure from the surrounding ionized gas. From the spectral energy distribution modeling toward the young stellar objects, the sequential star formation is revealed on a large scale in space spreading from the W-R star to the molecular ring. A small-scale sequential star formation is revealed toward core 'A', which harbors a very young star cluster. Triggered star formations are thus suggested. The presence of the photodissociation region, the fragmentation of the molecular ring, the collapse of the cores, and the large-scale sequential star formation indicate that the 'collect and collapse' process functions in this region. The star-forming activities in core 'A' seem to be affected by the 'radiation-driven implosion' process.

Liu Tie; Wu Yuefang; Zhang Huawei [Department of Astronomy, Peking University, 100871 Beijing (China); Qin Shengli, E-mail: liutiepku@gmail.com [I. Physikalisches Institut, Universitaet zu Koeln, Zuelpicher Str. 77, 50937 Koeln (Germany)

2012-05-20T23:59:59.000Z

144

Reading Municipal Light Department - Residential ENERGY STAR...  

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

Residential ENERGY STAR Appliance Rebate Program Reading Municipal Light Department - Residential ENERGY STAR Appliance Rebate Program Eligibility Residential Savings For Heating &...

145

ENERGY STAR Score for Medical Offices  

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

Medical Offices in the United States Page 1 ENERGY STAR Score for Medical Offices in the United States Technical Reference OVERVIEW The ENERGY STAR Score for Medical Offices...

146

Physics of Neutron Star Crusts  

E-Print Network (OSTI)

The physics of neutron star crusts is vast, involving many different research fields, from nuclear and condensed matter physics to general relativity. This review summarizes the progress, which has been achieved over the last few years, in modeling neutron star crusts, both at the microscopic and macroscopic levels. The confrontation of these theoretical models with observations is also briefly discussed.

N. Chamel; P. Haensel

2008-12-20T23:59:59.000Z

147

ENERGY STAR Snapshot Spring 2012  

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

Spring 2012 Spring 2012 Snapshot data runs through December 31, 2011. The ENERGY STAR Snapshot provides an at-a-glance summary of the latest national ENERGY STAR metrics to help you, our partners, see the impact of your efforts. The ENERGY STAR Snapshot is distributed twice a year and provides: * Trends in energy benchmarking of commercial and industrial buildings. * State-by-state activity along with activity for the top Designated Market Areas. * Industrial sector participation in ENERGY STAR. * Trends in ENERGY STAR certified commercial and industrial facilities. Summary By the end of calendar year 2011, commercial and industrial organizations exceeded figures for benchmarking and certification that were achieved in 2010. Since June, 2011:

148

Quadrupole moments of rotating neutron stars and strange stars  

E-Print Network (OSTI)

We present results for models of neutron stars and strange stars constructed using the Hartle-Thorne slow-rotation method with a wide range of equations of state, focusing on the values obtained for the angular momentum $J$ and the quadrupole moment $Q$, when the gravitational mass $M$ and the rotational frequency $\\Omega$ are specified. Building on previous work, which showed surprising uniformity in the behaviour of the moment of inertia for neutron-star models constructed with widely-different equations of state, we find similar uniformity for the quadrupole moment. These two quantities, together with the mass, are fundamental for determining the vacuum space-time outside neutron stars. We study particularly the dimensionless combination of parameters $QM/J^2$ (using units for which $c=G=1$). This quantity goes to 1 in the case of a Kerr-metric black hole and deviations away from 1 then characterize the difference between neutron-star and black-hole space-times. It is found that $QM/J^2$ for both neutron stars and strange stars decreases with increasing mass, for a given equation of state, reaching a value of around 2 (or even less) for maximum-mass models, meaning that their external space-time is then rather well approximated by the Kerr metric. If $QM/J^2$ is plotter against compactness $R/2M$ (where $R$ is the radius), it is found that the relationship is nearly unique for neutron-star models, independent of the equation of state, while it is significantly different for strange stars. This gives a new way of possibly distinguishing between them.

Martin Urbanec; John C. Miller; Zdenek Stuchlik

2013-01-24T23:59:59.000Z

149

ENERGY STAR certification for your building | ENERGY STAR Buildings &  

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certification for your building certification for your building Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Learn the benefits Get started Use Portfolio Manager Save energy Find financing Earn recognition 20-percent recognition ENERGY STAR certification How to apply for ENERGY STAR certification Tips for low-cost verifications Submit a profile of your building

150

ENERGY STAR Building Upgrade Manual | ENERGY STAR Buildings & Plants  

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ENERGY STAR Building Upgrade Manual ENERGY STAR Building Upgrade Manual Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Learn the benefits Get started Use Portfolio Manager Save energy Stamp out energy waste Find cost-effective investments Engage occupants Purchase energy-saving products Put computers to sleep Get help from an expert Take a comprehensive approach

151

Portfolio Manager Technical Reference: ENERGY STAR Score | ENERGY STAR  

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ENERGY STAR Score ENERGY STAR Score Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In This Section Campaigns Commercial building design Communications resources Energy management guidance Financial resources Portfolio Manager Products and purchasing Recognition Research and reports Service and product provider (SPP) resources Success stories Target Finder Technical documentation

152

Sample ENERGY STAR performance documents | ENERGY STAR Buildings & Plants  

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Existing buildings Existing buildings » Use Portfolio Manager » Verify and document your savings » Sample ENERGY STAR performance documents Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Learn the benefits Get started Use Portfolio Manager The new ENERGY STAR Portfolio Manager How Portfolio Manager helps you save The benchmarking starter kit

153

ENERGY STAR Focus on Energy Efficiency in Metalcasting | ENERGY STAR  

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Metalcasting Metalcasting Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Get started with ENERGY STAR Make the business case Build an energy management program Measure, track, and benchmark Tools for benchmarking energy management practices Tools for tracking and benchmarking facility energy performance ENERGY STAR Energy Performance Indicators for plants

154

Who else is partnered with ENERGY STAR? | ENERGY STAR Buildings...  

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Hospital logo Increased its average ENERGY STAR score by 12 points over 2010 TIAA-CREF logo Achieved its 2012 goal of a 15% portfolio-wide energy reduction Transwestern...

155

The ENERGY STAR Guidelines for Energy Management | ENERGY STAR  

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a star. Your guide to building a strategic energy management program So you want to start saving energy, but you don't know where to begin. Or perhaps you've been managing energy...

156

ENERGY STAR Update: ENERGY STAR Low Carbon IT Campaign Kicks...  

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Carbon IT Campaign Kicks Off 2013 with Organizations Pledging to Power Manage 360,000 Computers The ENERGY STAR Low Carbon IT (LCIT) Campaign, a nationwide effort to assist and...

157

ENERGY STAR Challenge for Industry  

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Industrial Plant Industrial Plant Certification Professional Engineers' Guide for Validating Statements of Energy Performance Office of Air and Radiation Climate Protection Partnerships Division June 2013 ii Introduction The U.S. Environmental Protection Agency's ENERGY STAR program provides guidance, tools, and recognition to help companies improve the energy performance of their facilities and strengthen the effectiveness of their energy management program. Through ENERGY STAR, the U.S. Environmental Protection Agency (EPA) offers a number of forms of recognition, including certification for facility energy efficiency. ENERGY STAR certification for industrial plants recognizes individual manufacturing plants whose

158

ENERGY STAR Newsletter: Fall 2009  

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in LOCATION> for a 40-minute brown bag session to find out how we can save energy, save money, and fight climate change when we "bring our green to work." ENERGY STAR, the U.S....

159

Shooting Star | Open Energy Information  

Open Energy Info (EERE)

Shooting Star Shooting Star Jump to: navigation, search Name Shooting Star Facility Shooting Star Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Exelon Wind Developer Infinity Wind Power Energy Purchaser Sunflower Electric Power Corporation Location Greensburg KS Coordinates 37.55019151°, -99.27585125° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":37.55019151,"lon":-99.27585125,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

160

ENERGY STAR Challenge for Industry  

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

Challenge Challenge for Industry Professional Engineers' Guide for Validating Statements of Energy Improvement Office of Air and Radiation Climate Protection Partnerships Division May 2013 Revised ii Introduction The U.S. Environmental Protection Agency's (U.S. EPA) ENERGY STAR program provides guidance, tools, and recognition to help companies improve their energy performance. ENERGY STAR is a voluntary partnership program that companies choose to join. Through ENERGY STAR, U.S. EPA offers a number of forms of recognition for achievements in energy efficiency. The ENERGY STAR Challenge for Industry recognizes individual industrial sites for achieving a 10 percent reduction in energy intensity within 5 years from the conclusion of an established baseline. To be

Note: This page contains sample records for the topic "waha lone star" 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

Appendix 5 - STARS Architectual Overview  

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

Last saved by Coombs Page 1 7/27/2012 Last saved by Coombs Page 1 7/27/2012 Draft Appendix 5 - STARS Architectural Overview ARC101 - Architectural Overview for Department of Energy iManage Program - STARS Project Deliverable ID: IT0013 Version number: 1.09 Draft/Final as of: 18 Oct 2005 Printed on: 27 Jul 2012 Author: Richard Popovich, STARS System Architect Richard.Popovich@hq.doe.gov (301) 903-2223 Owner: Laura Kramer, STARS Project Manager Status of Document Draft Delivered Accepted Last saved by Coombs Page 2 7/27/2012 Draft Document information Document source This document is maintained as an online document. Contact the author for the latest version. Revision history Version number Date Summary of changes Revised By 1.01 08 Jul 03 Version 1 Richard Popovich,

162

Make a commitment | ENERGY STAR  

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

my money go? Set and Save with ENERGY STAR Product Finder Rebate Finder Store Locator Energy Savings At Home Energy Savings At Home Improving your home's energy efficiency with...

163

Cooling Evolution of Hybrid Stars  

E-Print Network (OSTI)

The cooling of compact isolated objects for different values of the gravitational mass has been simulated for two alternative assumptions. One is that the interior of the star is purely hadronic and second that the star can have a rather large quark core. It has been shown that within a nonlocal chiral quark model the critical density for a phase transition to color superconducting quark matter under neutron star conditions can be low enough for these phases to occur in compact star configurations with masses below 1.3 M_sun. For a realistic choice of parameters the equation of state (EoS) allows for 2SC quark matter with a large quark gap ~ 100 MeV for u and d quarks of two colors that coexists with normal quark matter within a mixed phase in the hybrid star interior. We argue that, if in the hadronic phase the neutron pairing gap in 3P_2 channel is larger than few keV and the phases with unpaired quarks are allowed, the corresponding hybrid stars would cool too fast. Even in the case of the essentially suppressed 3P_2 neutron gap if free quarks occur for M cooling data existing by today. It is suggested to discuss a "2SC+X" phase, as a possibility to have all quarks paired in two-flavor quark matter under neutron star constraints, where the X-gap is of the order of 10 keV - 1 MeV. Density independent gaps do not allow to fit the cooling data. Only the presence of an X-gap that decreases with increase of the density could allow to appropriately fit the data in a similar compact star mass interval to that following from a purely hadronic model.

H. Grigorian

2005-02-28T23:59:59.000Z

164

STAR FORMATION IN DENSE CLUSTERS  

SciTech Connect

A model of core-clump accretion with equally likely stopping describes star formation in the dense parts of clusters, where models of isolated collapsing cores may not apply. Each core accretes at a constant rate onto its protostar, while the surrounding clump gas accretes as a power of protostar mass. Short accretion flows resemble Shu accretion and make low-mass stars. Long flows resemble reduced Bondi accretion and make massive stars. Accretion stops due to environmental processes of dynamical ejection, gravitational competition, and gas dispersal by stellar feedback, independent of initial core structure. The model matches the field star initial mass function (IMF) from 0.01 to more than 10 solar masses. The core accretion rate and the mean accretion duration set the peak of the IMF, independent of the local Jeans mass. Massive protostars require the longest accretion durations, up to 0.5 Myr. The maximum protostar luminosity in a cluster indicates the mass and age of its oldest protostar. The distribution of protostar luminosities matches those in active star-forming regions if protostars have a constant birthrate but not if their births are coeval. For constant birthrate, the ratio of young stellar objects to protostars indicates the star-forming age of a cluster, typically {approx}1 Myr. The protostar accretion luminosity is typically less than its steady spherical value by a factor of {approx}2, consistent with models of episodic disk accretion.

Myers, Philip C., E-mail: pmyers@cfa.harvard.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2011-12-10T23:59:59.000Z

165

Cooling Evolution of Hybrid Stars  

E-Print Network (OSTI)

The cooling of compact isolated objects for different values of the gravitational mass has been simulated for two alternative assumptions. One is that the interior of the star is purely hadronic and second that the star can have a rather large quark core. It has been shown that within a nonlocal chiral quark model the critical density for a phase transition to color superconducting quark matter under neutron star conditions can be low enough for these phases to occur in compact star configurations with masses below 1.3 M_sun. For a realistic choice of parameters the equation of state (EoS) allows for 2SC quark matter with a large quark gap ~ 100 MeV for u and d quarks of two colors that coexists with normal quark matter within a mixed phase in the hybrid star interior. We argue that, if in the hadronic phase the neutron pairing gap in 3P_2 channel is larger than few keV and the phases with unpaired quarks are allowed, the corresponding hybrid stars would cool too fast. Even in the case of the essentially supp...

Grigorian, H

2005-01-01T23:59:59.000Z

166

EERE EnergyStar State Allocations | Department of Energy  

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

EERE EnergyStar State Allocations EERE EnergyStar State Allocations EEEnergyStarStateAllocations.pdf More Documents & Publications State Energy Efficient Appliance Rebate...

167

How the 1-100 ENERGY STAR score is calculated | ENERGY STAR  

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

is calculated Using the 1 - 100 ENERGY STAR score, you can understand how your building's energy consumption measures up against similar buildings nationwide. The ENERGY STAR score...

168

Wave Star Energy | Open Energy Information  

Open Energy Info (EERE)

Star Energy Star Energy Jump to: navigation, search Name Wave Star Energy Place Denmark Zip DK-2920 Product Denmark-based private wave device developer. References Wave Star Energy[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This company is listed in the Marine and Hydrokinetic Technology Database. This company is involved in the following MHK Projects: Wave Star Energy 1 10 Scale Model Test This company is involved in the following MHK Technologies: C5 WaveStar This article is a stub. You can help OpenEI by expanding it. Wave Star Energy is a company located in Denmark . References ↑ "Wave Star Energy" Retrieved from "http://en.openei.org/w/index.php?title=Wave_Star_Energy&oldid=678928" Categories: Clean Energy Organizations

169

New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars  

E-Print Network (OSTI)

We present the results of the continuation of our magnetic survey with FORS1 at the VLT of a sample of B-type stars consisting of confirmed or candidate beta Cephei stars and Slowly Pulsating B (hereafter SPB) stars, along with a small number of normal B-type stars. A weak mean longitudinal magnetic field of the order of a few hundred Gauss was detected in three beta Cephei stars and two stars suspected to be beta Cephei stars, in five SPB stars and eight stars suspected to be SPB stars. Additionally, a longitudinal magnetic field at a level larger than 3sigma has been diagnosed in two normal B-type stars, the nitrogen-rich early B-type star HD52089 and in the B5 IV star HD153716. Roughly one third of beta Cephei stars have detected magnetic fields: Out of 13 beta Cephei stars studied to date with FORS1, four stars possess weak magnetic fields, and out of the sample of six suspected beta Cephei stars two show a weak magnetic field. The fraction of magnetic SPBs and candidate SPBs is found to be higher: roughl...

Hubrig, S; De Cat, P; Schller, M; Morel, T; Ilyin, I

2009-01-01T23:59:59.000Z

170

STAR FORMATION IN ATOMIC GAS  

SciTech Connect

Observations of nearby galaxies have firmly established, over a broad range of galactic environments and metallicities, that star formation occurs exclusively in the molecular phase of the interstellar medium (ISM). Theoretical models show that this association results from the correlation between chemical phase, shielding, and temperature. Interstellar gas converts from atomic to molecular only in regions that are well shielded from interstellar ultraviolet (UV) photons, and since UV photons are also the dominant source of interstellar heating, only in these shielded regions does the gas become cold enough to be subject to Jeans instability. However, while the equilibrium temperature and chemical state of interstellar gas are well correlated, the timescale required to reach chemical equilibrium is much longer than that required to reach thermal equilibrium, and both timescales are metallicity-dependent. Here I show that the difference in timescales implies that, at metallicities below a few percent of the solar value, well shielded gas will reach low temperatures and proceed to star formation before the bulk of it is able to convert from atomic to molecular. As a result, at extremely low metallicities, star formation will occur in a cold atomic phase of the ISM rather than a molecular phase. I calculate the observable consequences of this result for star formation in low-metallicity galaxies, and I discuss how some current numerical models for H{sub 2}-regulated star formation may need to be modified.

Krumholz, Mark R., E-mail: krumholz@ucolick.org [Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States)

2012-11-01T23:59:59.000Z

171

Old and new neutron stars  

Science Conference Proceedings (OSTI)

The youngest known radiopulsar in the rapidly spinning magnetized neutron star which powers the Crab Nebula, the remnant of the historical supernova explosion of 1054 AD. Similar neutron stars are probably born at least every few hundred years, but are less frequent than Galactic supernova explosions. They are initially sources of extreme relativistic electron and/or positron winds (approx.10/sup 38/s/sup -1/ of 10/sup 12/ eV leptons) which greatly decrease as the neutron stars spin down to become mature pulsars. After several million years these neutron stars are no longer observed as radiopulsars, perhaps because of large magnetic field decay. However, a substantial fraction of the 10/sup 8/ old dead pulsars in the Galaxy are the most probable source for the isotropically distributed ..gamma..-ray burst detected several times per week at the earth. Some old neutron stars are spun-up by accretion from companions to be resurrected as rapidly spinning low magnetic field radiopulsars. 52 references, 6 figures, 3 tables.

Ruderman, M.

1984-09-01T23:59:59.000Z

172

ENERGY STAR Score for Warehouses  

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

Warehouses in the United States Page 1 Warehouses in the United States Page 1 ENERGY STAR Score for Warehouses in the United States Technical Reference OVERVIEW The ENERGY STAR Score for warehouses applies to unrefrigerated or refrigerated buildings that are used to store goods, manufactured products, merchandise or raw materials. The objective of the ENERGY STAR score is to provide a fair assessment of the energy performance of a property relative to its peers, taking into account the climate, weather, and business activities at the property. To identify the aspects of building activity that are significant drivers of energy use and then normalize for those factors, a statistical analysis of the peer building population is

173

SNAPSHOT … THE ENERGY STAR  

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

Fall 2008 Introduction At mid-year 2008*, commercial and industrial (C&I) leaders continued to make great progress in their efforts to improve energy efficiency and reduce greenhouse gas emissions across their buildings and facilities. In the first six months of 2008, key indicators of progress have already exceeded activity levels from 2007. More than 1,500 organizations and individuals now participate in the ENERGY STAR Challenge Close to 2 billion new square feet of commercial building floor space rated in the first half of the year bringing the total to about 9.5 billion over 71,000 buildings Labels awarded through June 2008 almost equal the 2007 total, with about 5,000 facilities now qualified as ENERGY STAR ENERGY STAR Leader activity on the rise this year; almost 60 commercial partners achieved key

174

Toy Stars in two dimensions  

E-Print Network (OSTI)

Toy Stars are gas masses where the compressibility is treated without approximations but gravity is replaced by a force which, for any pair of masses, is along their line of centres and proportional to their separation. They provide an invaluable resource for testing the suitability of numerical codes for astrophysical gas dynamics. In this paper we derive the equations for both small amplitude oscillations and non linear solutions for rotating and pulsating Toy Stars in two dimensions, and show that the solutions can be reduced to a small number of ordinary differential equations. We compare the accurate solutions of these equations with Smoothed Particle Hydrodynamics (SPH) simulations. The two dimensional Toy Star solutions are found to provide an excellent benchmark for SPH algorithms, highlighting many of the strengths and also some weaknesses of the method.

J. J. Monaghan; D. J. Price

2005-10-25T23:59:59.000Z

175

Alliance Star Energy LLC | Open Energy Information  

Open Energy Info (EERE)

Star Energy LLC Jump to: navigation, search Name Alliance Star Energy LLC Place California Utility Id 56929 References EIA Form EIA-861 Final Data File for 2010 - File220101...

176

Solar Star NAFB LLC | Open Energy Information  

Open Energy Info (EERE)

Star NAFB LLC Jump to: navigation, search Name Solar Star NAFB LLC Place Nevada Utility Id 56203 References EIA Form EIA-861 Final Data File for 2010 - File220101 LinkedIn...

177

Note on star-autonomous comonads  

E-Print Network (OSTI)

We develop an alternative approach to star-autonomous comonads via linearly distributive categories. It is shown that in the autonomous case the notions of star-autonomous comonad and Hopf comonad coincide.

Pastro, Craig

2010-01-01T23:59:59.000Z

178

Photos and graphics | ENERGY STAR Buildings & Plants  

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guidelines Refer to the ENERGY STAR Identity Guidelines for proper usage of the ENERGY STAR and Portfolio Manager marks. Graphics Click on a graphic to bring up a larger...

179

Industrial energy management information center | ENERGY STAR  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

180

ENERGY STAR Score for Data Centers  

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

Data Centers in the United States Page 1 ENERGY STAR Score for Data Centers in the United States Technical Reference OVERVIEW The ENERGY STAR Score for Data Centers applies to...

Note: This page contains sample records for the topic "waha lone star" 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

Advance your energy program | ENERGY STAR  

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corporate energy directors is without parallel. Join ENERGY STAR and get connected to the learning curve. Learn about world-class energy programs. EPA has profiled key ENERGY STAR...

182

Cold quark matter in compact stars  

Science Conference Proceedings (OSTI)

We used an equation of state for the cold quark matter to the study of properties of quark stars. We also discuss the absolute stability of quark matter and compute the mass-radius relation for self-bound stars.

Franzon, B.; Fogaca, D. A.; Navarra, F. S. [Instituto de Fisica, Universidade de Sao Paulo Rua do Matao, Travessa R, 187, 05508-090 Sao Paulo, SP (Brazil); Horvath, J. E. [Instituto de Astronomia, Geofisica e Ciencias Atmosfericas, Universidade de Sao Paulo, Rua do Matao, 1226, 05508-090, Sao Paulo, SP (Brazil)

2013-03-25T23:59:59.000Z

183

Energy strategy for the future | ENERGY STAR  

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Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

184

Nuclear Physics of Neutron Stars  

E-Print Network (OSTI)

Understanding the equation of state (EOS) of cold nuclear matter, namely, the relation between the pressure and energy density, is a central goal of nuclear physics that cuts across a variety of disciplines. Indeed, the limits of nuclear existence, the collision of heavy ions, the structure of neutron stars, and the dynamics of core-collapse supernova, all depend critically on the equation of state of hadronic matter. In this contribution I will concentrate on the special role that nuclear physics plays in constraining the EOS of cold baryonic matter and its impact on the properties of neutron stars.

J. Piekarewicz

2009-01-28T23:59:59.000Z

185

ENERGY STAR Industrial Plant Certification: Professional Engineers...  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

186

New lambda Bootis stars with a shell  

E-Print Network (OSTI)

We publish here the second part of our spectroscopic survey at high dispersion of some known and suspected lambda Bootis stars with a view to detecting circumstellar shell features. Eight stars of our sample exhibit such features. These stars are fast rotators, a result which is in line with Holweger and Rentzsch-Holm's study (1995). The analysis of the photometric data has allowed us to confirm the exclusion of a few stars misclassified from the lambda Bootis group.

B. Hauck; D. Ballereau; J. Chauville

1997-09-02T23:59:59.000Z

187

Black Stars and Gamma Ray Bursts  

E-Print Network (OSTI)

Stars that are collapsing toward forming a black hole but are frozen near the Schwarzschild horizon are termed ``black stars''. Collisions of black stars, in contrast to black hole collisions, may be sources of gamma ray bursts, whose basic parameters are estimated quite simply and are found to be consistent with observed gamma ray bursts. Black star gamma ray bursts should be preceded by gravitational wave emission similar to that from the coalescence of black holes.

Tanmay Vachaspati

2007-06-08T23:59:59.000Z

188

Join ENERGY STAR as a partner | ENERGY STAR Buildings & Plants  

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Join ENERGY STAR as a partner Join ENERGY STAR as a partner Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can ENERGY STAR help your business? Get started Join ENERGY STAR as a partner Service and Product Provider associations partnering with ENERGY STAR ENERGY STAR service & product provider training series Service and product provider's marketing toolkit

189

Theory of cooling neutron stars versus observations  

E-Print Network (OSTI)

We review current state of neutron star cooling theory and discuss the prospects to constrain the equation of state, neutrino emission and superfluid properties of neutron star cores by comparing the cooling theory with observations of thermal radiation from isolated neutron stars.

Yakovlev, D G; Kaminker, A D; Potekhin, A Yu

2007-01-01T23:59:59.000Z

190

Diagnosability of star graphs with missing edges  

Science Conference Proceedings (OSTI)

In this paper, we study the system diagnosis on an n-dimensional star under the comparison model. Following the concept of local diagnosability [3], the strong local diagnosability property [7] is discussed; this property describes the equivalence of ... Keywords: Comparison diagnosis model, Extended star structure, Local diagnosability, MM* diagnosis model, Star graph, Strong local diagnosability property

Chieh-Feng Chiang; Guo-Huang Hsu; Lun-Min Shih; Jimmy J. M. Tan

2012-04-01T23:59:59.000Z

191

Asteroseismology of chemically peculiar stars  

E-Print Network (OSTI)

Pulsational variability is observed in several types of main sequence stars with anomalous chemical abundances. In this contribution I summarize the relationship between pulsations and chemical peculiarities, giving special emphasis to rapid oscillations in magnetic Ap stars. These magneto-acoustic pulsators provide unique opportunities to study the interaction of pulsations, chemical inhomogeneities, and strong magnetic fields. Time-series monitoring of rapidly oscillating Ap stars using high-resolution spectrometers at large telescopes and ultra-precise space photometry has led to a number of important breakthroughs in our understanding of these interesting objects. Interpretation of the roAp frequency spectra has allowed constraining fundamental stellar parameters and probing poorly known properties of the stellar interiors. At the same time, investigation of the pulsational wave propagation in chemically stratified atmospheres of roAp stars has been used as a novel asteroseismic tool to study pulsations as a function of atmospheric height and to map in detail the horizontal structure of the magnetically-distorted p-modes.

O. Kochukhov

2008-12-01T23:59:59.000Z

192

Building Energy Software Tools Directory: Star Perfomer  

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Star Perfomer Star Perfomer Star Perfomer logo. Outlines simple steps to help office building owners, managers and tenants improve their greenhouse and energy efficiency performance, simply by asking some straightforward questions about the size, operating hours, current performance and equipment standards of the building. Star Performer is a diagnostic tool that uses the current operational energy performance of the building measured against a national benchmark, obtained through the Australian Building Greenhouse Rating scheme (see links below), as a basis for making recommendations. The tool covers all areas of the building which affect operational energy performance, including building fabric, equipment and operational practices. Star Perfomer will point you in the right direction and give

193

NLTE wind models of hot subdwarf stars  

E-Print Network (OSTI)

We calculate NLTE models of stellar winds of hot compact stars (central stars of planetary nebulae and subdwarf stars). The studied range of subdwarf parameters is selected to cover a large part of these stars. The models predict the wind hydrodynamical structure and provide mass-loss rates for different abundances. Our models show that CNO elements are important drivers of subdwarf winds, especially for low-luminosity stars. We study the effect of X-rays and instabilities on these winds. Due to the line-driven wind instability, a significant part of the wind could be very hot.

Krticka, Jiri; 10.1007/s10509-010-0385-z

2010-01-01T23:59:59.000Z

194

Energy Star Rebate Finder | Open Energy Information  

Open Energy Info (EERE)

Energy Star Rebate Finder Energy Star Rebate Finder Jump to: navigation, search Tool Summary LAUNCH TOOL Name: Energy Star Rebate Finder Agency/Company /Organization: United States Environmental Protection Agency Sector: Energy Focus Area: Energy Efficiency Phase: Evaluate Options, Prepare a Plan Resource Type: Online calculator User Interface: Mobile Device Website: m.epa.gov/apps/energy.html Web Application Link: m.epa.gov/apps/energy.html Cost: Free Energy Star Rebate Finder Screenshot References: EPA[1] Logo: Energy Star Rebate Finder Find special offers and rebates from Energy Star partners by entering your zip code. Overview To encourage customers to buy energy efficient products, Energy Star partners occasionally sponsor special offers, such as sales tax exemptions or credits, or rebates on qualified products. Partners also occasionally

195

Green Star Alternative Energy | Open Energy Information  

Open Energy Info (EERE)

Green Star Alternative Energy Green Star Alternative Energy Jump to: navigation, search Name Green Star Alternative Energy Place San Diego, California Zip 92108 Sector Wind energy Product A US-based wind energy project developer. References Green Star Alternative Energy[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Green Star Alternative Energy is a company located in San Diego, California . References ↑ "Green Star Alternative Energy" Retrieved from "http://en.openei.org/w/index.php?title=Green_Star_Alternative_Energy&oldid=346056" Categories: Clean Energy Organizations Companies Organizations Stubs What links here Related changes Special pages Printable version Permanent link

196

Build Your Business with ENERGY STAR  

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

Service and Product Providers: Service and Product Providers: Build Your Business with ENERGY STAR ® Let ENERGY STAR Be Your Market Advantage Look to ENERGY STAR to help you bring value to your customers and more sales to your organization. Service and Product Providers (SPPs) are integral in helping existing commercial buildings use energy more efficiently. Partnering with ENERGY STAR provides you with access to free tools and resources to help you devise and implement energy- efficient strategies that are right for your customers: > Use the ENERGY STAR Brand to Enhance Your Credibility: Use the nationally recognized ENERGY STAR partner logo on your promotional materials to symbolize your commitment to delivering energy efficiency and financial savings to customers. Help customers build their reputation as environmental and social leaders through work with an ENERGY STAR SPP partner.

197

Supermassive black holes from supermassive stars  

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

Supermassive black holes from supermassive stars Supermassive black holes from supermassive stars 1663 Los Alamos science and technology magazine Latest Issue:November 2013 All Issues » submit Supermassive black holes from supermassive stars Supermassive stars in the early universe gave supermassive black holes a head start March 25, 2013 simulations suggest that star formation conditions back then allowed the first stars to become supermassive themselves In this simulation, a black hole that was just formed by the collapse of a supermassive star is surrounded by a distribution of gas (color indicates density). Because the black hole (located at the center but too small to see) grows by consuming the available gas, simulations like this one help determine how quickly the black hole can grow. The progenitor of this black

198

ORISE: Voluntary Protection Program (VPP) Star Status  

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

Voluntary Protection Program (VPP) Star Status Voluntary Protection Program (VPP) Star Status Within the U.S. Department of Energy's (DOE) Voluntary Protection Program (VPP), there are three levels of recognition: STAR, MERIT and DEMONSTRATION. Contractors' programs that meet the requirements for outstanding safety and health programs, earn VPP STAR status-the highest achievement level. In December of 2003, the Oak Ridge Institute for Science and Education (ORISE) first earned STAR distinction following a comprehensive evaluation of its application for the VPP program. At that time, ORISE was just the 21st DOE site and the first in Tennessee to earn such exemplary recognition. In 2011 ORISE received its seventh consecutive Star of Excellence award. Today, ORISE is one of more than two dozen DOE sites to achieve VPP STAR

199

Find ENERGY STAR certified buildings and plants | ENERGY STAR Buildings &  

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

» Buildings & Plants » Buildings & Plants » About us » Find ENERGY STAR certified buildings and plants Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Find out who's partnered with ENERGY STAR Become an ENERGY STAR partner Find ENERGY STAR certified buildings and plants Registry of ENERGY STAR certified buildings and plants

200

ENERGY STAR SNAPSHOT - Spring 2009  

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

Measuring Progress in the Measuring Progress in the Commercial and Industrial Sectors Fall 2009 Summary By mid-year 2009, key commercial and industrial organizations have already surpassed their 2008 efforts to improve energy performance and reduce greenhouse gas emissions: * More buildings have been rated at mid year 2009 than in all of last year. This brings the total number of buildings with energy performance ratings to more than 97,000. * Nearly 1,850 buildings have earned the ENERGY STAR in 2009, ahead of the 2008 mid-year total. * Almost 30 organizations, mostly among our nation's public school districts, have already achieved significant portfolio-wide energy improvements or top performance. The ENERGY STAR Snapshot provides an at-a-glance summary of the key performance indicators behind

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


201

Magnetization of neutron star matter  

E-Print Network (OSTI)

The magnetization of neutron star matter in magnetic fields is studied by employing the FSUGold interaction. It is found that the magnetic susceptibilities of the charged particles (proton, electron and muon) can be larger than that of neutron. The effects of the anomalous magnetic moments (AMM) of each component on the magnetic susceptibility are examined in detail. It is found that the proton and electron AMM affect their respective magnetic susceptibility evidently in strong magnetic fields. In addition, they are the protons instead of the electrons that contribute most significantly to the magnetization of the neutron star matter in a relative weak magnetic field, and the induced magnetic field due to the magnetization can be appear to be very large. Finally, the effect of the density-dependent symmetry energy on the magnetization is discussed.

Dong, Jianmin; Gu, Jianzhong

2013-01-01T23:59:59.000Z

202

Properties of Neutron Star Critical Collapses  

E-Print Network (OSTI)

Critical phenomena in gravitational collapse opened a new mathematical vista into the theory of general relativity and may ultimately entail fundamental physical implication in observations. However, at present, the dynamics of critical phenomena in gravitational collapse scenarios are still largely unknown. My thesis seeks to understand the properties of the threshold in the solution space of the Einstein field equations between the black hole and neutron star phases, understand the properties of the neutron star critical solution and clarify the implication of these results on realistic astrophysical scenarios. We develop a new set of neutron star-like initial data to establish the universality of the neutron star critical solution and analyze the structure of neutron star and neutron star-like critical collapses via the study of the phase spaces. We also study the different time scales involved in the neutron star critical solution and analyze the properties of the critical index via comparisons between neutron star and neutron star-like initial data. Finally, we explore the boundary of the attraction basin of the neutron star critical solution and its transition to a known set of non-critical fixed points.

Mew-Bing Wan

2010-01-10T23:59:59.000Z

203

Home Performance with Energy Star  

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

- HPwES - HPwES Home Performance with ENERGY STAR Ely Jacobsohn U.S. Department of Energy Ely.jacobsohn@ee.doe.gov, 202-287-1333 April 3, 2013 2 | Building Technologies Office eere.energy.gov Purpose and Objectives: Problem Statement Works to advance the Department's and Administration's energy-related goals in the residential sector Face challenging and often conflicting mandates to save energy, meet environmental goals, and satisfy needs of

204

Energy Star Lighting Verification Program  

SciTech Connect

The Program for the Evaluation and Analysis of Residential Lighting (PEARL) is a watchdog program. It was created in response to complaints received by utility program managers about the performance of certain Energy Star lighting products being promoted within their service territories and the lack of a self-policing mechanism within the lighting industry that would ensure the reliability of these products and their compliance with ENERGY STAR specifications. To remedy these problems, PEARL purchases and tests products that are available to the consumers in the marketplace. The Lighting Research Center (LRC) tests the selected products against the corresponding Energy Star specifications. This report includes the experimental procedure and results of Cycle Seven of PEARL program during the period of April 2006 to September 2006, along with the description of apparatus used, equipment calibration process, experimental methodology, and research findings from the testing. LRC continued receiving the CFL samples purchased by sponsors and finished performing the sphere testing for all CFL models at 100 hours of life. After that LRC aged the CFL samples to 1000 hours of life, and then performed sphere testing for all CFL models at 1000 hours of life. Then the CFLs were placed on the test rack to be aged to 40% of their rated life. Rapid Cycle Stress Test was also performed for all models using different sets of CFL samples.

Conan O'Rourke; Yutao Zhou

2006-09-30T23:59:59.000Z

205

Energy Star Lighting Verification Program  

SciTech Connect

The Program for the Evaluation and Analysis of Residential Lighting (PEARL) is a watchdog program. It was created in response to complaints received by utility program managers about the performance of certain Energy Star lighting products being promoted within their service territories and the lack of a self-policing mechanism within the lighting industry that would ensure the reliability of these products and their compliance with ENERGY STAR specifications. To remedy these problems, PEARL purchases and tests products that are available to the consumers in the marketplace. The Lighting Research Center (LRC) tests the selected products against the corresponding Energy Star specifications. This report includes the experimental procedure and results of Cycle Seven and Cycle Eight of PEARL program during the period of October 2006 to March 2007, along with the description of apparatus used, equipment calibration process, experimental methodology, and research findings from the testing. LRC finished performing the sphere testing for all CFL models in Cycle Seven at 40% of their rated life. LRC also performed re-test of Rapid Cycle Stress Test, under the request of DOE, for five CFL models that failed the Rapid Cycle Stress Test in Cycle Seven. From January 2007 to March 2007, LRC coordinated the procuring efforts for the CFL models that were selected for Cycle Eight.

Conan O'Rourke; Yutao Zhou

2007-03-31T23:59:59.000Z

206

From Gas to Stars Over Cosmic Time  

E-Print Network (OSTI)

From the time the first stars formed over 13 billion years ago to the present, star formation has had an unexpectedly dynamic history. At first, the star formation rate density increased dramatically, reaching a peak 10 billion years ago more than ten times the present day value. Observations of the initial rise in star formation remain difficult, poorly constraining it. Theoretical modeling has trouble predicting this history because of the difficulty in following the feedback of energy from stellar radiation and supernova explosions into the gas from which further stars form. Observations from the ground and space with the next generation of instruments should reveal the full history of star formation in the universe, while simulations appear poised to accurately predict the observed history.

Mac Low, Mordecai-Mark

2013-01-01T23:59:59.000Z

207

Boson stars: Chemical potential and quark condensates  

E-Print Network (OSTI)

We study the properties of a star made of self-gravitating bosons gas in a mean-field approximation. A generalized set of Tolman-Oppenheimer-Volkov(TOV) equations is derived to incorporate the effect of chemical-potential in the general relativistic frame work. The metric-dependence of the chemical-potential gives a new class of solutions for the boson stars. It is demonstrated that the maximum mass and radius of the star change in a significant way when the effect of finite chemical-potential is considered. We also discuss the case of a boson star made of quark-condensates. It is found that when the self-interaction between the condensates is small as compared to their mass, the typical density is too high to form a diquark-boson star. Our results indicate that the star of quark-condensate may be formed in a low-density and high-pressure regime.

Jitesh R. Bhatt; V. Sreekanth

2009-10-12T23:59:59.000Z

208

Why you should design to earn EPA's ENERGY STAR | ENERGY STAR  

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

bills and help protect our environment. Learn about ENERGY STAR Products Save Energy at Home Take the Pledge Learn about Climate Change ENERGY STAR Products Tax Credits Ask an...

209

From nuclear matter to Neutron Stars  

E-Print Network (OSTI)

Neutron stars are the most dense objects in the observable Universe and conventionally one uses nuclear theory to obtain the equation of state (EOS) of dense hadronic matter and the global properties of these stars. In this work, we review various aspects of nuclear matter within an effective Chiral model and interlink fundamental quantities both from nuclear saturation as well as vacuum properties and correlate it with the star properties.

T. K. Jha

2009-02-02T23:59:59.000Z

210

ENERGY STAR Guide for Licensed Professionals | ENERGY STAR Buildings &  

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

Guide for Licensed Professionals Guide for Licensed Professionals Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In This Section Campaigns Commercial building design Communications resources Energy management guidance Financial resources Portfolio Manager Products and purchasing Recognition Research and reports Service and product provider (SPP) resources Success stories Target Finder

211

ENERGY STAR Challenge for Industry: Registration Form | ENERGY STAR  

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

Registration Form Registration Form Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In This Section Campaigns Commercial building design Communications resources Energy management guidance Financial resources Portfolio Manager Products and purchasing Recognition Research and reports Service and product provider (SPP) resources Success stories Target Finder Technical documentation

212

ENERGY STAR Success Story: Kohl's Department Stores | ENERGY STAR  

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

Kohl's Department Stores Kohl's Department Stores Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In This Section Campaigns Commercial building design Communications resources Energy management guidance Financial resources Portfolio Manager Products and purchasing Recognition Research and reports Service and product provider (SPP) resources Success stories Target Finder

213

ENERGY STAR Challenge for Industry: Participant Handbook | ENERGY STAR  

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

Participant Handbook Participant Handbook Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In This Section Campaigns Commercial building design Communications resources Energy management guidance Financial resources Portfolio Manager Products and purchasing Recognition Research and reports Service and product provider (SPP) resources Success stories Target Finder Technical documentation

214

ENERGY STAR Building Upgrade Manual Chapter 6: Lighting | ENERGY STAR  

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

6: Lighting 6: Lighting Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In This Section Campaigns Commercial building design Communications resources Energy management guidance Financial resources Portfolio Manager Products and purchasing Recognition Research and reports Service and product provider (SPP) resources Success stories Target Finder Technical documentation

215

ENERGY STAR Success Story: San Diego Convention Center | ENERGY STAR  

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

San Diego Convention Center San Diego Convention Center Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In This Section Campaigns Commercial building design Communications resources Energy management guidance Financial resources Portfolio Manager Products and purchasing Recognition Research and reports Service and product provider (SPP) resources Success stories Target Finder

216

ENERGY STAR Building Upgrade Manual Chapter 2: Benchmarking | ENERGY STAR  

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

2: Benchmarking 2: Benchmarking Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In This Section Campaigns Commercial building design Communications resources Energy management guidance Financial resources Portfolio Manager Products and purchasing Recognition Research and reports Service and product provider (SPP) resources Success stories Target Finder Technical documentation

217

ENERGY STAR Success Story: Verizon Wireless | ENERGY STAR Buildings &  

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Verizon Wireless Verizon Wireless Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In This Section Campaigns Commercial building design Communications resources Energy management guidance Financial resources Portfolio Manager Products and purchasing Recognition Research and reports Service and product provider (SPP) resources Success stories Target Finder Technical documentation

218

Nuclear Star Clusters - Structure and Stellar Populations  

E-Print Network (OSTI)

This is an overview of nuclear star cluster observations, covering their structure, stellar populations, kinematics and possible connection to black holes at the centers of galaxies.

Neumayer, Nadine

2012-01-01T23:59:59.000Z

219

Get started | ENERGY STAR Buildings & Plants  

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

strides toward our energy conservation goals. Nelly Gomez, Vons Credit Union, 1 winner, bankfinancial institution category, 2012 ENERGY STAR National Building Competition...

220

Improve building and plant performance | ENERGY STAR  

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

performance Through ENERGY STAR, EPA provides tools and resources to help you save money and reduce your carbon emissions by improving the energy efficiency of building and...

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


221

Partnership Requirements: ENERGY STAR Partnership for Commercial...  

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

Partnership Requirements: ENERGY STAR Partnership for Commercial & Industrial Service and Product Providers (SPP) Secondary menu About us Press room Contact Us Portfolio Manager...

222

ENERGY STAR Qualified Boilers | Data.gov  

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

Qualified Boilers Consumer Data Apps Challenges Resources About Blogs Let's Talk Feedback Consumer You are here Data.gov Communities Consumer Data ENERGY STAR Qualified...

223

Grocery and convenience stores | ENERGY STAR  

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

To save energy while using larger equipment, such as HVAC, heat pumps, motors, boilers, furnaces, and turbines, consider buying ENERGY STAR certified products. Whether you...

224

ENERGY STAR Score for Wastewater Treatment Plants  

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

!! !! July 2013 ENERGY STAR Score for Wastewater Treatment Plants in the United States Page 1 ENERGY STAR Score for Wastewater Treatment Plants in the United States Technical Reference OVERVIEW ! The ENERGY STAR Score for Wastewater Treatment Plants applies to primary, secondary, and advanced treatment facilities with or without nutrient removal capacity. The objective of the ENERGY STAR score is to provide a fair assessment of the energy performance of a property relative to its peers, taking into account the climate, weather, and business activities at the property. To identify the aspects of building activity that are significant drivers of energy

225

Residential Energy Star Appliance Rebate Program  

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

Energy Trust of Oregon offers rebates for Energy Star refrigerators, freezers and clothes washers to Oregon residential electric service customers of Portland General Electric (PGE) and Pacific...

226

EPA's Target Finder calculator | ENERGY STAR  

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

sample in the nation, plus have it normalized for size, operating characteristics, and weather. Target Finder Access ENERGY STAR Target Finder When to use Portfolio Manager instead...

227

StarSolar Corporation | Open Energy Information  

Open Energy Info (EERE)

Cambridge, Massachusetts Product Developing a nanostructured 'photonic crystal' PV cell with antireflective coating. References StarSolar Corporation1 LinkedIn Connections...

228

Operations and maintenance reports | ENERGY STAR  

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

from an expert Take a comprehensive approach Operations and maintenance reports ENERGY STAR Building Upgrade Manual Install renewable energy systems Save water to save energy...

229

Nine New Variable Stars in Camelopardalis  

E-Print Network (OSTI)

Nine new short period variable stars have been discovered in the direction of the open cluster Cr464 in Camelopardalis. The field was observed using Tzec Maun Observatory's telescope AP180. Two new variable stars were classified as pulsating stars (RRab and RRc types). The other seven stars are binary systems. One of them is of ELL-type, four binaries were recognized as EW-type, and two systems are rather short period EA-type binaries. All new variables were registered in the VSX catalogue.

Virnina, Natalia A

2013-01-01T23:59:59.000Z

230

ENERGY STAR Score for Wastewater Treatment Plants  

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

1 to 100 percentile ranking of performance, relative to the national population. Property Types. The ENERGY STAR score for wastewater treatment plants applies to primary,...

231

ENERGY STAR Score for Retail Stores  

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

100 percentile ranking of performance, relative to the national population. Property Types. The ENERGY STAR score for retail stores applies to retail stores and wholesale...

232

Step 5: Implement action plan | ENERGY STAR  

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

team to help them get the word out. Find ENERGY STAR communications tools Train staff Through training, access to information, and transfer of successful practices,...

233

ENERGY STAR Performance Contracting Best Practices  

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

Contracting Best Practices Prepared for: U.S. Environmental Protection Agency ENERGY STAR Buildings Prepared by: ICF International National Association of Energy Services...

234

ENERGY STAR Guidelines for Energy Management  

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

Guidelines for Energy Management ENERGY STAR is a U.S. Environmental Protection Agency Program helping organizations and individuals fight climate change through superior energy...

235

ENERGY STAR Resources for Small & Medium Manufactures  

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

Small & Medium Manufacturers Guide to Energy Management June 2013 ENERGY STAR is a U.S. Environmental Protection Agency Program helping organizations and individuals fight climate...

236

How to Apply for Energy Star Certification  

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

Receive notification of the application's status. June 2013 1 Property Types Eligible for ENERGY STAR Certification Bank Branch Courthouse Data Center Distribution Center Financial...

237

Hotel Scoring Model FAQs | ENERGY STAR  

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

use per square foot, and service levels based on operating characteristics. Download the ENERGY STAR Hotel Rating Model FAQs here. Energy Efficient Products Learn about ENERGY...

238

ENERGY STAR Industrial Plant Certification: Instructions for...  

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

Senior care resources Small business resources State and local government resources ENERGY STAR Industrial Plant Certification: Instructions for applying This document...

239

STATE AND LOCAL GOVERNMENTS LEVERAGING ENERGY STAR  

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

across the country are taking bold steps to protect the environment and lower energy costs by adopting policies that leverage EPA's ENERGY STAR tools to reduce energy use...

240

2006 Is the Sun a Random Star  

E-Print Network (OSTI)

Abstract: The properties of our star may be associated with special prerequisites for life. By comparing our Sun to other stars in our galaxy, we may be able to identify such prerequisites. If our star is typical, stellar conditions appropriate for life, and life itself may be common in the Universe. On the other hand, if the Sun is atypical, conditions appropriate for life may be uncommon. Here we describe a method to quantify how typical or atypical the Sun is compared with other stars

Jose A. Robles; Charles H. Lineweaver

2007-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "waha lone star" 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

How to Apply for ENERGY STAR Certification  

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

a site visit, verifying the information in your application. Property Types Eligible for ENERGY STAR Certification Bank Branch Courthouse Data Center Distribution Center Financial...

242

The Nuclear Physics of Neutron Stars  

E-Print Network (OSTI)

A remarkable fact about spherically-symmetric neutron stars in hydrostatic equilibrium - the so-called Schwarzschild stars - is that the only physics that they are sensitive to is the equation of state of neutron-rich matter. As such, neutron stars provide a myriad of observables that may be used to constrain poorly known aspects of the nuclear interaction under extreme conditions of density. After discussing many of the fascinating phases encountered in neutron stars, I will address how powerful theoretical, experimental, and observational constraints may be used to place stringent limits on the equation of state of neutron-rich matter.

J. Piekarewicz

2008-02-27T23:59:59.000Z

243

Star Formation in the Gulf of Mexico  

E-Print Network (OSTI)

We present an optical/infrared study of the dense molecular cloud, L935, dubbed "The Gulf of Mexico", which separates the North America and the Pelican nebulae, and we demonstrate that this area is a very active star forming region. A wide-field imaging study with interference filters has revealed 35 new Herbig-Haro objects in the Gulf of Mexico. A grism survey has identified 41 Halpha emission-line stars, 30 of them new. A small cluster of partly embedded pre-main sequence stars is located around the known LkHalpha 185-189 group of stars, which includes the recently erupting FUor HBC 722.

Armond, Tina; Bally, John; Aspin, Colin

2011-01-01T23:59:59.000Z

244

Help your clients improve energy performance with ENERGY STAR...  

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

STAR tools and resources in your proposal. Read our introductory and best practices papers to learn why ESCOs use ENERGY STAR tools and how to integrate ENERGY STAR tools...

245

Support for ENERGY STAR Enforcement | Department of Energy  

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

Support for ENERGY STAR Enforcement Support for ENERGY STAR Enforcement By offering a means for consumers to buy products more energy-efficient than required by law, ENERGY STAR...

246

Do We Know of Any Maunder Minimum Stars?  

E-Print Network (OSTI)

Most stars previously identified as Maunder minimum stars are old stars evolved off of the main sequence. Analysis of activity measurements from the California and Carnegie Planet Search program stars and Hipparcos parallaxes implies that the canonical age-chromospheric activity relation breaks down for stars older than $\\sim 6$ Gyr when activity is calculated from Mount Wilson S values. Stars only 1 magnitude above the main sequence exhibit significantly suppressed activity levels which have been mistaken for examples of Maunder minimum behavior.

Jason T. Wright

2004-06-15T23:59:59.000Z

247

Columbia Water & Light - New Home Energy Star Rebate | Department...  

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

New Home Energy Star Rebate Columbia Water & Light - New Home Energy Star Rebate Eligibility Construction Residential Savings For Heating & Cooling Home Weatherization Construction...

248

Columbia Water & Light - Home Performance with Energy Star Rebates...  

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

Home Performance with Energy Star Rebates Columbia Water & Light - Home Performance with Energy Star Rebates Eligibility Residential Savings For Home Weatherization Commercial...

249

Equator Appliance: ENERGY STAR Referral (EZ 3720) | Department...  

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

Equator Appliance: ENERGY STAR Referral (EZ 3720) Equator Appliance: ENERGY STAR Referral (EZ 3720) October 5, 2010 DOE referred Equator Appliance clothes washer EZ 3720 to EPA,...

250

DOE Defends Decision to Revoke Energy Star Designation for Certain...  

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

Defends Decision to Revoke Energy Star Designation for Certain LG Refrigerators DOE Defends Decision to Revoke Energy Star Designation for Certain LG Refrigerators December 23,...

251

Equator Appliance: ENERGY STAR Referral (EZ 3720 CEE) | Department...  

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

Equator Appliance: ENERGY STAR Referral (EZ 3720 CEE) Equator Appliance: ENERGY STAR Referral (EZ 3720 CEE) October 5, 2010 DOE referred the matter of Equator clothes washer model...

252

Calendar Year 2009 Program Benefits for ENERGY STAR Labeled Products  

E-Print Network (OSTI)

to limited data regarding energy and usage patterns. The UECconsumption, usage, total energy, and ENERGY STAR marketBAU and ENERGY STAR cases, using power consumption and usage

Homan, Gregory K

2011-01-01T23:59:59.000Z

253

Laboratory Equipment - DynaPro NanoStar Dynamic Light ...  

Science Conference Proceedings (OSTI)

DynaPro NanoStar Dynamic Light Scattering. Description: Location: E136. The DynaPro NanoStar is a dynamic light scattering ...

2012-10-31T23:59:59.000Z

254

Green Star Products Inc GSPI | Open Energy Information  

Open Energy Info (EERE)

"Green Star Products Inc (GSPI)" Retrieved from "http:en.openei.orgwindex.php?titleGreenStarProductsIncGSPI&oldid346058" Categories: Clean Energy Organizations...

255

ENERGY STAR Challenge for Industry: Poster, "Our Actions Made...  

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

business resources State and local government resources ENERGY STAR Challenge for Industry: Poster, "Our Actions Made a Difference" This co-brandable poster is for ENERGY STAR...

256

Clean Energy Action Star Governor Schwarzenegger to Keynote ARPA...  

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

Action Star Governor Schwarzenegger to Keynote ARPA-E Energy Innovation Summit Clean Energy Action Star Governor Schwarzenegger to Keynote ARPA-E Energy Innovation Summit February...

257

Get buy-in from leadership and staff | ENERGY STAR  

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

energy, from simple steps to the comprehensive five-stage approach outlined in the ENERGY STAR Building Upgrade Manual. Or, consider enlisting the services of an ENERGY STAR...

258

Taunton Municipal Lighting Plant - Residential Energy Star Appliance...  

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

Taunton Municipal Lighting Plant - Residential Energy Star Appliance Rebate Program Taunton Municipal Lighting Plant - Residential Energy Star Appliance Rebate Program Eligibility...

259

NineStar Connect - Residential Energy Efficient Equipment Rebate...  

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

NineStar Connect - Residential Energy Efficient Equipment Rebate Program NineStar Connect - Residential Energy Efficient Equipment Rebate Program Eligibility Residential Savings...

260

Energy Star Guide for Restaurants, Putting Energy into Profit...  

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

STAR Guide for Restaurants Putting Energy into Profit ENERGY STAR , a U.S. Environmental Protection Agency program, helps us all save money and protect our environment through...

Note: This page contains sample records for the topic "waha lone star" 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

ENERGY STAR for Congregations: Action Workbook for Energy Stewardship  

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

light bulbs with ENERGY STAR qualified compact fluorescent lights (CFLs) or light emitting diode (LED) equipment, wherever appropriate. ENERGY STAR for Congregations: Action...

262

Energy-saving tips for everyone | ENERGY STAR  

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

Communicate and educate ENERGY STAR communications toolkit Bring Your Green to Work with ENERGY STAR Energy-saving tips for everyone Secondary menu About us Press room...

263

List of most active service and product providers | ENERGY STAR  

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

quality, and durability. Find Builders and Incentives Home Features and Benefits Homeowner Testimonials Resources for Partners Find ENERGY STAR Home Builders ENERGY STAR Home...

264

The role of low-mass star clusters in massive star formation. The Orion Case  

E-Print Network (OSTI)

To distinguish between the different theories proposed to explain massive star formation, it is crucial to establish the distribution, the extinction, and the density of low-mass stars in massive star-forming regions. We analyze deep X-ray observations of the Orion massive star-forming region using the Chandra Orion Ultradeep Project (COUP) catalog. We studied the stellar distribution as a function of extinction, with cells of 0.03 pc x 0.03 pc, the typical size of protostellar cores. We derived stellar density maps and calculated cluster stellar densities. We found that low-mass stars cluster toward the three massive star-forming regions: the Trapezium Cluster (TC), the Orion Hot Core (OHC), and OMC1-S. We derived low-mass stellar densities of 10^{5} stars pc^{-3} in the TC and OMC1-S, and of 10^{6} stars pc^{-3} in the OHC. The close association between the low-mass star clusters with massive star cradles supports the role of these clusters in the formation of massive stars. The X-ray observations show for ...

Rivilla, V M; Jimenez-Serra, I; Rodriguez-Franco, A

2013-01-01T23:59:59.000Z

265

Win ENERGY STAR Partner of the Year | ENERGY STAR Buildings & Plants  

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

Win ENERGY STAR Partner of the Year Win ENERGY STAR Partner of the Year Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Build an energy program Improve building and plant performance Earn the ENERGY STAR and other recognition Benchmark energy use ENERGY STAR in action Communicate and educate ENERGY STAR communications toolkit Bring Your Green to Work with ENERGY STAR

266

Why you should design to earn the ENERGY STAR | ENERGY STAR Buildings &  

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

Why you should design to earn the ENERGY STAR Why you should design to earn the ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Why you should design to earn the ENERGY STAR Leading firms choose ENERGY STAR Why new doesn't always mean efficient Follow EPA's step-by-step process ENERGY STAR Challenge for Architects Why you should design to earn the ENERGY STAR

267

Step 6: Complete the ENERGY STAR lifecycle | ENERGY STAR Buildings & Plants  

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

6: Complete the ENERGY STAR lifecycle 6: Complete the ENERGY STAR lifecycle Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Why design to earn ENERGY STAR Design to earn ENERGY STAR Step 1: Include efficiency in your project specs Step 2: Meet with your team and set a goal Step 3: Apply for Designed to Earn the ENERGY STAR recognition Step 4: Market your project as Designed to Earn the ENERGY STAR

268

SDSS spectroscopic survey of stars  

E-Print Network (OSTI)

In addition to optical photometry of unprecedented quality, the Sloan Digital Sky Survey (SDSS) is also producing a massive spectroscopic database. We discuss determination of stellar parameters, such as effective temperature, gravity and metallicity from SDSS spectra, describe correlations between kinematics and metallicity, and study their variation as a function of the position in the Galaxy. We show that stellar parameter estimates by Beers et al. show a good correlation with the position of a star in the g-r vs. u-g color-color diagram, thereby demonstrating their robustness as well as a potential for photometric parameter estimation methods. Using Beers et al. parameters, we find that the metallicity distribution of the Milky Way stars at a few kpc from the galactic plane is bimodal with a local minimum at [Z/Zo]~ -1.3. The median metallicity for the low-metallicity [Z/Zo] -1.3 sample. We also find that the low-metallicity sample has ~2.5 times larger velocity dispersion and that it does not rotate (at ...

Ivezic, Z; Uomoto, A; Bond, N; Beers, T; Allende-Prieto, C; Wilhelm, R; Lee, Y S; Sivarani, T; Juric, M; Lupton, R; Rockosi, C M; Knapp, G; Gunn, J; Yanny, B; Jester, S; Kent, S; Pier, J; Munn, J A; Richards, G; Newberg, H; Blanton, M; Eisenstein, D; Hawley, S; Anderson, S; Harris, H; Kiuchi, F; Chen, A; Bushong, J; Sohi, H; Haggard, D; Kimball, A; Barentine, J; Brewington, H; Harvanek, M; Kleinman, S; Krzesnski, J; Long, D; Nitta, A; Snedden, S A

2007-01-01T23:59:59.000Z

269

SDSS spectroscopic survey of stars  

E-Print Network (OSTI)

In addition to optical photometry of unprecedented quality, the Sloan Digital Sky Survey (SDSS) is also producing a massive spectroscopic database. We discuss determination of stellar parameters, such as effective temperature, gravity and metallicity from SDSS spectra, describe correlations between kinematics and metallicity, and study their variation as a function of the position in the Galaxy. We show that stellar parameter estimates by Beers et al. show a good correlation with the position of a star in the g-r vs. u-g color-color diagram, thereby demonstrating their robustness as well as a potential for photometric parameter estimation methods. Using Beers et al. parameters, we find that the metallicity distribution of the Milky Way stars at a few kpc from the galactic plane is bimodal with a local minimum at [Z/Zo]~ -1.3. The median metallicity for the low-metallicity [Z/Zo] -1.3 sample. We also find that the low-metallicity sample has ~2.5 times larger velocity dispersion and that it does not rotate (at the ~10 km/s level), while the rotational velocity of the high-metallicity sample decreases smoothly with the height above the galactic plane.

Z. Ivezic; D. Schlegel; A. Uomoto; N. Bond; T. Beers; C. Allende Prieto; R. Wilhelm; Y. Sun Lee; T. Sivarani; M. Juric; R. Lupton; C. Rockosi; G. Knapp; J. Gunn; B. Yanny; S. Jester; S. Kent; J. Pier; J. Munn; G. Richards; H. Newberg; M. Blanton; D. Eisenstein; S. Hawley; S. Anderson; H. Harris; F. Kiuchi; A. Chen; J. Bushong; H. Sohi; D. Haggard; A. Kimball; J. Barentine; H. Brewington; M. Harvanek; S. Kleinman; J. Krzesinski; D. Long; A. Nitta; S. Snedden; for the SDSS Collaboration

2007-01-17T23:59:59.000Z

270

ENERGY STAR SNAPSHOT … Spring 2009  

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

1 1 Snapshot data runs through June 30, 2011. The ENERGY STAR Snapshot provides an at-a-glance summary of the latest national ENERGY STAR metrics to help you, our partners, see the impact of your efforts. The ENERGY STAR Snapshot is distributed twice a year and provides: * Trends in energy benchmarking of commercial and industrial buildings. * State-by-state activity along with activity for the top Designated Market Areas. * Industrial sector participation in ENERGY STAR. * Trends in ENERGY STAR labeled commercial and industrial facilities. Summary By mid-year 2011, commercial and industrial organizations were on track to, or were already exceeding, figures for benchmarking and labeling that were set by end of year 2010. Since December, 2010:

271

ENERGY STAR SNAPSHOT … Spring 2010  

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

10 10 Summary In 2009, commercial and industrial organizations continued their impressive efforts to improve their energy performance and reduce greenhouse emissions. As a result: * More than 65,000 buildings received an ENERGY STAR energy performance score in 2009, a 50 percent increase over 2008 * Nearly 3,900 buildings earned the ENERGY STAR, a 20 percent increase over the record- breaking activity of the previous year * Almost 60 organizations achieved ENERGY STAR Leader recognition providing the greatest single year of savings since the program began in 2004 The ENERGY STAR Snapshot provides an at-a-glance summary of the key performance indicators behind these impressive results. The Snapshot reports the latest national ENERGY STAR metrics to help

272

ENERGY STAR SNAPSHOT … Spring 2009  

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

Snapshot data runs through December 31, 2010. Snapshot data runs through December 31, 2010. The ENERGY STAR Snapshot provides an at-a-glance summary of the latest national ENERGY STAR metrics to help you, our partners, see the impact of your efforts. The ENERGY STAR Snapshot is distributed twice a year and provides: Trends in energy benchmarking of commercial and industrial buildings. State-by-state activity along with activity for the top Designated Market Areas. Industrial sector participation in ENERGY STAR. Trends in ENERGY STAR certified buildings and plants. Summary By end-of-year 2010, commercial and industrial organizations nearly exceeded activity levels reached throughout all of 2009 for benchmarking and certification. Since June 30, 2010: The number of benchmarked buildings has grown to 185,000 buildings, representing over 21

273

Home Energy Yardstick : ENERGY STAR  

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

Home > Home Improvement > Home Energy Yardstick Home > Home Improvement > Home Energy Yardstick Home Energy Yardstick Assess the energy efficiency of your home and see how it measures up: EPA's Home Energy Yardstick provides a simple assessment of your home's annual energy use compared to similar homes. By answering a few basic questions about your home, you can get: Your home's Home Energy Yardstick score (on a scale of 1 to 10); Insights into how much of your home's energy use is related to heating and cooling versus other everyday uses like appliances, lighting, and hot water; Links to guidance from ENERGY STAR on how to increase your home's score, improve comfort, and lower utility bills; and An estimate of your home's annual carbon emissions. Learn more about how the Home Energy Yardstick works.

274

QUARK MATTER IN MASSIVE COMPACT STARS  

SciTech Connect

The recent observation of the pulsar PSR J1614-2230 with a mass of 1.97 {+-} 0.04 M{sub sun} gives a strong constraint on the quark and nuclear matter equations of state (EoS). We explore the parameter ranges for a parameterized EoS for quark stars. We find that strange stars, made of absolutely stable strange quark matter, comply with the new constraint only if effects from the strong coupling constant and color-superconductivity are taken into account. Hybrid stars, compact stars with a quark matter core and a hadronic outer layer, can be as massive as 2 M{sub sun}, but only for a significantly limited range of parameters. We demonstrate that the appearance of quark matter in massive stars crucially depends on the stiffness of the nuclear matter EoS. We show that the masses of hybrid stars stay below the ones of hadronic and pure quark stars, due to the softening of the EoS at the quark-hadron phase transition.

Weissenborn, Simon; Pagliara, Giuseppe; Schaffner-Bielich, Juergen [Institute for Theoretical Physics, Ruprecht-Karls University, 69120 Heidelberg (Germany); Sagert, Irina [Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824 (United States); Hempel, Matthias [Department of Physics, University of Basel, 4056 Basel (Switzerland)

2011-10-10T23:59:59.000Z

275

Star Formation from Galaxies to Globules  

E-Print Network (OSTI)

The empirical laws of star formation suggest that galactic-scale gravity is involved, but they do not identify the actual triggering mechanisms for clusters in the final stages. Many other triggering processes satisfy the empirical laws too, including turbulence compression and expanding shell collapse. The self-similar nature of the gas and associated young stars suggests that turbulence is more directly involved, but the small scale morphology of gas around most embedded clusters does not look like a random turbulent flow. Most clusters look triggered by other nearby stars. Such a prominent local influence makes it difficult to understand the universality of the Kennicutt and Schmidt laws on galactic scales. A unified view of multi-scale star formation avoids most of these problems. Ambient self-gravity produces spiral arms and drives much of the turbulence that leads to self-similar structures, while localized energy input from existing clusters and field supernovae triggers new clusters in pre-existing clouds. The hierarchical structure in the gas made by turbulence ensures that the triggering time scales with size, giving the Schmidt law over a wide range of scales and the size-duration correlation for young star fields. The efficiency of star formation is determined by the fraction of the gas above a critical density of around 10^5 m(H2)/cc. Star formation is saturated to its largest possible value given the fractal nature of the interstellar medium.

Bruce G. Elmegreen

2002-07-04T23:59:59.000Z

276

Magnitude systems in old star catalogues  

E-Print Network (OSTI)

The current system of stellar magnitudes first introduced by Hipparchus was strictly defined by Norman Robert Pogson in 1856. He based his system on Ptolemys star catalogue Almagest, recorded in about 137 A.D., and defined the magnitude-intensity relationship on a logarithmic scale. Stellar magnitudes observed with the naked eye recorded in seven old star catalogues were analyzed in order to examine the visual magnitude systems. Despite that psychophysists have proposed that humans sensitivities are on a power-law scale, it is shown that the degree of agreement is far better for a logarithmic magnitude than a power-law magnitude. It is also found that light ratios in each star catalogue nearly equal to 2.512, excluding the brightest (1st) and the dimmest (6th and dimmer) stars being unsuitable for the examination. It means that the visual magnitudes in old star catalogues fully agree with Pogsons logarithmic scale. keywords stars: general historical star catalogues stellar magnitude system visual magnitude estimates astronomical photometry 1

Tomoko Fujiwara; Hitoshi Yamaoka

2004-01-01T23:59:59.000Z

277

THE SIZE SCALE OF STAR CLUSTERS  

SciTech Connect

Direct N-body simulations of star clusters in a realistic Milky-Way-like potential are carried out using the code NBODY6. Based on these simulations, a new relationship between scale size and galactocentric distance is derived: the scale size of star clusters is proportional to the hyperbolic tangent of the galactocentric distance. The half-mass radius of star clusters increases systematically with galactocentric distance but levels off when star clusters orbit the galaxy beyond {approx}40 kpc. These simulations show that the half-mass radius of individual star clusters varies significantly as they evolve over a Hubble time, more so for clusters with shorter relaxation times, and remains constant through several relaxation times only in certain situations when expansion driven by the internal dynamics of the star cluster and the influence of the host galaxy tidal field balance each other. Indeed, the radius of a star cluster evolving within the inner 20 kpc of a realistic galactic gravitational potential is severely truncated by tidal interactions and does not remain constant over a Hubble time. Furthermore, the half-mass radius of star clusters measured with present-day observations bears no memory of the original cluster size. Stellar evolution and tidal stripping are the two competing physical mechanisms that determine the present-day size of globular clusters. These simulations also show that extended star clusters can form at large galactocentric distances while remaining fully bound to the host galaxy. There is thus no need to invoke accretion from an external galaxy to explain the presence of extended clusters at large galactocentric distances in a Milky-Way-type galaxy.

Madrid, Juan P.; Hurley, Jarrod R.; Sippel, Anna C. [Center for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122 (Australia)

2012-09-10T23:59:59.000Z

278

OVERVIEW AND STATUS OF THE STAR DETECTOR AT RHIC.  

SciTech Connect

Presented here is the current status of the STAR Detector. STAR is one of the four detectors being constructed at the RHIC collider facility. The STAR detector is scheduled to have its first engineering run with the RHIC beams about six months from the date of this conference. The STAR project is on schedule and expects to recomplete on time.

CHRISTIE,W.B. FOR THE STAR COLLABORATION

1999-01-09T23:59:59.000Z

279

NorthStar Medical Technologies LLC  

National Nuclear Security Administration (NNSA)

Environmental Assessment for Environmental Assessment for NorthStar Medical Technologies LLC Commercial Domestic Production of the Medical Isotope Molybdenum-99 (DOE/EA-1929) Prepared for U.S. Department of Energy National Nuclear Security Administration Defense Nuclear Nonproliferation/ Global Threat Reduction Initiative August 2012 EA for NorthStar Medical Technologies LLC Commercial Domestic Production of the Medical Isotope Mo-99 i COVER SHEET ENVIRONMENTAL ASSESSMENT FOR NORTHSTAR MEDICAL TECHNOLOGIES LLC COMMERCIAL DOMESTIC PRODUCTION OF THE MEDICAL ISOTOPE MOLYBDENUM-99 Proposed Action: The Department of Energy (DOE) National Nuclear Security Administration (NNSA) proposes to provide funding to NorthStar to accelerate the establishment of the commercial production of

280

ENERGY STAR Score for Senior Care Communities  

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

Senior Care Communities in the United States Page 1 Senior Care Communities in the United States Page 1 ENERGY STAR Score for Senior Care Communities in the United States Technical Reference OVERVIEW The ENERGY STAR Score for Senior Care Communities applies to buildings that house and provide care and assistance for elderly residents. The objective of the ENERGY STAR score is to provide a fair assessment of the energy performance of a property relative to its peers, taking into account the climate, weather, and business activities at the property. To identify the aspects of building activity that are significant drivers of energy use and then

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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
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281

ENERGY STAR Guidelines for Energy Management  

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

Guidelines for Energy Guidelines for Energy Management ENERGY STAR is a U.S. Environmental Protection Agency Program helping organizations and individuals fight climate change through superior energy efficiency. Learn more at energystar.gov/buildings. 2 ENERGY STAR Guidelines for Energy Management Overview Continuous improvement of energy performance requires establishing effective energy management practices and processes to guide the energy program. Any organization, regardless of size, function, or mission can develop an effective energy program if they are willing to make the commitment. The US EPA's ENERGY STAR Guidelines for Energy Management provides a proven strategy for creating an energy management program focused on continuous improvement of energy performance. The

282

Creative graphics | ENERGY STAR Buildings & Plants  

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

How can we help you? How can we help you? » Communicate and educate » ENERGY STAR communications toolkit » Motivate with a competition » ENERGY STAR National Building Competition » Competitor resources » Creative graphics Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Build an energy program Improve building and plant performance

283

Energy guides | ENERGY STAR Buildings & Plants  

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

guides guides Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Get started with ENERGY STAR Make the business case Build an energy management program Measure, track, and benchmark Improve energy performance ENERGY STAR industrial partnership Energy guides Energy efficiency and air regulation Plant energy auditing Industrial service and product providers

284

DYNAMICAL CAPTURE BINARY NEUTRON STAR MERGERS  

SciTech Connect

We study dynamical capture binary neutron star mergers as may arise in dense stellar regions such as globular clusters. Using general-relativistic hydrodynamics, we find that these mergers can result in the prompt collapse to a black hole or in the formation of a hypermassive neutron star, depending not only on the neutron star equation of state but also on impact parameter. We also find that these mergers can produce accretion disks of up to a tenth of a solar mass and unbound ejected material of up to a few percent of a solar mass. We comment on the gravitational radiation and electromagnetic transients that these sources may produce.

East, William E.; Pretorius, Frans [Department of Physics, Princeton University, Princeton, NJ 08544 (United States)

2012-11-20T23:59:59.000Z

285

Star-free geodesic languages for groups  

E-Print Network (OSTI)

In this article we show that every group with a finite presentation satisfying one or both of the small cancellation conditions $C'(1/6)$ and $C'(1/4)-T(4)$ has the property that the set of all geodesics (over the same generating set) is a star-free regular language. Star-free regularity of the geodesic set is shown to be dependent on the generating set chosen, even for free groups. We also show that the class of groups whose geodesic sets are star-free with respect to some generating set is closed under taking graph (and hence free and direct) products, and includes all virtually abelian groups.

Hermiller, S; Rees, Sarah

2011-01-01T23:59:59.000Z

286

Lithium abundances in exoplanet-hosts stars  

E-Print Network (OSTI)

Exoplanet-host stars (EHS) are known to present surface chemical abundances different from those of stars without any detected planet (NEHS). EHS are, on the average, overmetallic compared to the Sun. The observations also show that, for cool stars, lithium is more depleted in EHS than in NEHS. The overmetallicity of EHS may be studied in the framework of two different scenarii. We have computed main sequence stellar models with various masses, metallicities and accretion rates. The results show different profiles for the lithium destruction according to the scenario. We compare these results to the spectroscopic observations of lithium.

M. Castro; S. Vauclair; O. Richard; N. C. Santos

2008-03-20T23:59:59.000Z

287

Combustion of a neutron star into a strange quark star: The neutrino signal  

E-Print Network (OSTI)

There are strong indications that the process of conversion of a neutron star into a strange quark star proceeds as a strong deflagration implying that in a few milliseconds almost the whole star is converted. Starting from the three-dimensional hydrodynamic simulations of the combustion process which provide the temperature profiles inside the newly born strange star, we calculate for the first time the neutrino signal that is to be expected if such a conversion process takes place. The neutrino emission is characterized by a luminosity and a duration that is typical for the signal expected from protoneutron stars and represents therefore a powerful source of neutrinos which could be possibly directly detected in case of events occurring close to our Galaxy. We discuss moreover possible connections between the birth of strange stars and explosive phenomena such as supernovae and gamma-ray-bursts.

G. Pagliara; M. Herzog; F. K. Roepke

2013-04-25T23:59:59.000Z

288

Molecular gas and triggered star formation surrounding Wolf-Rayet stars  

E-Print Network (OSTI)

The environments surrounding nine Wolf-Rayet stars were studied in molecular emission. Expanding shells were detected surrounding these WR stars (see left panels of Figure 1). The average masses and radii of the molecular cores surrounding these WR stars anti-correlate with the WR stellar wind velocities (middle panels of Figure 1), indicating the WR stars has great impact on their environments. The number density of Young Stellar Objects (YSOs) is enhanced in the molecular shells at $\\sim$5 arcmin from the central WR star (lower-right panel of Figure 1). Through detailed studies of the molecular shells and YSOs, we find strong evidences of triggered star formation in the fragmented molecular shells (\\cite[Liu et al. 2010]{liu_etal12}

Liu, Tie; Zhang, Huawei

2012-01-01T23:59:59.000Z

289

CFL Manufacturers: ENERGY STAR Letters | Department of Energy  

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

CFL Manufacturers: ENERGY STAR Letters CFL Manufacturers: ENERGY STAR Letters CFL Manufacturers: ENERGY STAR Letters January 25, 2010 DOE issued letters to 25 manufacturers of compact fluorescent lamps (CFLs) involving various models after PEARL Cycle 9 testing indicated that the models do not meet the ENERGY STAR specification and, therefore, are disqualified from the ENERGY STAR Program. When a product is disqualified from the ENERGY STAR Program, all corresponding packaging and supplier's products will be disqualified as well. CFL Manufacturers: ENERGY STAR Letters More Documents & Publications Ex Parte Communication Memo Realizing Building End-Use Efficiency with Ermerging Technologies Identifying Cost-Effective Residential Energy Efficiency Opportunities for the Kauai Island Utility Cooperative

290

Magic Valley Electric Cooperative - ENERGY STAR Builders Program (Texas) |  

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

Magic Valley Electric Cooperative - ENERGY STAR Builders Program Magic Valley Electric Cooperative - ENERGY STAR Builders Program (Texas) Magic Valley Electric Cooperative - ENERGY STAR Builders Program (Texas) < Back Eligibility Construction Savings Category Heating & Cooling Home Weatherization Construction Commercial Weatherization Commercial Heating & Cooling Design & Remodeling Appliances & Electronics Water Heating Program Info State Texas Program Type Utility Rebate Program Rebate Amount ENERGY STAR Home: $150-$600 ENERGY STAR Home with Version 3.0 Checklist: $200 Marathon Water Heater Installation: $150 ENERGY STAR Heat Pump Water Heater: $250 Provider Magic Valley Electric Cooperative Magic Valley Electric Cooperative's (MVEC) ENERGY STAR Builders Program offers a variety of incentives to builders of energy efficiency homes

291

Federal Energy Management Program: Covered Product Category: ENERGY STAR  

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

Covered Product Covered Product Category: ENERGY STAR Displays to someone by E-mail Share Federal Energy Management Program: Covered Product Category: ENERGY STAR Displays on Facebook Tweet about Federal Energy Management Program: Covered Product Category: ENERGY STAR Displays on Twitter Bookmark Federal Energy Management Program: Covered Product Category: ENERGY STAR Displays on Google Bookmark Federal Energy Management Program: Covered Product Category: ENERGY STAR Displays on Delicious Rank Federal Energy Management Program: Covered Product Category: ENERGY STAR Displays on Digg Find More places to share Federal Energy Management Program: Covered Product Category: ENERGY STAR Displays on AddThis.com... Energy-Efficient Products Federal Requirements Covered Product Categories

292

CFL Manufacturers: ENERGY STAR Letters | Department of Energy  

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

CFL Manufacturers: ENERGY STAR Letters CFL Manufacturers: ENERGY STAR Letters CFL Manufacturers: ENERGY STAR Letters January 25, 2010 DOE issued letters to 25 manufacturers of compact fluorescent lamps (CFLs) involving various models after PEARL Cycle 9 testing indicated that the models do not meet the ENERGY STAR specification and, therefore, are disqualified from the ENERGY STAR Program. When a product is disqualified from the ENERGY STAR Program, all corresponding packaging and supplier's products will be disqualified as well. CFL Manufacturers: ENERGY STAR Letters More Documents & Publications Ex Parte Communication Memo Identifying Cost-Effective Residential Energy Efficiency Opportunities for the Kauai Island Utility Cooperative Realizing Building End-Use Efficiency with Ermerging Technologies

293

Variable stars in the Fornax dSph Galaxy. II. Pulsating stars below the horizontal branch  

E-Print Network (OSTI)

We have carried out an intensive survey of the northern region of the Fornax dwarf spheroidal galaxy with the aim of detecting the galaxy's short--period pulsating stars (Pled us to reconstruct the Period-Luminosity relation for short-period pulsating stars. An excellent linear fit, M(V)=-1.83(+/-0.08)-3.65(+/-0.07) log P(fund), was obtained using 153 Delta Scuti and SX Phoenicis stars in a number of different stellar systems.

Ennio Poretti; Gisella Clementini; Enrico V. Held; Claudia Greco; Mario Mateo; Luca Dell'Arciprete; Luca Rizzi; Marco Gullieuszik; Marcella Maio

2008-06-27T23:59:59.000Z

294

The new ENERGY STAR Portfolio Manager | ENERGY STAR Buildings & Plants  

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

The new ENERGY STAR Portfolio Manager The new ENERGY STAR Portfolio Manager Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Learn the benefits Get started Use Portfolio Manager The new ENERGY STAR Portfolio Manager How Portfolio Manager helps you save The benchmarking starter kit Identify your property type Enter data into Portfolio Manager The data quality checker

295

VARIABILITY AND STAR FORMATION IN LEO T, THE LOWEST LUMINOSITY STAR-FORMING GALAXY KNOWN TODAY  

SciTech Connect

We present results from the first combined study of variable stars and star formation history (SFH) of the Milky Way 'ultra-faint' dwarf (UFD) galaxy Leo T, based on F606W and F814W multi-epoch archive observations obtained with the Wide Field Planetary Camera 2 on board the Hubble Space Telescope. We have detected 14 variable stars in the galaxy. They include one fundamental-mode RR Lyrae star and 11 Anomalous Cepheids with periods shorter than 1 day, thus suggesting the occurrence of multiple star formation episodes in this UFD, of which one about 10 Gyr ago produced the RR Lyrae star. A new estimate of the distance to Leo T of 409{sup +29}{sub -27} kpc (distance modulus of 23.06 {+-} 0.15 mag) was derived from the galaxy's RR Lyrae star. Our V, V - I color-magnitude diagram (CMD) of Leo T reaches V {approx} 29 mag and shows features typical of a galaxy in transition between dwarf irregular and dwarf spheroidal types. A quantitative analysis of the SFH, based on the comparison of the observed V, V - I CMD with the expected distribution of stars for different evolutionary scenarios, confirms that Leo T has a complex SFH dominated by two enhanced periods about 1.5 and 9 Gyr ago, respectively. The distribution of stars and gas shows that the galaxy has a fairly asymmetric structure.

Clementini, Gisella; Cignoni, Michele; Ramos, Rodrigo Contreras; Federici, Luciana; Tosi, Monica [INAF, Osservatorio Astronomico di Bologna, I-40127 Bologna (Italy); Ripepi, Vincenzo; Marconi, Marcella; Musella, Ilaria, E-mail: gisella.clementini@oabo.inaf.it, E-mail: rodrigo.contreras@oabo.inaf.it, E-mail: luciana.federici@oabo.inaf.it, E-mail: monica.tosi@oabo.inaf.it, E-mail: michele.cignoni@unibo.it, E-mail: ripepi@na.astro.it, E-mail: marcella@na.astro.it, E-mail: ilaria@na.astro.it [INAF, Osservatorio Astronomico di Capodimonte, I-80131 Napoli (Italy)

2012-09-10T23:59:59.000Z

296

Isotopic Anomalies in CP Stars: Helium, Mercury, Platinum, and Calcium  

E-Print Network (OSTI)

We review the classical observational results for isotopic abundance variations for several elements in CP stars. We concentrate on the "newest" anomaly, in calcium. The cosmically very rare isotope, Ca-48 can rival and even dominate the more common, alpha nuclide, Ca-40. Relevant examples are found in the hot, non-magnetic HgMn stars, and the field horizontal-branch star, Feige 86. The calcium anomaly is also present in cool, magnetic stars, including the notorious HD 101065, Przybylski's star.

C. R. Cowley; S. Hubrig; F. Castelli

2007-11-15T23:59:59.000Z

297

William Fowler and Elements in the Stars  

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

William Fowler and Elements in the Stars Resources with Additional Information William A. Fowler Courtesy AIP Emilio Segrè Visual Archives 'William A. Fowler ... shared the 1983 Nobel Prize in physics for his research into the creation of chemical elements inside stars ... . During his career in nuclear physics and nuclear astrophysics, which spanned more that 60 years, Fowler was primarily concerned with studies of fusion reactions--how the nuclei of lighter chemical elements fuse to create the heavier ones in a process known as nucleosynthesis. In 1957, Fowler coauthored ... the seminal paper "Synthesis of the Elements in the Stars", [which] showed that all of the elements from carbon to uranium could be produced by nuclear processes in stars, starting only with the hydrogen and helium produced in the Big Bang.

298

ENERGY STAR SNAPSHOT … Spring 2009  

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

09 09 Introduction In 2008, leading commercial and industrial organizations outpaced their 2007 efforts to improve energy efficiency and reduce greenhouse gas emissions. Rating activity continued to be strong, particularly for offices and schools; and new organizations partnering with ENERGY STAR nearly tripled. Recognition for improvement and top performance grew significantly in 2008. Almost 3,300 buildings earned the ENERGY STAR, bringing the overall total to more than 6,200 facilities representing over 1 billion square feet. Twenty-seven partners reduced overall energy use to be designated as an ENERGY STAR Leader, 14 for the first time. By the end of the year, a total of 65 partners had demonstrated reaching such milestones. The ENERGY STAR Snapshot provides an at-a-glance summary of the key performance indicators

299

StarTex Power | Open Energy Information  

Open Energy Info (EERE)

StarTex Power StarTex Power Jump to: navigation, search Name StarTex Power Place Texas Utility Id 55875 Utility Location Yes Ownership R NERC ERCOT Yes Activity Retail Marketing Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png No rate schedules available. Average Rates Residential: $0.1150/kWh Commercial: $0.1260/kWh Industrial: $0.1210/kWh References ↑ "EIA Form EIA-861 Final Data File for 2010 - File1_a" Retrieved from "http://en.openei.org/w/index.php?title=StarTex_Power&oldid=411605" Categories: EIA Utility Companies and Aliases Utility Companies

300

Blue Star Energy Services | Open Energy Information  

Open Energy Info (EERE)

BlueStar) BlueStar) Jump to: navigation, search Name Blue Star Energy Services Place Illinois Utility Id 55722 Utility Location Yes Ownership R NERC Location RFC NERC RFC Yes Activity Retail Marketing Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png No rate schedules available. Average Rates Residential: $0.1180/kWh Commercial: $0.0687/kWh References ↑ "EIA Form EIA-861 Final Data File for 2010 - File1_a" Retrieved from "http://en.openei.org/w/index.php?title=Blue_Star_Energy_Services&oldid=409064" Categories: EIA Utility Companies and Aliases

Note: This page contains sample records for the topic "waha lone star" 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

Storm Studies in the Arctic (STAR)  

Science Conference Proceedings (OSTI)

The Storm Studies in the Arctic (STAR) network (20072010) conducted a major meteorological field project from 10 October30 November 2007 and in February 2008, focused on southern Baffin Island, Nunavut, Canadaa region that experiences intense ...

John Hanesiak; Ronald Stewart; David Barber; George Liu; Justin Gilligan; Danielle Desjardins; Robyn Dyck; Shannon Fargey; Klaus Hochheim; Rebekah Martin; Peter Taylor; Sumita Biswas; Mark Gordon; Marna Albarran Melzer; Kent Moore; Robert Field; Carling Hay; Shunli Zhang; Gordon McBean; Walter Strapp; David Hudak; John Scott; Mengistu Wolde; Ron Goodson; Edward Hudson; Gabrielle Gascon; Heather Greene; William Henson; Alex Laplante

2010-01-01T23:59:59.000Z

302

Add ENERGY STAR to Your Course Catalog  

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

good for the bottom line-ENERGY STAR labeled office buildings cost 50 cents less per square foot to operate and have higher occupancy rates and increased asset value. Thirty...

303

Bill Nye (Energy All Stars Presentation)  

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

Bill Nye the Science Guy delivered this presentation on space and the lessons about climate change that can be gleaned from the other planets in our solar system at the Energy All Stars event on...

304

Probing Axions with Radiation from Magnetic Stars  

E-Print Network (OSTI)

Recent experiments suggest that polarized photons may couple significantly to pseudoscalar particles such as axions. We study the possible observational signatures of axion-photon coupling for radiation from magnetic stars, with particular focus on neutron stars. We present general methods for calculating the axion-photon conversion probability during propagation through a varying magnetized vacuum as well as across an inhomogeneous atmosphere. Partial axion-photon conversion may take place in the vacuum region outside the neutron star. Strong axion-photon mixing occurs due to a resonance in the atmosphere, and depending on the axion coupling strength and other parameters, significant axion-photon conversion can take place at the resonance. Such conversions may produce observable effects on the radiation spectra and polarization signals from the star. We also apply our results to axion-photon propagation in the Sun and in magnetic white dwarfs. We find that there is no appreciable conversion of solar axions to photons during the propagation.

Dong Lai; Jeremy Heyl

2006-09-28T23:59:59.000Z

305

Bring Your Green to Work | ENERGY STAR  

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

interactive activities-to encourage your team to save energy in the workplace. Bring Your Green to Work is a national ENERGY STAR campaign encouraging all of us to help improve the...

306

Mayor Antonio Villaraigosa (Energy All Stars Presentation)  

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

Los Angeles Mayor Antonio Villaraigosa delivered this presentation touting the energy efficiency and renewable energy related accomplishments of his city at the Energy All Stars event on January 19...

307

Cohesion Web Interface to EmStar  

E-Print Network (OSTI)

Networked Sensing Cohesion: Web Interface to EmStar SaharSolution: Easy to Use Web Interface Title of Interface:of CGI-based World Wide Web applications. Common Gateway

Sahar Kashef; Jia Ning (Jane) Qu; Karen Weeks

2005-01-01T23:59:59.000Z

308

Sue Tierney (Energy All Stars Presentation)  

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

Sue Tierney delivered this presentation"The Future of Energy: Toward the 21st Century Energy System We Need (With an Eye on the Rear View Mirror)"at the Energy All Stars event on January 19, 2013...

309

STATE AND LOCAL GOVERNMENTS LEVERAGING ENERGY STAR  

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

buildings over 5,000 square feet to earn the ENERGY STAR or be certified under the LEED-NC or Earth Light for Commercial Construction rating systems. It also grants expedited...

310

Blue Star Energy Services | Open Energy Information  

Open Energy Info (EERE)

Blue Star Energy Services Place Illinois Utility Id 55722 Utility Location Yes Ownership R NERC Location RFC NERC RFC Yes Activity Retail Marketing Yes References EIA Form EIA-861...

311

Jennifer Granholm (Energy All Stars Presentation)  

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

Former Michigan Governor Jennifer Granholm delivered this presentation advocating for an energy Race to the Top competition between the states at the Energy All Stars event on January 19, 2013, at...

312

MULTIPLICITY AMONG F-TYPE STARS  

SciTech Connect

As part of a homogeneous all-sky volume-complete sample of half a thousand solar-type stars within 25 pc we present a census for the subset of the 150-mostly F-type stars-in the mass range 1.1 M{sub Sun} {<=} M {<=} 1.7 M{sub Sun} in terms of their observed multiplicities. The major obstacle, as expected, arises from the onset of stellar rotation in this mass range for it continues to support many hidden companions. Yet, a solid increase of the fraction of binary and higher level systems as a function of the primary mass is manifest. There is even the prospect that on account of many companion candidates the single-star fraction may already converge to zero at the transition to the A-type stars.

Fuhrmann, K.; Chini, R., E-mail: klaus@ing.iac.es [Astronomisches Institut, Ruhr-Universitaet Bochum, Universitaetsstrasse 150, D-44801 Bochum (Germany)

2012-12-15T23:59:59.000Z

313

How can we help you? | ENERGY STAR  

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

industrial buildings. Click through these sections to get a broad understanding of why saving energy makes sense, how ENERGY STAR can help, and quick links to help you get...

314

Condensation temperature trends among stars with planets  

E-Print Network (OSTI)

Results from detailed spectroscopic analyses of stars hosting massive planets are employed to search for trends between abundances and condensation temperatures. The elements C, S, Na, Mg, Al, Ca, Sc, Ti, V, Cr, Mn, Fe, Ni and Zn are included in the analysis of 64 stars with planets and 33 comparison stars. No significant trends are evident in the data. This null result suggests that accretion of rocky material onto the photospheres of stars with planets is not the primary explanation for their high metallicities. However, the differences between the solar photospheric and meteoritic abundances do display a weak but significant trend with condensation temperature. This suggests that the metallicity of the sun's envelope has been enriched relative to its interior by about 0.07 dex.

Guillermo Gonzalez

2005-12-08T23:59:59.000Z

315

MagStar Technologies | Open Energy Information  

Open Energy Info (EERE)

Partnership Type Other Relationship LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now MagStar Technologies is a company located in Hopkins, MN....

316

CapStar Health System Feedback Report  

Science Conference Proceedings (OSTI)

... and CapStar's daily briefings are patterned after those of a hotel industry leader. ... results on readmission rates shown in Figure 7.4-5, the utility of the ...

2013-06-09T23:59:59.000Z

317

Forecasting neutron star temperatures: predictability and variability  

E-Print Network (OSTI)

It is now possible to model thermal relaxation of neutron stars after bouts of accretion during which the star is heated out of equilibrium by nuclear reactions in its crust. Major uncertainties in these models can be encapsulated in modest variations of a handful of fudge parameters that change the crustal thermal conductivity, specific heat, and heating rates. Observations of thermal relaxation constrain these fudge parameters and allow us to predict longer term variability in terms of the neutron star core temperature. We demonstrate this explicitly by modeling ongoing thermal relaxation in the neutron star XTE J1701-462. Its future cooling, over the next 5 to 30 years, is strongly constrained and depends mostly on its core temperature, uncertainties in crust physics having essentially been pinned down by fitting to the first three years of observations.

Dany Page; Sanjay Reddy

2013-07-17T23:59:59.000Z

318

Whirlpool: ENERGY STAR Referral (ASD2524VE)  

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

DOE referred the matter of Whirlpool's Amana-brand dishwasher model ASD2524VE to the EPA for appropriate action after DOE testing showed that the model does not meet the ENERGY STAR specification.

319

Home Performance with ENERGY STAR - Webinar Slides  

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

Existing Homes Efficiency - If You Want BetterBuildings - Go with HPwES Home Performance with ENERGY STAR August 5, 2010 Chandler von Schrader, EPA Casey Murphy, ICF Int'l Matthew...

320

Michael Liebreich (Energy All Stars Presentation)  

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

Michael Liebreich, CEO of Bloomberg New Energy Finance, delivered this presentation on the energy economy at the Energy All Stars event on January 19, 2013, at the US Department of Energy in...

Note: This page contains sample records for the topic "waha lone star" 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

NOVI Energy & Honeywell Teaming Profile | ENERGY STAR  

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

my money go? Set and Save with ENERGY STAR Product Finder Rebate Finder Store Locator Energy Savings At Home Energy Savings At Home Improving your home's energy efficiency with...

322

Verify and document your savings | ENERGY STAR  

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

my money go? Set and Save with ENERGY STAR Product Finder Rebate Finder Store Locator Energy Savings At Home Energy Savings At Home Improving your home's energy efficiency with...

323

Give incentives and recognition | ENERGY STAR  

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

my money go? Set and Save with ENERGY STAR Product Finder Rebate Finder Store Locator Energy Savings At Home Energy Savings At Home Improving your home's energy efficiency with...

324

Improvements in industrial energy performance | ENERGY STAR  

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

my money go? Set and Save with ENERGY STAR Product Finder Rebate Finder Store Locator Energy Savings At Home Energy Savings At Home Improving your home's energy efficiency with...

325

Star product algebras of test functions  

E-Print Network (OSTI)

We prove that the Gelfand-Shilov spaces $S^\\beta_\\alpha$ are topological algebras under the Moyal star product if and only if $\\alpha\\ge\\beta$. These spaces of test functions can be used in quantum field theory on noncommutative spacetime. The star product depends continuously in their topology on the noncommutativity parameter. We also prove that the series expansion of the Moyal product is absolutely convergent in $S^\\beta_\\alpha$ if and only if $\\beta<1/2$.

Soloviev, Michael A

2007-01-01T23:59:59.000Z

326

Gas/Star Offsets in Tidal Tails  

E-Print Network (OSTI)

We use numerical simulations to study the development of gas/star offsets in the tidal tails of merging galaxies. These offsets are shown to be a natural consequence of the radially extended HI spatial distribution in disk galaxies, coupled with internal dissipation in the gaseous component driven by the interaction. This mechanism explains the observed gas/star offsets in interacting galaxies without invoking interactions with a hot (unseen) gaseous component.

Mihos, C

2000-01-01T23:59:59.000Z

327

Gas/Star Offsets in Tidal Tails  

E-Print Network (OSTI)

We use numerical simulations to study the development of gas/star offsets in the tidal tails of merging galaxies. These offsets are shown to be a natural consequence of the radially extended HI spatial distribution in disk galaxies, coupled with internal dissipation in the gaseous component driven by the interaction. This mechanism explains the observed gas/star offsets in interacting galaxies without invoking interactions with a hot (unseen) gaseous component.

Chris Mihos

2000-08-09T23:59:59.000Z

328

Xenon in Mercury-Manganese Stars  

E-Print Network (OSTI)

Previous studies of elemental abundances in Mercury-Manganese (HgMn) stars have occasionally reported the presence of lines of the ionized rare noble gas Xe II, especially in a few of the hottest stars with Teff ~ 13000--15000 K. A new study of this element has been undertaken using observations from Lick Observatory's Hamilton Echelle Spectrograph. In this work, the spectrum synthesis program UCLSYN has been used to undertake abundance analysis assuming LTE. We find that in the Smith & Dworetsky sample of HgMn stars, Xe is vastly over-abundant in 21 of 22 HgMn stars studied, by factors of 3.1--4.8 dex. There does not appear to be a significant correlation of Xe abundance with Teff. A comparison sample of normal late B stars shows no sign of Xe II lines that could be detected, consistent with the expected weakness of lines at normal abundance. The main reason for the previous lack of widespread detection in HgMn stars is probably due to the strongest lines being at longer wavelengths than the photographic blue. The lines used in this work were 4603.03A, 4844.33A and 5292.22A.

M. M. Dworetsky; J. L. Persaud; K. Patel

2008-01-16T23:59:59.000Z

329

Superfluidity of $?$ hyperons in neutron stars  

E-Print Network (OSTI)

We study the $^1S_0$ superfluidity of $\\Lambda$ hyperons in neutron star matter and neutron stars. We use the relativistic mean field (RMF) theory to calculate the properties of neutron star matter. In the RMF approach, the meson-hyperon couplings are constrained by reasonable hyperon potentials that include the updated information from recent developments in hypernuclear physics. To examine the $^1S_0$ pairing gap of $\\Lambda$ hyperons, we employ several $\\Lambda\\Lambda$ interactions based on the Nijmegen models and used in double-$\\Lambda$ hypernuclei studies. It is found that the maximal pairing gap obtained is a few tenths of a MeV. The magnitude and the density region of the pairing gap are dependent on the $\\Lambda\\Lambda$ interaction and the treatment of neutron star matter. We calculate neutron star properties and find that whether the $^1S_0 $ superfluidity of $\\Lambda$ hyperons exists in the core of neutron stars mainly depends on the $\\Lambda\\Lambda$ interaction used.

Y. N. Wang; H. Shen

2010-02-01T23:59:59.000Z

330

EPA ENERGY STAR: Tackling Growth in Home Electronics and Small Appliances  

E-Print Network (OSTI)

ICF Consulting. 2003. Energy Star Market Penetration ReportConsulting. . 2004. Energy Star Market Penetration Reportmarket data. Figure 4. ENERGY STAR Market Penetration ENERGY

Sanchez, Marla Christine

2008-01-01T23:59:59.000Z

331

Dark Stars: A New Study of the FIrst Stars in the Universe  

E-Print Network (OSTI)

We have proposed that the first phase of stellar evolution in the history of the Universe may be Dark Stars (DS), powered by dark matter heating rather than by nuclear fusion. Weakly Interacting Massive Particles, which may be their own antipartners, collect inside the first stars and annihilate to produce a heat source that can power the stars. A new stellar phase results, a Dark Star, powered by dark matter annihilation as long as there is dark matter fuel, with lifetimes from millions to billions of years. We find that the first stars are very bright ($\\sim 10^6 L_\\odot$) and cool ($T_{surf} 50,000$K); hence DS should be observationally distinct from standard Pop III stars. Once the dark matter fuel is exhausted, the DS becomes a heavy main sequence star; these stars eventually collapse to form massive black holes that may provide seeds for supermassive black holes observed at early times as well as explanations for recent ARCADE data and for intermediate black holes.

Freese, Katherine; Bodenheimer, Peter; Gondolo, Paolo

2009-01-01T23:59:59.000Z

332

ENERGY STAR portfolio-wide recognition | ENERGY STAR Buildings & Plants  

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

ENERGY STAR portfolio-wide recognition ENERGY STAR portfolio-wide recognition Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Build an energy program Improve building and plant performance Earn the ENERGY STAR and other recognition Earn recognition for your building or plant Earn recognition for your commercial construction project ENERGY STAR portfolio-wide recognition

333

ENERGY STAR sales tools for service and product providers | ENERGY STAR  

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

sales tools for service and product providers sales tools for service and product providers Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can ENERGY STAR help your business? Get started Join ENERGY STAR as a partner ENERGY STAR service & product provider training series Service and product provider's marketing toolkit ENERGY STAR sales tools for service and product providers

334

Neutron Stars and the Cosmological Constant Problem  

E-Print Network (OSTI)

The gravitational aether theory is a modification of general relativity that decouples vacuum energy from gravity, and thus can potentially address the cosmological constant problem. The classical theory is distinguishable from general relativity only in the presence of relativistic pressure (or vorticity). Since the interior of neutron stars has high pressure and as their mass and radius can be measured observationally, they are the perfect laboratory for testing the validity of the aether theory. In this paper, we solve the equations of stellar structure for the gravitational aether theory and find the predicted mass-radius relation of non-rotating neutron stars using two different realistic proposals for the equation of state of nuclear matter. We find that the maximum neutron star mass predicted by the aether theory is 12% - 16% less than the maximum mass predicted by general relativity assuming these two equations of state. We also show that the effect of aether is similar to modifying the equation of state in general relativity. The effective pressure of the neutron star given by the aether theory at a fiducial density differs from the values given by the two nuclear equations of state to an extent that can be constrained using future gravitational wave observations of neutron stars in compact systems. This is a promising way to test the aether theory if further progress is made in constraining the equation of state of nuclear matter in densities above the nuclear saturation density.

Farbod Kamiab; Niayesh Afshordi

2011-04-29T23:59:59.000Z

335

Multiscale Modeling and Applications  

Science Conference Proceedings (OSTI)

Mar 6, 2013 ... Room: Lone Star Salon B Location: Grand Hyatt Session Chair: Yunzhi Wang, The Ohio State University; Darren Hartl, Texas A&M University...

336

March 3-7, 2013 Henry B. Gonzalez Convention Center San ...  

Science Conference Proceedings (OSTI)

Mar 4, 2013 ... Advance Materials & Innovative Solutions for Oil and Gas I. WED. AM. Lone Star Salon A. 178. Materials Challanges in Hostile Environments.

337

Tick Identification and Prevention  

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

to humans. The lone star tick is not believed to transmit the bacteria that causes Lyme disease (Borrelia burgdorferi), but it may be associated with a related bacteria...

338

Ms. Leslie Jones ENERGY STAR Program  

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

June 6, 2012 June 6, 2012 U.S. Environmental Protection Agency 1200 Pennsylvania Avenue, NW Room62023 Washington, DC 20460 Dear Ms. Jones: On October 28, 2011, the United States Depatiment of Energy (DOE) notified Friedrich Air Conditioning Company (Friedrich) that DOE had completed testing of Friedrich room air conditioner models WS12Cl0 and WS13C30 under the ENERGY STAR Testing Pilot Program and confirmed that these models do not meet the ENERGY STAR energy efficiency requirement of9.4 EER. On November 3, 201 I, DOE notified Friedrich that its room air conditioner model USI2C30 does not meet the ENERGY STAR energy efficiency requirement of9.4 EER. In each notice, DOE gave Friedrich twenty days to provide conclusive manufacturing or design evidence or quality assurance information on why DOE testing showed that these models do not

339

TRAN-STAR EXECUTIVE LIMOUSINE COMPANY  

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

TRAN-STAR EXECUTIVE LIMOUSINE COMPANY TRAN-STAR EXECUTIVE LIMOUSINE COMPANY http://www.tranexec.com 20% off published rates for BNL Our reservation center is open 24 hours a day, 365 days a year, so you will always talk to a live agent who has direct contact with our chauffeurs. You can make reservations via phone, website or a simple e-mail to customerservice@tranexec.com once a profile has been established. Our advanced reservation system will track any flight and you can rest assured someone will always be there to meet the arriving passenger, no matter what time the flight arrives. http://www.tranexec.com/TranStarSalesBrochure.pdf These rates are inclusive rates, meaning they include gratuity, taxes....everything. They do not include parking or tolls

340

Christmas burst reveals neutron star collision  

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

Christmas burst reveals neutron star collision Christmas burst reveals neutron star collision Christmas burst reveals neutron star collision Called the Christmas Burst, GRB 101225A was freakishly lengthy and it produced radiation at unusually varying wavelengths. December 1, 2011 Los Alamos National Laboratory sits on top of a once-remote mesa in northern New Mexico with the Jemez mountains as a backdrop to research and innovation covering multi-disciplines from bioscience, sustainable energy sources, to plasma physics and new materials. Los Alamos National Laboratory sits on top of a once-remote mesa in northern New Mexico with the Jemez mountains as a backdrop to research and innovation covering multi-disciplines from bioscience, sustainable energy sources, to plasma physics and new materials. Contact

Note: This page contains sample records for the topic "waha lone star" 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

Energy Star Product Rebates | Department of Energy  

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

Energy Star Product Rebates Energy Star Product Rebates Energy Star Product Rebates < Back Eligibility General Public/Consumer Residential Savings Category Appliances & Electronics Commercial Lighting Lighting Program Info Funding Source New Jersey Societal Benefits Charge (public benefits fund) State New Jersey Program Type State Rebate Program Rebate Amount Lighting: varies Refrigerator: $50 Clothes washers: $50 Provider c/o Honeywell The New Jersey Office of Clean Energy (OCE) offers rebates to state residents who purchase certain energy efficient home appliances. As of April 2, 2013, active rebates exist for energy efficient clothes washers and refrigerators. The program website has a search engine where consumers can look up local retailers offering discounts on compact fluorescent

342

CalStar Products | Open Energy Information  

Open Energy Info (EERE)

CalStar Products CalStar Products Jump to: navigation, search Name CalStar Products Place Newark, California Zip 94560 Product California-based environmentally friendly brick and paving stone manufacturer. Coordinates 44.690435°, -71.951685° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":44.690435,"lon":-71.951685,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

343

Ms. Leslie Jones ENERGY STAR Program  

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

December 21,2010 December 21,2010 U.S. Environmental Protection Agency 1200 Pennsylvania Avenue, NW Room 62023 Washington, DC 20460 Dear Ms. Jones: On November 24, 2010, the United States Department of Energy (DOE) notified Haier that DOE had tested the Haier room air conditioner model ESA3087 as part of the ENERGY STAR Testing Pilot Program, and that, according to Stage I testing, this model exceeded allowable ENERGY STAR energy-efficiency requirements by 18 percent. DOE gave Haier until December 3, 2010, to request additional testing or have this matter referred to the United States Environmental Protection Agency (EPA) for disqualification from the ENERGY STAR program. On December 2, Haier notified DOE that it was in the process of voluntarily removing model

344

Five Star Technologies | Open Energy Information  

Open Energy Info (EERE)

Star Technologies Star Technologies Jump to: navigation, search Name Five Star Technologies Place Independence, Ohio Zip 44131 Sector Solar Product US manufacturer of inks and pastes for the electronics industry; in solar, manufactures silver paste for screen printing PV cells. Coordinates 44.356672°, -91.421315° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":44.356672,"lon":-91.421315,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

345

ENERGY STAR Homes Program | Department of Energy  

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

ENERGY STAR Homes Program ENERGY STAR Homes Program ENERGY STAR Homes Program < Back Eligibility Installer/Contractor Multi-Family Residential Residential Savings Category Heating & Cooling Home Weatherization Construction Commercial Weatherization Commercial Heating & Cooling Design & Remodeling Maximum Rebate Single-Family: $26,000 per unit Multiple Single-Family (townhomes): $17,000 per unit Multi-Family Buildings: $12,000 per unit Program Info Funding Source New Jersey Societal Benefits Charge (public benefits fund) State New Jersey Program Type State Rebate Program Rebate Amount Varies by efficiency level and type of residence Provider New Jersey Clean Energy Program : Note: The Smart Growth requirement for incentive eligibility has been removed in areas affected by Hurricane Sandy, for projects enrolled from

346

STATE AND LOCAL GOVERNMENTS LEVERAGING ENERGY STAR  

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

Federal agencies and state and local governments across the country are taking bold steps to protect the environment and lower energy costs by adopting Federal agencies and state and local governments across the country are taking bold steps to protect the environment and lower energy costs by adopting policies that leverage EPA's ENERGY STAR tools to reduce energy use in commercial buildings, through both required policy measures and voluntary campaigns. This document provides a summary of federal, state, and local efforts that refer to ENERGY STAR tools. Download an interactive copy at www.energystar.gov/government. POLICIES LEVERAGING ENERGY STAR TOOLS Jurisdiction Policy Summary Alabama Executive Order 25 December 2011 By December Fiscal Year 2015, all state departments and agencies will implement energy efficiency measures in order to achieve a 30 percent reduction in energy consumption relative to Fiscal Year 2005

347

Ms. Leslie Jones ENERGY STAR Program  

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

September 20, 2011 September 20, 2011 U.S. Environmental Protection Agency 1200 Pennsylvania Avenue, NW Room 62023 Washington, DC 20460 Dear Ms. Jones: On March 7, 2011, the United States Depmiment of Energy (DOE) notified Baier America Trading, L.L.C. (Baier) that DOE had completed testing of Baier refrigerator model PRTS21SAC* under the ENERGY STAR Verification Testing Pilot Program and confirmed that the model did not meet ENERGY STAR energy efficiency requirements. DOE gave Baier until March 28, 2011, to provide conclusive manufacturing or design evidence or quality assurance information to rebut DOE testing results, which showed that this product did not meet the ENERGY STAR Program's energy efficiency requirement. Baier responded to DOE in a letter dated March 22, 2011, contending that the results of

348

ENERGY STAR Score for Data Centers  

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

Data Centers in the United States Page 1 Data Centers in the United States Page 1 ENERGY STAR Score for Data Centers in the United States Technical Reference OVERVIEW The ENERGY STAR Score for Data Centers applies to spaces specifically designed and equipped to meet the needs of high density computing equipment such as server racks, used for data storage and processing. The objective of the ENERGY STAR score is to provide a fair assessment of the energy performance of a property relative to its peers, taking into account the climate, weather, and business activities at the property. To identify the aspects of building activity that are significant drivers of energy use and then normalize for those factors, a statistical analysis of

349

ENERGY STAR Success Story: Staples, Inc.  

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

STAR Success Story: STAR Success Story: Staples, Inc. Staples, the world's largest office products company, has been an energy management and environmental leader in the retail industry for several years. Staples first partnered with the U.S. Environmental Protection Agency's (EPA) Green Lights Program, the predecessor to ENERGY STAR, and in 1999, won the Green Lights Partner of the Year recognition. Staples also has the distinction of being one of the first retailers to benchmark its entire portfolio of over 1,500 retail stores and 200 distribution centers. Even as the company's building portfolio has grown, with total square footage increasing by over 6 percent in just the past three years, Staples has reduced its building portfolio-wide energy usage by more than 11.4%, and recently became the first retailer

350

DarkStar VI | Open Energy Information  

Open Energy Info (EERE)

DarkStar VI DarkStar VI Jump to: navigation, search Name DarkStar VI Place Collinsville, Illinois Zip 62234-2022 Sector Services Product Manufacturer of biodiesel processing equipment and supplier of accessories, information and services. Coordinates 36.720014°, -79.91284° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":36.720014,"lon":-79.91284,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

351

Abundance analysis of planetary host stars  

E-Print Network (OSTI)

We present atmospheric parameters and Fe abundances derived for the majority of dwarf stars (north of -30 degrees declination) which are up to now known to host extrasolar planets. High-resolution spectra have been obtained with the Sandiford Echelle spectrograph on the 2.1m telescope at the University of Texas McDonald Observatory. We have used the same model atmospheres, atomic data and equivalent width modeling program for the analysis of all stars. Abundances have been derived differentially to the Sun, using a solar spectrum obtained with Callisto as the reflector with the same instrumentation. A similar analysis has been performed for a sample of stars for which radial velocity data exclude the presence of a close-in giant planetary companion. The results are compared to the recent studies found in the literature.

U. Heiter; R. E. Luck

2002-09-27T23:59:59.000Z

352

Results from STAR Beam Energy Scan Program  

E-Print Network (OSTI)

Results from the Beam Energy Scan (BES) program conducted recently by STAR experiment at RHIC are presented. The data from Phase-I of the BES program collected in Au+Au collisions at center-of-mass energies (\\sqrt{s_{NN}}) of 7.7, 11.5, 19.6, 27, and 39 GeV cover a wide range of baryon chemical potential ?\\mu_B (100-400 MeV) in the QCD phase diagram. Several STAR results from the BES Phase-I related to "turn-o?ff" of strongly inter- acting quark-gluon plasma (sQGP) signatures and signals of QCD phase boundary are reported. In addition to this, an outlook is presented for the future BES Phase-II program and a possible ?fixed target program at STAR.

Michal Sumbera

2013-01-30T23:59:59.000Z

353

Stability windows for proto-quark stars  

E-Print Network (OSTI)

We investigate the existence of possible stable strange matter and related stability windows at finite temperature for different models that are generally applied to describe quark stars, namely, the quark-mass density dependent model, the MIT bag model and the Nambu-Jona-Lasinio model. We emphasize that, although the limits for stable strange matter depend on a comparison with the ground state of 56Fe, which is a zero temperature state, the quantity that has to be used in the search for strange matter in proto-quark stars is the free energy and we analyze stability windows up to temperatures of the order of 40 MeV. The effects of strong magnetic fields on stability windows are computed and the resulting mass-radius relations for different stages of the proto-quark star are analyzed.

V. Dexheimer; J. R. Torres; D. P. Menezes

2013-03-20T23:59:59.000Z

354

Carbon Enhanced Metal-Poor Stars. I. Chemical Compositions of 26 Stars  

E-Print Network (OSTI)

The chemical compositions of 26 metal-poor stars that exhibit strong CH and/or C2 molecular bands are determined based on high-resolution spectroscopy. We define carbon-enhanced stars taking account of the carbon abundance ratio ([C/Fe]) and the evolutionary status. Twenty two stars in our sample satisfy our modified definition for Carbon-Enhanced Metal-Poor (CEMP) stars. In addition, we measure Na abundances for nine other carbon-enhanced stars for which abundances of other elements have been previously reported. Combining our new sample with the results of previous work, we investigate the abundance and evolutionary status of a total of 64 CEMP stars. In this paper, we separate the carbon-enhanced objects into Ba-rich and Ba-normal objects, and discuss on (1) the metallicity distributions, (2) the correlation between Ba and C (and C+N) abundances, (3) C abundance distributions, (3) the distributions of evolutionary status, and (5) Na abundances. The implications of these results on the origins of carbon in CEMP stars are discussed.

Wako Aoki; Timothy C. Beers; Norbert Christlieb; John E. Norris; Sean G. Ryan; Stelios Tsangarides

2006-09-26T23:59:59.000Z

355

Probing the Birth of Super Star Clusters: Implications for Massive Star Formation  

E-Print Network (OSTI)

Super Star Clusters are one of the most extreme star forming environments in the universe, and the most massive and dense of these may be proto globular clusters. Like individual massive stars, the earliest stages of super star cluster evolution are deeply obscured, and therefore our knowledge about their birth environments is currently very incomplete. However, the study of natal super star clusters has become somewhat of a cottage industry in recent years, and the sample of such objects has been growing rapidly with high-quality long-wavelength data now available from a number of observatories. The natal super star clusters identified in thermal-infrared and radio observations represent the youngest stage of massive star cluster evolution yet observed. Their properties appear to be similar to those of ultracompact HII regions in the Milky Way, but scaled up in total mass and luminosity. I will overview what we think we know about these objects based on existing observations, discuss their relationship to ultracompact HII regions, present new models of their spectral energy distributions based on 3-D simulations, and outline some of the most significant gaps in our current understanding.

Kelsey E. Johnson

2005-06-21T23:59:59.000Z

356

ENERGY STAR Enterprise Storage Draft Specification Framework  

E-Print Network (OSTI)

This document describes the key building blocks that form the basis for every ENERGY STAR specification; these items are intended to provide the framework around which the EPA can develop an effective energy efficiency program for Enterprise Storage. The principal objectives for this ENERGY STAR specification are threefold: (1) to encourage widespread adoption of appropriate hardware and software strategies to improve energy efficiency in enterprise storage systems, (2) to provide purchasers with the means to identify the most energy efficient enterprise storage solutions for their specific end-use application, and (3) to provide tools and information to designers and mangers looking to improve the efficiency of data center operations. The purpose of each building block is provided under the subheadings below, along with EPAs preliminary thoughts on how each may ultimately be incorporated into the Version 1.0 Enterprise Storage specification. At the end of each section are a series of questions aimed at generating discussion about the proposed approach. Please note that this document is not intended to be a comprehensive review of the ENERGY STAR perspective on enterprise storage, rather it serves as a starting point for EPAs specification development efforts. Stakeholders are encouraged to provide feedback on the specific concepts and definitions presented in this document, and are also welcome to submit comments of a more general nature. Communication between EPA and industry stakeholders is critical to the success of the ENERGY STAR program, especially in this early stage of the specification development process. Any and all creative suggestions for improvements to the basic ENERGY STAR approach outlined in this document will be considered for inclusion in subsequent draft and final specifications. ENERGY STAR representatives are available for additional technical discussions with interested parties at any time during the specification development process. Please contact Steve Pantano, ICF International, at

unknown authors

2009-01-01T23:59:59.000Z

357

R modes of slowly pulsating B stars  

E-Print Network (OSTI)

We examine pulsational stability of low $m$ $r$ modes in SPB stars by calculating fully nonadiabatic oscillations of uniformly rotating stars, where $m$ is an integer representing the azimuthal wave number around the rotation axis. $R$ modes are rotationally induced, non-axisymmetric, oscillation modes, whose oscillation frequency strongly depends on the rotation frequency $\\Omega$ of the star. They are conveniently classified by using two integer indices $m$ and $l^\\prime\\ge |m|$ that define the asymptotic oscillation frequency $2m\\Omega/[l^\\prime(l^\\prime+1)]$ in the limit of $\\Omega\\to 0$. We find low $m$, high radial order, odd $r$ modes with $l^\\prime=m$ in SPB stars are excited by the same iron opacity bump mechanism that excites low frequency $g$ modes of the variables, when the rotation frequency $\\Omega$ is sufficiently high. No even $r$ modes with low $m$ are found to be pulsationally unstable. Since the surface pattern of the temperature perturbation of odd modes is antisymmetric about the equator of the star, observed photometric amplitudes caused by the unstable odd $r$ modes with $l^\\prime=m$ are strongly dependent on the inclination angle between the axis of rotation and the line of sight. Applying the wave-meanflow interaction formalism to nonadiabatic $r$ modes in rapidly rotating SPB models, we find that because of the $r\\phi$ component of the Reynolds stress and the radial transport of the eddy fluctuation of density in the rotating star, the surface rotation is accelerated by the forcing due to the low $l^\\prime=m$ unstable $r$ modes.

Umin Lee

2005-09-12T23:59:59.000Z

358

Support for ENERGY STAR Enforcement | Department of Energy  

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

Support for ENERGY STAR Enforcement Support for ENERGY STAR Enforcement Support for ENERGY STAR Enforcement By offering a means for consumers to buy products more energy-efficient than required by law, ENERGY STAR has huge potential to save money for consumers by offering buyers more options in energy-efficient products. In a new initiative, the Department is expanding verification and supporting enforcement of ENERGY STAR to preserve the viability and effectiveness of the ENERGY STAR program. Through independent testing, we are working to verify manufacturer certifications of the efficiency or energy use ratings of their appliances and ensuring manufacturers provide the increased energy and cost savings they advertise. Learn more about ENERGY STAR and DOE's ENERGY STAR Verification Testing

359

Buying an Appliance this Holiday Season? ENERGY STAR Products...  

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

an Appliance this Holiday Season? ENERGY STAR Products will Save You Money and Energy All Year Buying an Appliance this Holiday Season? ENERGY STAR Products will Save You Money...

360

Designed to earn the ENERGY STAR: eligibility rules and requirements...  

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

ENERGY STAR project archive Step 6: Market your project as Designed to Earn the ENERGY STAR Step 7: Commission the building Step 8: Work with the building owner to complete the...

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


361

DOE Energy Star Testing Reveals Inefficient ASKO Dishwasher | Department of  

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

Energy Star Testing Reveals Inefficient ASKO Dishwasher Energy Star Testing Reveals Inefficient ASKO Dishwasher DOE Energy Star Testing Reveals Inefficient ASKO Dishwasher June 1, 2010 - 2:07pm Addthis DOE testing in support of the Energy Star program has revealed that an ASKO dishwasher (model D5122XXLB), which the company had claimed was Energy Star compliant, consumes more energy than permitted by the Energy Star program. Test results for the ASKO model at issue show that, when tested in accordance with DOE's test procedure, it consumed 12 percent more energy than the Energy Star requirement. Based on this testing, DOE is referring ASKO Model D5122XXLB to the U.S. Environmental Protection Agency for appropriate action with respect to the Energy Star program. DOE's testing revealed that dishwasher model D5122XXLB also may not meet

362

The Biggest, Brightest Star of Energy Efficiency | Department...  

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

The Biggest, Brightest Star of Energy Efficiency The Biggest, Brightest Star of Energy Efficiency February 22, 2013 - 1:30pm Addthis Learn more about daylighting with this Energy...

363

Haier: ENERGY STAR Referral (PRTS21SAC*) | Department of Energy  

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

Haier: ENERGY STAR Referral (PRTS21SAC*) Haier: ENERGY STAR Referral (PRTS21SAC*) September 20, 2011 DOE referred the matter of Haier refrigerator model PRTS21SAC* to the U.S....

364

Emerson: ENERGY STAR Referral (CR289E) | Department of Energy  

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

Emerson: ENERGY STAR Referral (CR289E) Emerson: ENERGY STAR Referral (CR289E) May 6, 2013 DOE referred the matter of Emerson-brand refrigerator, model CR289E, to the U.S....

365

Haier: ENERGY STAR Referral (ESA408J) | Department of Energy  

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

ESA408J) Haier: ENERGY STAR Referral (ESA408J) March 4, 2011 DOE referred Haier room air conditioner model ESA408J to EPA, brand manager of the ENERGY STAR program, for appropriate...

366

Haier: ENERGY STAR Referral (DE45EK) | Department of Energy  

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

ENERGY STAR Referral (DE45EK) Haier: ENERGY STAR Referral (DE45EK) May 10, 2013 DOE referred the matter of Haier-brand dehumidifier, model DE45EK, to the U.S. Environmental...

367

ASKO: ENERGY STAR Referral (D5253XXL) | Department of Energy  

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

ASKO: ENERGY STAR Referral (D5253XXL) ASKO: ENERGY STAR Referral (D5253XXL) December 22, 2011 DOE referred the matter of ASKO dishwasher model D5253XXL to the EPA for appropriate...

368

Dayton: ENERGY STAR Referral (5NTX1) | Department of Energy  

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

Dayton: ENERGY STAR Referral (5NTX1) Dayton: ENERGY STAR Referral (5NTX1) December 22, 2011 DOE referred the matter of Dayton-brand refrigerator-freezer model 5NTX1, which is...

369

Edgestar: ENERGY STAR Referral (DEP400EW) | Department of Energy  

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

Edgestar: ENERGY STAR Referral (DEP400EW) Edgestar: ENERGY STAR Referral (DEP400EW) June 7, 2013 DOE referred the matter of Edgestar-brand dehumidifier, model DEP400EW, to the U.S....

370

Midea: ENERGY STAR Referral (MWF-08CR) | Department of Energy  

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

Midea: ENERGY STAR Referral (MWF-08CR) Midea: ENERGY STAR Referral (MWF-08CR) March 4, 2011 DOE referred the matter of Westpointe-brand room air conditioner model MWF-08CR, which...

371

Haier: ENERGY STAR Referral (ESA3087) | Department of Energy  

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

ESA3087) Haier: ENERGY STAR Referral (ESA3087) December 21, 2010 DOE referred Haier room air conditioner model ESA3087 to EPA, brand manager of the ENERGY STAR program, for...

372

Sunpentown: ENERGY STAR Referral (RF-330SS) | Department of Energy  

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

ENERGY STAR Referral (RF-330SS) Sunpentown: ENERGY STAR Referral (RF-330SS) May 10, 2013 DOE referred the matter of Sunpentown-brand refrigerator, model RF-330SS, manufactured by...

373

Danby: ENERGY STAR Referral (DAC10507EE) | Department of Energy  

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

Danby: ENERGY STAR Referral (DAC10507EE) Danby: ENERGY STAR Referral (DAC10507EE) November 4, 2010 DOE referred the matter of Danby room air conditioner model DAC10507EE to the EPA...

374

Samsung: ENERGY STAR Referral (RF26VAB) | Department of Energy  

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

Samsung: ENERGY STAR Referral (RF26VAB) Samsung: ENERGY STAR Referral (RF26VAB) March 16, 2010 DOE referred the matter of Samsung refrigerator-freezer model RF26VAB to the U.S....

375

Summit: ENERGY STAR Referral (F1112BL) | Department of Energy  

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

Summit: ENERGY STAR Referral (F1112BL) Summit: ENERGY STAR Referral (F1112BL) June 20, 2013 DOE referred the matter of Summit-brand refrigerator-freezer model F1112BL, which is...

376

ASKO: ENERGY STAR Referral (D5122XXLB) | Department of Energy  

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

ASKO: ENERGY STAR Referral (D5122XXLB) ASKO: ENERGY STAR Referral (D5122XXLB) May 27, 2010 DOE referred the matter of ASKO dishwasher model D5122XXLB to the EPA for appropriate...

377

Intirion: ENERGY STAR Referral (MFRA-4GF) | Department of Energy  

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

Intirion: ENERGY STAR Referral (MFRA-4GF) Intirion: ENERGY STAR Referral (MFRA-4GF) August 14, 2012 DOE referred the matter of Intirion refrigerator model MFRA-4GF to the U.S....

378

ALS Stars in New Video from California Academy of Sciences  

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

ALS Stars in New Video from California Academy of Sciences ALS Stars in New Video from California Academy of Sciences Print Tuesday, 30 October 2012 13:51 cal academy of sciences...

379

ENERGY STAR Focus on Energy Efficiency in Corn Refining | ENERGY...  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

380

ENERGY STAR Focus on Energy Efficiency in Glass Manufacturing...  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

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


381

ENERGY STAR Energy Performance Indicators for plants | ENERGY...  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

382

ENERGY STAR Focus on Energy Efficiency in Pharmaceutical Manufacturing...  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

383

ENERGY STAR Focus on Energy Efficiency in Food Processing | ENERGY...  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

384

ENERGY STAR Focus on Energy Efficiency in Cement Manufacturing...  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

385

ENERGY STAR Focus on Energy Efficiency in Petroleum Refining...  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

386

ENERGY STAR Focus on Energy Efficiency in Ready Mix Concrete...  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

387

ENERGY STAR Focus on Energy Efficiency in Dairy Processing |...  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

388

ENERGY STAR Residential Water Heaters to Save Americans Up to...  

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

ENERGY STAR Residential Water Heaters to Save Americans Up to 823 Million in the Next Five Years ENERGY STAR Residential Water Heaters to Save Americans Up to 823 Million in the...

389

ENERGY STAR Snapshot December with Data through December 2012  

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

Buildings Sector Spring 2013 Snapshot data runs through December 31, 2012. The ENERGY STAR Snapshot provides an at-a-glance summary of the latest national ENERGY STAR metrics to...

390

ENERGY STAR Score for Residence Halls/Dormitories  

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

Residence HallsDormitories in the United States Page 1 ENERGY STAR Score for Residence HallsDormitories in the United States Technical Reference OVERVIEW The ENERGY STAR Score...

391

ENERGY STAR Score for Supermarkets/Grocery Stores  

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

SupermarketsGrocery Stores in the United States Page 1 ENERGY STAR Score for SupermarketsGrocery Stores in the United States Technical Reference OVERVIEW The ENERGY STAR Score...

392

ENERGY STAR Focus on Energy Efficiency in Metalcasting | ENERGY...  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

393

ENERGY STAR Focus on Energy Efficiency in Petrochemical Manufacturing...  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

394

ENERGY STAR Focus on Energy Efficiency in Motor Vehicle Manufacturing...  

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

Skip to main content ENERGY STAR logo Skip directly to page content Facebook Twitter YouTube Our Blog Search Search Energy Efficient Products Energy Efficient Products ENERGY STAR...

395

The FourStar Infrared Camera  

E-Print Network (OSTI)

The FourStar infrared camera is a 1.0-2.5 micron (JHKs) near infrared camera for the Magellan Baade 6.5m telescope at Las Campanas Observatory (Chile). It is being built by Carnegie Observatories and the Instrument Development Group at Johns Hopkins and is scheduled for completion in 2009. The instrument uses four Teledyne HAWAII-2RG arrays that produce a 10.9 x 10.9 arcmin field of view. The outstanding seeing at the Las Campanas site coupled with FourStar's high sensitivity and large field of view will enable many new survey and targeted science programs.

S. E. Persson; Robert Barkhouser; Christoph Birk; Randy Hammond; Albert Harding; E. R. Koch; J. L. Marshall; Patrick J. McCarthy; David Murphy; Joe Orndorff; Gregg Scharfstein; Stephen A. Shectman; Stephen Smee; Alan Uomoto

2008-07-24T23:59:59.000Z

396

Auto-correlation of Binary stars  

E-Print Network (OSTI)

Speckle interferometric technique is used to record a series of short exposure images of several close binary stars with sub-arcsecond separation through a narrow band filter centred at H$\\alpha$ at the Cassegrain focus of the 2.34 meter Vainu Bappu telescope (VBT), situated at Vainu Bappu Observatory (VBO), Kavalur. The auto-correlation method is developed under Image Reduction Analysis Facility (IRAF). Wiener filter is included in the programme to eliminate spurious high frequency contributions; a few sets of data provide the optimised results. The auto-correlated image of these stars gives the separation of the binary components.

S. K. Saha; D. Maitra

2001-06-07T23:59:59.000Z

397

[Your Industrial Plant] Earns the ENERGY STAR | ENERGY STAR Buildings &  

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

Industrial Plant] Earns the ENERGY STAR Industrial Plant] Earns the ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In This Section Campaigns Commercial building design Communications resources Energy management guidance Financial resources Portfolio Manager Products and purchasing Recognition Research and reports Service and product provider (SPP) resources Success stories

398

ENERGY STAR Focus on Energy Efficiency in Food Processing | ENERGY STAR  

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

Food Processing Food Processing Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Get started with ENERGY STAR Make the business case Build an energy management program Measure, track, and benchmark Tools for benchmarking energy management practices Tools for tracking and benchmarking facility energy performance ENERGY STAR Energy Performance Indicators for plants

399

DataTrends: ENERGY STAR Certification | ENERGY STAR Buildings & Plants  

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

ENERGY STAR Certification ENERGY STAR Certification Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In This Section Campaigns Commercial building design Communications resources Energy management guidance Financial resources Portfolio Manager Products and purchasing Recognition Research and reports Service and product provider (SPP) resources Success stories Target Finder

400

Build Your Business with ENERGY STAR | ENERGY STAR Buildings & Plants  

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

Build Your Business with ENERGY STAR Build Your Business with ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In This Section Campaigns Commercial building design Communications resources Energy management guidance Financial resources Portfolio Manager Products and purchasing Recognition Research and reports Service and product provider (SPP) resources Success stories

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


401

Conversion of neutron stars to strange stars as the central engine of gamma-ray bursts  

E-Print Network (OSTI)

We study the conversion of a neutron star to a strange star as a possible energy source for gamma-ray bursts. We use different recent models for the equation of state of neutron star matter and strange quark matter. We show that the total amount of energy liberated in the conversion is in the range of (1-4) 10^{53} ergs (one order of magnitude larger than previous estimates) and is in agreement with the energy required to power gamma-ray burst sources at cosmological distances.

Ignazio Bombaci; Bhaskar Datta

2000-01-27T23:59:59.000Z

402

Gamma-Ray Bursts and Afterglows from Rotating Strange Stars and Neutron Stars  

E-Print Network (OSTI)

We here discuss a new model of $\\gamma$-ray bursts (GRBs) based on differentially rotating strange stars. Strange stars in this model and differentially rotating neutron stars in the Klu\\'zniak-Ruderman model can produce extremely relativistic, variable fireballs required by GRBs and then become millisecond pulsars. The effect of such pulsars on expansion of the postburst fireballs through magnetic dipole radiation is studied. We show that these two models can explain naturally not only various features of GRBs but also light curves of afterglows.

Z. G. Dai; T. Lu

1998-10-21T23:59:59.000Z

403

Stars in Photographic Emulsions Initiated by Deuterons Part II. Theoretical  

E-Print Network (OSTI)

SSiFIED ( The theory of high energy nuclear stars depends onto construct a theory of high energy nuclear reactions.

Horning, Wendell

2010-01-01T23:59:59.000Z

404

Putting Energy into Stewardship: ENERGY STAR Guide for Congregations...  

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

business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators...

405

ENERGY STAR Challenge for Industry: BTU QuickConverter | ENERGY...  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

406

ENERGY STAR Score for Hospitals (General Medical and Surgical...  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

407

ENERGY STAR Partner of the Year Award for your organization ...  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

408

ENERGY STAR Success Story: Kohl's Department Stores | ENERGY...  

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

Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program...

409

ENERGY STAR Commercial Buildings College Course: Week 4 Sample...  

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

and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program...

410

ENERGY STAR Commercial Buildings College Course: About the Course...  

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

and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program...

411

ENERGY STAR Commercial Buildings College Course: Week 3 Sample...  

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

and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program...

412

Make the business case | ENERGY STAR Buildings & Plants  

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

Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and...

413

Energy star compliant voice over internet protocol (VoIP) telecommunications network including energy star compliant VoIP devices  

DOE Patents (OSTI)

A Voice over Internet Protocol (VoIP) communications system, a method of managing a communications network in such a system and a program product therefore. The system/network includes an ENERGY STAR (E-star) aware softswitch and E-star compliant communications devices at system endpoints. The E-star aware softswitch allows E-star compliant communications devices to enter and remain in power saving mode. The E-star aware softswitch spools messages and forwards only selected messages (e.g., calls) to the devices in power saving mode. When the E-star compliant communications devices exit power saving mode, the E-star aware softswitch forwards spooled messages.

Kouchri, Farrokh Mohammadzadeh

2012-11-06T23:59:59.000Z

414

Generalized equation of state for cold superfluid neutron stars  

SciTech Connect

Mature neutron stars are expected to contain various kinds of superfluids in their interiors. Modeling such stars requires the knowledge of the mutual entrainment couplings between the different condensates. We present a unified equation of state describing the different regions of a neutron star with superfluid neutrons and superconducting protons in its core.

Chamel, N.; Goriely, S. [Institut d'Astronomie et d'Astrophysique, Universite Libre de Bruxelles, B-1050 Brussels (Belgium); Pearson, J. M. [Departement de Physique, Universite de Montreal, Montreal (Quebec), H3C 3J7 (Canada)

2011-09-21T23:59:59.000Z

415

THE Be STAR SPECTRA (BeSS) DATABASE  

Science Conference Proceedings (OSTI)

Be stars vary on many timescales, from hours to decades. A long time base of observations to analyze certain phenomena in these stars is therefore necessary. Collecting all existing and future Be star spectra into one database has thus emerged as an important tool for the Be star community. Moreover, for statistical studies, it is useful to have centralized information on all known Be stars via an up-to-date catalog. These two goals are what the Be Star Spectra (BeSS, http://basebe.obspm.fr) database proposes to achieve. The database contains an as-complete-as-possible catalog of known Be stars with stellar parameters, as well as spectra of Be stars from all origins (any wavelength, any epoch, any resolution, etc.). It currently contains over 54,000 spectra of more than 600 different Be stars among the {approx}2000 Be stars in the catalog. A user can access and query this database to retrieve information on Be stars or spectra. Registered members can also upload spectra to enrich the database. Spectra obtained by professional as well as amateur astronomers are individually validated in terms of format and science before being included in BeSS. In this paper, we present the database itself as well as examples of the use of BeSS data in terms of statistics and the study of individual stars.

Neiner, C.; De Batz, B. [LESIA, UMR 8109 du CNRS, Observatoire de Paris, UPMC, Univ. Paris Diderot, 92195 Meudon Cedex (France); Cochard, F. [Shelyak Instruments, Les Roussets, 38420 Revel (France); Floquet, M.; Mekkas, A. [GEPI, UMR 8111 du CNRS, Observatoire de Paris, Univ. Paris Diderot, 92195 Meudon Cedex (France); Desnoux, V., E-mail: coralie.neiner@obspm.fr [ARAS, Astronomical Ring for Access to Spectroscopy (Country Unknown)

2011-11-15T23:59:59.000Z

416

ENERGY STAR Jeopardy History Facts Universities Products Other  

E-Print Network (OSTI)

ENERGY STAR Jeopardy History Facts Universities Products Other 10 10 10 10 10 20 20 20 20 20 30 30 30 30 30 40 40 40 40 40 50 50 50 50 50 #12;In what year did ENERGY STAR start? A)2002 B)2008 C)1992 D)1999 #12;Answer: C) 1992! In 1992 the US Environmental Protection Agency (EPA) introduced ENERGY STAR

Brownstone, Rob

417

Property types eligible to receive a 1-100 ENERGY STAR score | ENERGY STAR  

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

Identify your property type Identify your property type » Property types eligible to receive a 1-100 ENERGY STAR score Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Learn the benefits Get started Use Portfolio Manager The new ENERGY STAR Portfolio Manager How Portfolio Manager helps you save The benchmarking starter kit Identify your property type Property types eligible to receive a 1-100 ENERGY STAR score

418

Eligibility criteria for the 1-100 ENERGY STAR score | ENERGY STAR  

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

Eligibility criteria for the 1-100 ENERGY STAR score Eligibility criteria for the 1-100 ENERGY STAR score Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Learn the benefits Get started Use Portfolio Manager The new ENERGY STAR Portfolio Manager How Portfolio Manager helps you save The benchmarking starter kit Identify your property type Enter data into Portfolio Manager The data quality checker

419

Kenmore: ENERGY STAR Referral (253.16582104)  

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

DOE referred the matter of Kenmore-brand freezer model 253.16582104, which is manufactured by Electrolux Major Appliances North America ("Electrolux"), to the EPA for appropriate action after DOE testing raised issues regarding whether model 253.16582104 was properly qualified as an ENERGY STAR model.

420

DayStar Technologies | Open Energy Information  

Open Energy Info (EERE)

DayStar Technologies DayStar Technologies Jump to: navigation, search Logo: DayStar Technologies Name DayStar Technologies Address 2972 Stender Way Place Santa Clara, California Zip 95054 Sector Solar Product Manufacturer of low-cost, high performance, CIGS thin film photovoltaic products Year founded 1997 Number of employees 51-200 Phone number 408-582-7100 Website http://www.daystartech.com/ Coordinates 37.375996°, -121.970815° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":37.375996,"lon":-121.970815,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

Note: This page contains sample records for the topic "waha lone star" 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

Silver Star Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Silver Star Wind Farm Silver Star Wind Farm Jump to: navigation, search Name Silver Star Wind Farm Facility Silver Star Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner BP Alternative Energy/Clipper Developer BP Alternative Energy/Clipper Energy Purchaser Market Location Eastland and Erath Counties TX Coordinates 32.332058°, -98.466783° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":32.332058,"lon":-98.466783,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

422

Gluon Polarization and Jet Production at STAR  

Science Conference Proceedings (OSTI)

I will discuss the most recent measurements of the inclusive jet longitudinal spin asymmetry A LL in polarized proton?proton collisions. STAR collected its largest data sample thus far 4.7? pb ?1 of integrated luminosity at an average beam polarization of ?57%

Pibero Djawotho; the STAR Collaboration

2009-01-01T23:59:59.000Z

423

Solar-like oscillations in cluster stars  

E-Print Network (OSTI)

We present a brief overview of the history of attempts to obtain a clear detection of solar-like oscillations in cluster stars, and discuss the results on the first clear detection, which was made by the Kepler Asteroseismic Science Consortium (KASC) Working Group 2.

Stello, D; Bedding, T R; Brogaard, K; Bruntt, H; Chaplin, W J; Christensen-Dalsgaard, J; Demarque, P; Elsworth, Y P; Garca, R A; Gilliland, R L; Hekker, S; Huber, D; Karoff, C; Kjeldsen, H; Lebreton, Y; Mathur, S; Meibom, S; Zakowicz, J Molenda-\\; Noels, A; Roxburgh, I W; Aguirre, V S; Sterken, C; Szab, R

2010-01-01T23:59:59.000Z

424

Current Status of Transverse Spin at STAR  

E-Print Network (OSTI)

The origins of the proton spin remain an area of active investigation. The Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Lab uniquely provides polarized proton data at high center of mass energies. STAR has previously reported large transverse single spin asymmetries for inclusive neutral pion production in the forward direction at square root of s of 200 GeV, measured with a modular Pb-glass calorimeter called the "Forward Pion Detector" (FPD). Beginning in 2008 (Run 8), STAR's forward calorimetry was significantly enhanced with the commissioning of the "Forward Meson Spectrometer" (FMS), which has full azimuthal coverage in the pseudo-rapidity range 2.5 to 4.2. This detector has extended asymmetry measurements to higher transverse momentum, and its large areal coverage enables measurements of higher mass resonances and "jet-like" correlations. STAR also provides excellent tracking and full azimuthal electromagnetic calorimeter coverage at mid-rapidity, which facilitates analyses of spin-dependent jet structure. Here we review recent transverse spin measurements with the STAR detector and also present an update on some existing analyses.

Andrew Gordon for the STAR Collaboration

2010-07-29T23:59:59.000Z

425

Star Formation from Galaxies to Globules  

E-Print Network (OSTI)

The empirical laws of star formation suggest that galactic-scale gravity is involved, but they do not identify the actual triggering mechanisms for clusters in the final stages. Many other triggering processes satisfy the empirical laws too, including turbulence compression and expanding shell collapse. The self-similar nature of the gas and associated young stars suggests that turbulence is more directly involved, but the small scale morphology of gas around most embedded clusters does not look like a random turbulent flow. Most clusters look triggered by other nearby stars. Such a prominent local influence makes it difficult to understand the universality of the Kennicutt and Schmidt laws on galactic scales. A unified view of multi-scale star formation avoids most of these problems. Ambient self-gravity produces spiral arms and drives much of the turbulence that leads to self-similar structures, while localized energy input from existing clusters and field supernovae triggers new clusters in pre-existing cl...

Elmegreen, B G

2002-01-01T23:59:59.000Z

426

Singularity-free dark energy star  

E-Print Network (OSTI)

We propose a model for an anisotropic dark energy star where we assume that the radial pressure exerted on the system due to the presence of dark energy is proportional to the isotropic perfect fluid matter density. We discuss various physical features of our model and show that the model satisfies all the regularity conditions and stable as well as singularity-free.

Farook Rahaman; Anil Kumar Yadav; Saibal Ray; Raju Maulick; Ranjan Sharma

2011-02-07T23:59:59.000Z

427

The chemical composition of the Orion star forming region: stars, gas and dust  

E-Print Network (OSTI)

We present a summary of main results from the studies performed in the series of papers "The chemical composition of the Orion star forming region". We reinvestigate the chemical composition of B-type stars in the Orion OB1 association by means of state-of-the-art stellar atmosphere codes, atomic models and techniques, and compare the resulting abundances with those obtained from the emission line spectra of the Orion nebula (M42), and recent determinations of the Solar chemical composition.

Simn-Daz, S; Przybilla, N; Stasi?ska, G

2010-01-01T23:59:59.000Z

428

Kurucz model energy distributions: a comparison with real stars. II. Metal-deficient stars  

E-Print Network (OSTI)

Energy distributions of synthetic spectra for Kurucz model atmospheres are compared with observed energy distributions of metal-deficient stars of the blue horizontal-branch (BHB), F-G-K subdwarf (SD) and G-K giant (MDG) types. The best coincidence of the synthetic and observed energy curves is found for BHB stars. The largest differences are found in the ultraviolet wavelengths for subdwarfs and cool MDGs. The influence of errors of effective temperatures, gravities and metallicities is estimated.

V. Straizys; R. Lazauskaite; G. Valiauga

2002-12-04T23:59:59.000Z

429

THE STAR FORMATION HISTORY OF M32  

SciTech Connect

We use deep Hubble Space Telescope Advanced Camera for Surveys/High Resolution Channel observations of a field within M32 (F1) and an M31 background field (F2) to determine the star formation history (SFH) of M32 from its resolved stellar population. We find that 2-5 Gyr old stars contribute {approx}40% {+-} 17% of M32's mass, while {approx}55% {+-} 21% of M32's mass comes from stars older than 5 Gyr. The mass-weighted mean age and metallicity of M32 at F1 are (Age) = 6.8 {+-} 1.5 Gyr and ([M/H]) = -0.01 {+-} 0.08 dex. The SFH additionally indicates the presence of young (<2 Gyr old), metal-poor ([M/H] {approx} -0.7) stars, suggesting that blue straggler stars contribute {approx}2% of the mass at F1; the remaining {approx}3% of the mass is in young metal-rich stars. Line-strength indices computed from the SFH imply a light-weighted mean age and metallicity of 4.9 Gyr and [M/H] = -0.12 dex, and single stellar population-equivalent parameters of 2.9 {+-} 0.2 Gyr and [M/H] = 0.02 {+-} 0.01 dex at F1 ({approx}2.7 r{sub e} ). This contradicts spectroscopic studies that show a steep age gradient from M32's center to 1 r{sub e} . The inferred SFH of the M31 background field F2 reveals that the majority of its stars are old, with {approx}95% of its mass already acquired 5-14 Gyr ago. It is composed of two dominant populations; {approx}30% {+-} 7.5% of its mass is in a 5-8 Gyr old population, and {approx}65% {+-} 9% of the mass is in an 8-14 Gyr old population. The mass-weighted mean age and metallicity of F2 are (Age) = 9.2 {+-} 1.2 Gyr and ([M/H]) = -0.10 {+-} 0.10 dex, respectively. Our results suggest that the inner disk and spheroid populations of M31 are indistinguishable from those of the outer disk and spheroid. Assuming the mean age of M31's disk at F2 ({approx}1 disk scale length) to be {approx}5-9 Gyr, our results agree with an inside-out disk formation scenario for M31's disk.

Monachesi, Antonela; Trager, Scott C. [Kapteyn Astronomical Institute, P.O. Box 800, 9700 AV Groningen (Netherlands); Lauer, Tod R.; Mighell, Kenneth J. [National Optical Astronomy Observatory, P.O. Box 26732, Tucson, AZ 85726 (United States); Hidalgo, Sebastian L. [Instituto de Astrofisica de Canarias, Via Lactea s/n, E-38200 La Laguna, Tenerife (Spain); Freedman, Wendy; Dressler, Alan [The Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Grillmair, Carl, E-mail: antonela@umich.edu [Spitzer Science Center, 1200 East California Boulevard, Pasadena, CA 91125 (United States)

2012-01-20T23:59:59.000Z

430

Gamma Ray Bursts from delayed collapse of neutron stars to quark matter stars  

E-Print Network (OSTI)

We propose a model to explain how a Gamma Rays Burst can take place days or years after a supernova explosion. Our model is based on the conversion of a pure hadronic star (neutron star) into a star made at least in part of deconfined quark matter. The conversion process can be delayed if the surface tension at the interface between hadronic and deconfined-quark-matter phases is taken into account. The nucleation time (i.e. the time to form a critical-size drop of quark matter) can be extremely long if the mass of the star is small. Via mass accretion the nucleation time can be dramaticaly reduced and the star is finally converted into the stable configuration. A huge amount of energy, of the order of 10$^{52}$--10$^{53}$ erg, is released during the conversion process and can produce a powerful Gamma Ray Burst. The delay between the supernova explosion generating the metastable neutron star and the new collapse can explain the delay proposed in GRB990705 and in GRB011211.

Z. Berezhiani; I. Bombaci; A. Drago; F. Frontera; A. Lavagno

2002-09-13T23:59:59.000Z

431

Passive load follow analysis of the STAR-LM and STAR-H2 systems.  

E-Print Network (OSTI)

A steady-state model for the calculation of temperature and pressure distributions, and heat and work balance for the STAR-LM and the STAR-H2 systems was developed. The STAR-LM system is designed for electricity production and consists of the lead cooled reactor on natural circulation and the supercritical carbon dioxide Brayton cycle. The STAR-H2 system uses the same reactor which is coupled to the hydrogen production plant, the Brayton cycle, and the water desalination plant. The Brayton cycle produces electricity for the on-site needs. Realistic modules for each system component were developed. The model also performs design calculations for the turbine and compressors for the CO2 Brayton cycle. The model was used to optimize the performance of the entire system as well as every system component. The size of each component was calculated. For the 400 MWt reactor power the STAR-LM produces 174.4 MWe (44% efficiency) and the STAR-H2 system produces 7450 kg H2/hr. The steady state model was used to conduct quasi-static passive load follow analysis. The control strategy was developed for each system; no control action on the reactor is required. As a main safety criterion, the peak cladding temperature is used. It was demonstrated that this temperature remains below the safety limit during both normal operation and load follow.

Moisseytsev, Anton

2003-12-01T23:59:59.000Z

432

Climate change and buildings | ENERGY STAR Buildings & Plants  

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

Climate change and buildings Climate change and buildings Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Find out who's partnered with ENERGY STAR Become an ENERGY STAR partner Find ENERGY STAR certified buildings and plants ENERGY STAR certification Featured research and reports Facts and stats Climate change and buildings Climate change and buildings

433

Thermal evolution of rotating strange stars in color superconductivity phase  

E-Print Network (OSTI)

Under the combination effect of the recommencement heating due to spin-down of strange stars and the heat perseveration due to weak conduct heat of the crust, the Cooper pair breaking and formation(PBF) in color superconduction quark matter arises. We investigated the cooling of the strange stars with a crust in color superconductivity phase including both decomfinement heating and PBF process. We find that deconfinement heating can delay the thermal evolution of strange stars and the PBF process suppresses the early temperature rise of the stars. The cooling strange stars behave within the brightness constraint of young compact objects when the color superconductivity gap is small enough.

X. P. Zheng; X. Zhou; Y. W. Yu

2006-07-04T23:59:59.000Z

434

Gravitational field energy contribution to the neutron star mass  

E-Print Network (OSTI)

Neutron stars are discussed as laboratories of physics of strong gravitational fields. The mass of a neutron star is split into matter energy and gravitational field energy contributions. The energy of the gravitational field of neutron stars is calculated with three different approaches which give the same result. It is found that up to one half of the gravitational mass of maximum mass neutron stars is comprised by the gravitational field energy. Results are shown for a number of realistic equations of state of neutron star matter.

M. Dyrda; B. Kinasiewicz; M. Kutschera; A. Szmaglinski

2006-01-16T23:59:59.000Z

435

ENERGY STAR Test Procedures and Verification | Department of Energy  

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

ENERGY STAR » ENERGY STAR Test ENERGY STAR » ENERGY STAR Test Procedures and Verification ENERGY STAR Test Procedures and Verification The Department of Energy (DOE) is the lead agency in the development and revision of all test procedures for products in the ENERGY STAR® program, including those products that are also subject to DOE's Energy Conservation Standards program. As specifications are updated and new products or metrics are added to the ENERGY STAR program, DOE is responsible for developing and revising methods, responding to stakeholder comments, and answering any testing-related questions that arise as a result of the procedures being utilized. To simplify the process for interested parties, more information on the test procedure development for ENERGY STAR products can be found on each of

436

Two ENERGY STAR Products Fail Testing | Department of Energy  

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

Two ENERGY STAR Products Fail Testing Two ENERGY STAR Products Fail Testing Two ENERGY STAR Products Fail Testing August 9, 2011 - 4:42pm Addthis DOE testing has identified two additional models of home appliances that do not meet the ENERGY STAR Program's energy efficiency requirements. A refrigerator manufactured by the Perlick Corporation and a room air conditioner manufactured by Electrolux Home Products, Inc. were selected for testing as part of the DOE's ENERGY STAR Verification Testing Pilot Program. DOE testing revealed that Electrolux air conditioner (model FRA256ST2) and Perlick refrigerator (model HP48RO-S), both of which claimed ENERGY STAR ratings, do not meet the ENERGY STAR requirements. Multiple test results for the Electrolux model show that, when tested in accordance with DOE's

437

Ms. Leslie Jones ENERGY STAR Program  

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

July 7, 2011 July 7, 2011 U.S. Environmental Protection Agency 1200 Pennsylvania Avenue NW Room62023 Washington, DC 20460 Dear Ms. Jones: Electrolux Home Products, Inc. (Electro lux) room air conditioner model FRA256ST2 was selected for testing as part of the U.S. Department of Energy's (DOE) ENERGY STAR® Verification Testing Pilot Program. DOE's initial testing, performed on a unit of this model, indicated that it may not meet ENERGY STAR requirements. After testing three additional units of this model, and finding that each fell short of the minimum standard of9.4 EER, DOE asked Electrolux to provide conclusive manufacturing or design evidence or quality assurance information on why this product should be viewed as meeting the ENERGY STAR Program's energy efficiency

438

Star Energy Systems | Open Energy Information  

Open Energy Info (EERE)

Star Energy Systems Star Energy Systems Place Ahmedabad, Gujarat, India Zip 380 009 Sector Solar Product Solar PV product distributor. Coordinates 26.93077°, 80.66416° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":26.93077,"lon":80.66416,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

439

Star Point Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Point Wind Farm Point Wind Farm Jump to: navigation, search Name Star Point Wind Farm Facility Star Point Wind Farm Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Iberdrola Renewables Developer Iberdrola Renewables Energy Purchaser Modesto Irrigation District Location Near Moro OR Coordinates 45.474734°, -120.704412° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":45.474734,"lon":-120.704412,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

440

Star, Idaho: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Star, Idaho: Energy Resources Star, Idaho: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 43.6921071°, -116.4934631° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":43.6921071,"lon":-116.4934631,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

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441

Green Star Energy LLC | Open Energy Information  

Open Energy Info (EERE)

Star Energy LLC Star Energy LLC Place Houston, Texas Zip 77002 Product Houston-based producer of sugar cane processed ethanol, with additional electricity generation activities from agricultural waste. Coordinates 29.76045°, -95.369784° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":29.76045,"lon":-95.369784,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

442

A SECOND NEUTRON STAR IN M4?  

SciTech Connect

We show that the optical counterpart of the X-ray source CX 1 in M4 is a {approx}20th magnitude star, located in the color-magnitude diagram on (or very close to) the main sequence of the cluster, and exhibiting sinusoidal variations of the flux. We find the X-ray flux to be also periodically variable, with X-ray and optical minima coinciding. Stability of the optical light curve, lack of UV-excess, and unrealistic mean density resulting from period-density relation for semidetached systems speak against the original identification of CX 1 as a cataclysmic variable. We argue that the X-ray active component of this system is a neutron star (probably a millisecond pulsar).

Kaluzny, J.; Rozanska, A.; Rozyczka, M.; Krzeminski, W. [Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw (Poland); Thompson, Ian B. [Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101 (United States)

2012-05-01T23:59:59.000Z

443

Carbon stars in the IRTS survey  

E-Print Network (OSTI)

We have identified 139 cool carbon stars in the near-infrared spectro-photometric survey of the InfraRed Telescope in Space (IRTS) from the conspicuous presence of molecular absorption bands at 1.8, 3.1 and 3.8 microns. Among them 14 are new, bright (K ~ 4.0-7.0), carbon stars. We find a trend relating the 3.1 microns band strength to the K-L' color index, which is known to correlate with mass-loss rate. This could be an effect of a relation between the depth of the 3.1 microns feature and the degree of development of the extended stellar atmosphere where dust starts to form.

T. Le Bertre; M. Tanaka; I. Yamamura; H. Murakami; D. J. MacConnell

2004-12-13T23:59:59.000Z

444

METALLICITY GRADIENTS OF THICK DISK DWARF STARS  

Science Conference Proceedings (OSTI)

We examine the metallicity distribution of the Galactic thick disk using F, G, and K dwarf stars selected from the Sloan Digital Sky Survey, Data Release 8. Using the large sample of dwarf stars with proper motions and spectroscopically determined stellar parameters, metallicity gradients in the radial direction for various heights above the Galactic plane and in the vertical direction for various radial distances from the Galaxy center have been found. In particular, we find a vertical metallicity gradient of -0.113 {+-} 0.010 (-0.125 {+-} 0.008) dex kpc{sup -1} using an isochrone (photometric) distance determination in the range 1 kpc solar neighborhood. Metallicity gradients in the thin and thick disks are important probes into possible formation scenarios for our Galaxy and a consistent picture is beginning to emerge from results using large spectroscopic surveys, such as the ones presented here.

Carrell, Kenneth; Chen Yuqin; Zhao Gang, E-mail: carrell@nao.cas.cn [Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 (China)

2012-12-01T23:59:59.000Z

445

NLTE wind models for SMC stars  

E-Print Network (OSTI)

We study stellar wind properties of selected late O stars in the Small Magellanic Cloud (SMC). We calculate NLTE line-driven wind models for these stars and compare predicted wind parameters with observed values. We found satisfactory agreement between theoretical and observed terminal velocities. On the other hand, predicted and observed mass-loss rates are in a good agreement only for higher mass-loss rates. For mass-loss rates lower than approximately 10^{-7} M_sun / year we found large discrepancy between theoretical and observed values. We propose a new explanation of this effect based on dynamical decoupling of some atoms. Finally, we study the dependence of wind terminal velocities and mass-loss rates on metallicity.

Jiri Krticka

2005-09-15T23:59:59.000Z

446

A Neutron Star in F-sharp  

E-Print Network (OSTI)

In this short introductory commentary on the paper (Hessels et al 2006, Science, 311, 1901) reporting the discovery of the shortest spin period millisecond pulsar (MSP) Ter5-ad in the globular cluster Terzan 5, I also point out a new explanation for possible minimum spin periods, P, of MSPs without requiring gravitational radiation (or other) slow-down torques. If the accretion of matter required to spinup a MSP also reduces (buries) the neutron star (NS) magnetic field, B, as commonly believed, an inverse correlation between neutron star mass, M, and B is expected together with a positive correlation between P and B. Both are suggested for the 4 MSPs with NS mass measures reported (Latimer and Prakash 2004, Science, 304, 536) to have tested when a timing solution is found. If confirmed, the highest spin frequency NSs do not pulse simply because their B fields are too low.

Jonathan E. Grindlay

2006-05-04T23:59:59.000Z

447

Isocurvature Fluctuations Induce Early Star Formation  

E-Print Network (OSTI)

The early reionisation of the Universe inferred from the WMAP polarisation results, if confirmed, poses a problem for the hypothesis that scale-invariant adiabatic density fluctuations account for large-scale structure and galaxy formation. One can only generate the required amount of early star formation if extreme assumptions are made about the efficiency and nature of early reionisation. We develop an alternative hypothesis that invokes an additional component of a non-scale-free isocurvature power spectrum together with the scale-free adiabatic power spectrum for inflation-motivated primordial density fluctuations. Such a component is constrained by the Lyman alpha forest observations, can account for the small-scale power required by spectroscopic gravitational lensing, and yields a source of early star formation that can reionise the universe at z~20 yet becomes an inefficient source of ionizing photons by z~10, thereby allowing the conventional adiabatic fluctuation component to reproduce the late thermal history of the intergalactic medium.

Naoshi Sugiyama; Saleem Zaroubi; Joseph Silk

2003-10-21T23:59:59.000Z

448

Binary central stars of planetary nebulae  

E-Print Network (OSTI)

Abstract. Only a handful of binary central stars of planetary nebulae (PNe) are known today, due to the difficulty of detecting their companions. Preliminary results from radial velocity surveys, however, seem to indicate that binarity plays a fundamental, rather than marginal role in the evolution of PNe and that the close binary fraction might be much larger than the currently known value of 10-15%. In this review, we list all the known binary central stars, giving an updated census of their numbers and selected characteristics. A review is also given of the techniques used to detect binaries as well as selected characteristics of related stellar classes which might provide constraints (or additional puzzles) to the theory of PN evolution. Finally, we will formulate the conjecture that all PNe derive from binary interactions and suggest that this is not inconsistent with our current knowledge. 1.

Orsola De Marco

2006-01-01T23:59:59.000Z

449

A NEW CEMP-s RR LYRAE STAR  

SciTech Connect

We show that SDSS J170733.93+585059.7 (hereafter SDSS J1707+58), previously identified by Aoki and collaborators as a carbon-enhanced metal-poor star (with s-process-element enhancements, CEMP-s), on the assumption that it is a main-sequence turnoff star, is the RR Lyrae star VIII-14 identified by the Lick Astrograph Survey. Revised abundances for SDSS J1707+58 are [Fe/H] = -2.92, [C/Fe] = +2.79, and [Ba/Fe] = +2.83. It is thus one of the most metal-poor RR Lyrae stars known, and has more extreme [C/Fe] and [Ba/Fe] than the only other RR Lyrae star known to have a CEMP-s spectrum (TY Gru). Both stars are Oosterhoff II stars with prograde kinematics, in contrast to stars with [C/Fe] < + 0.7, such as KP Cyg and UY CrB, which are disk stars. Twelve other RR Lyrae stars with [C/Fe] {>=}+0.7 are presented as CEMP candidates for further study.

Kinman, T. D.; Beers, Timothy C. [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States); Aoki, Wako [National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588 (Japan); Brown, Warren R. [Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138 (United States)

2012-08-10T23:59:59.000Z

450

Evolution of emission line activity in intermediate mass young stars  

E-Print Network (OSTI)

We present optical spectra of 45 intermediate mass Herbig Ae/Be stars. Together with the multi-epoch spectroscopic and photometric data compiled for a large sample of these stars and ages estimated for individual stars by using pre-main sequence evolutionary tracks, we have studied the evolution of emission line activity in them. We find that, on average, the H_alpha emission line strength decreases with increasing stellar age in HAeBe stars, indicating that the accretion activity gradually declines during the PMS phase. This would hint at a relatively long-lived (a few Myr) process being responsible for the cessation of accretion in Herbig Ae/Be stars. We also find that the accretion activity in these stars drops substantially by ~ 3 Myr. This is comparable to the timescale in which most intermediate mass stars are thought to lose their inner disks, suggesting that inner disks in intermediate mass stars are dissipated rapidly after the accretion activity has fallen below a certain level. We, further find a relatively tight correlation between strength of the emission line and near-infrared excess due to inner disks in HAeBe stars, indicating that the disks around Herbig Ae/Be stars cannot be entirely passive. We suggest that this correlation can be understood within the frame work of the puffed-up inner rim disk models if the radiation from the accretion shock is also responsible for the disk heating.

P. Manoj; H. C. Bhatt; G. Maheswar; S. Muneer

2006-08-25T23:59:59.000Z

451

Forming a Primordial Star in a Relic HII Region  

DOE Green Energy (OSTI)

There has been considerable theoretical debate over whether photoionization and supernova feedback from the first Population III stars facilitate or suppress the formation of the next generation of stars. We present results from an Eulerian adaptive mesh refinement simulation demonstrating the formation of a primordial star within a region ionized by an earlier nearby star. Despite the higher temperatures of the ionized gas and its flow out of the dark matter potential wells, this second star formed within 23 million years of its neighbor's death. The enhanced electron fraction within the HII region catalyzes rapid molecular hydrogen formation that leads to faster cooling in the subsequent star forming halos than in the first halos. This ''second generation'' primordial protostar has a much lower accretion rate because, unlike the first protostar, it forms in a rotationally supported disk of {approx} 10-100 M{center_dot}. In contrast to unpreprocessed regions, such configurations may allow binaries or multiple systems of lower mass stars to form. These first high resolution calculations offer insight into the impact of feedback upon subsequent populations of stars and clearly demonstrate how primordial chemistry promotes the formation of subsequent generations of stars even in the presence of the entropy injected by the first stars into the IGM.

O'Shea, Brian

2005-04-12T23:59:59.000Z

452

Tight LMC massive star clusters R 127 and R 128  

E-Print Network (OSTI)

We study the Large Magellanic Cloud (LMC) star clusters R 127 and R 128 using imaging and spectroscopy obtained at the ESO NTT telescope. An advanced image restoration technique allows us to resolve these two clusters into at least 14 and 33 stars respectively and obtain their photometry. In particular, we show that the core of R 127 is composed of at least four stars and identify the Luminous Blue Variable (LBV) component. The closest neighbor of the LBV (star #8) is 1".5 away. Moreover, from medium dispersion spectroscopy we determine the spectral types for 19 stars in and near both clusters, and in particular present the first spatially resolved observation of the second brightest component of the R 127 cluster (star #3) situated 3".3 from the LBV. By comparing with evolutionary models we also look into the stellar ages. The oldest stars of the cluster are ~ 6-8 Myr old, whereas the most massive star of the region (#7), formed ~ 3 Myr ago as an 80 solar mass star, has turned into an LBV, the ``R 127'' star.

M. Heydari-Malayeri; F. Meynadier; Nolan R. Walborn

2003-01-15T23:59:59.000Z

453

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

SciTech Connect

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

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

2012-12-10T23:59:59.000Z

454

Coronal Abundances in Orion Nebula Cluster Stars  

E-Print Network (OSTI)

Following the Chandra Orion Ultradeep Project (COUP) observation, we have studied the chemical composition of the hot plasma in a sample of 146 X-ray bright pre-main sequence stars in the Orion Nebula Cluster. We report measurements of individual element abundances for a subsample of 86 slightly-absorbed and bright X-ray sources, using low resolution X-ray spectra obtained from the Chandra ACIS instrument. The X-ray emission originates from a plasma with temperatures and elemental abundances very similar to those of active coronae in older stars. A clear pattern of abundances vs. First Ionization Potential (FIP) is evident if solar photospheric abundances are assumed as reference. The results are validated by extensive simulations. The observed abundance distributions are compatible with a single pattern of abundances for all stars, although a weak dependence on flare loop size may be present. The abundance of calcium is the only one which appears to vary substantially between stars, but this quantity is affected by relatively large uncertainties. The ensemble properties of the X-ray bright COUP sources confirm that the iron in the emitting plasma is underabundant with respect to both the solar composition and to the average stellar photospheric values. Comparison of the present plasma abundances with those of the stellar photospheres and those of the gaseous component of the nebula, indicates a good agreement for all the other elements with available measurements, and in particular for the high-FIP elements (Ne, Ar, O, and S) and for the low-FIP element Si. We conclude that there is evidence of a significant chemical fractionation effect only for iron, which appears to be depleted by a factor 1.5--3 with respect to the stellar composition.

A. Maggio; E. Flaccomio; F. Favata; G. Micela; S. Sciortino; E. D. Feigelson; K. V. Getman

2007-03-16T23:59:59.000Z

455

Cooling of Neutron Stars. Hadronic Model  

E-Print Network (OSTI)

We study the cooling of isolated neutron stars. The main cooling regulators are introduced: EoS, thermal transport, heat capacity, neutrino and photon emissivity, superfluid nucleon gaps. Neutrino emissivity includes main processes. A strong impact of medium effects on the cooling rates is demonstrated. With taking into account of medium effects in reaction rates and in nucleon superfluid gaps modern experimental data can be well explained.

D. Blaschke; H. Grigorian; D. N. Voskresensky

2004-03-07T23:59:59.000Z

456

Energy Star Concepts for Highway Vehicles  

Science Conference Proceedings (OSTI)

The authors of this report, under the sponsorship of the U.S. Department of Energy (DOE) Office of Energy Efficiency and Renewable Energy (EERE) Weatherization and Intergovernmental Program, have investigated the possible application of Energy Star ratings to passenger cars and light trucks. This study establishes a framework for formulating and evaluating Energy Star rating methods that is comprised of energy- and environmental-based metrics, potential vehicle classification systems, vehicle technology factors, and vehicle selection criteria. The study tests several concepts and Energy Star rating methods using model-year 2000 vehicle data--a spreadsheet model has been developed to facilitate these analyses. This study tests two primary types of rating systems: (1) an outcome-based system that rates vehicles based on fuel economy, GHG emissions, and oil use and (2) a technology-based system that rates vehicles based on the energy-saving technologies they use. Rating methods were evaluated based on their ability to select vehicles with high fuel economy, low GHG emissions, and low oil use while preserving a full range of service (size and acceleration) and body style choice. This study concludes that an Energy Star rating for passenger cars and light trucks is feasible and that several methods could be used to achieve reasonable tradeoffs between low energy use and emissions and diversity in size, performance, and body type. It also shows that methods that consider only fuel economy, GHG emissions, or oil use will not select a diverse mix of vehicles. Finally, analyses suggest that methods that encourage the use of technology only, may result in increases in acceleration power and weight rather than reductions in oil use and GHG emissions and improvements in fuel economy.

Greene, D.L.

2003-06-24T23:59:59.000Z

457

Asteroseismology of DAV White Dwarf Stars  

DOE Green Energy (OSTI)

The author reviews the seismological structural determinations of ZZ Ceti stars done to date, and supplement these with additional preliminary determinations of his own. He compares the constraints on the hydrogen layer mass to see what trends emerge and also determines if the observed hydrogen layer masses are consistent with proposed theories. He then looks ahead to the prospects of further DAV white dwarf seismology.

Bradley, Paul A.

1997-12-31T23:59:59.000Z

458

Radiation Pressure in Massive Star Formation  

E-Print Network (OSTI)

Stars with masses of >~ 20 solar masses have short Kelvin times that enable them to reach the main sequence while still accreting from their natal clouds. The resulting nuclear burning produces a huge luminosity and a correspondingly large radiation pressure force on dust grains in the accreting gas. This effect may limit the upper mass of stars that can form by accretion. Indeed, simulations and analytic calculations to date have been unable to resolve the mystery of how stars of 50 solar masses and up form. We present two new ideas to solve the radiation pressure problem. First, we use three-dimensional radiation hydrodynamic adaptive mesh refinement simulations to study the collapse of massive cores. We find that in three dimensions a configuration in which radiation holds up an infalling envelope is Rayleigh-Taylor unstable, leading radiation driven bubbles to collapse and accretion to continue. We also present Monte Carlo radiative transfer calculations showing that the cavities created by protostellar winds provides a valve that allow radiation to escape the accreting envelope, further reducing the ability of radiation pressure to inhibit accretion.

Mark R. Krumholz; Richard I. Klein; Christopher F. McKee

2005-10-14T23:59:59.000Z

459

Molecular cloud regulated star formation in galaxies  

E-Print Network (OSTI)

We describe a numerical implementation of star formation in disk galaxies, in which the conversion of cooling gas to stars in the multiphase interstellar medium is governed by the rate at which molecular clouds are formed and destroyed. In the model, clouds form from thermally unstable ambient gas and get destroyed by feedback from massive stars and thermal conduction. Feedback in the ambient phase cycles gas into a hot galactic fountain or wind. We model the ambient gas hydrodynamically using smoothed particle hydrodynamics (SPH). However, we cannot resolve the Jeans mass in the cold and dense molecular gas and, therefore, represent the cloud phase with ballistic particles that coagulate when colliding. We show that this naturally produces a multiphase medium with cold clouds, a warm disk, hot supernova bubbles and a hot, tenuous halo. Our implementation of this model is based on the Gadget N-Body code. We illustrate the model by evolving an isolated Milky Way-like galaxy and study the properties of a disk formed in a rotating spherical collapse. Many observed properties of disk galaxies are reproduced well, including the molecular cloud mass spectrum, the molecular fraction as a function of radius, the Schmidt law, the stellar density profile and the appearance of a galactic fountain.

C. M. Booth; T. Theuns; T. Okamoto

2007-01-30T23:59:59.000Z

460

Multiperiodic RR Lyrae Stars in Omega Centauri  

E-Print Network (OSTI)

We have conducted a systematic search for multiperiodic pulsations in the RR Lyrae-type stars of the galactic globular cluster Omega Cen. Secondary periodicities close to the primary pulsation frequency have been detected in 17 out of 70 studied fundamental mode (RRab) pulsators and in 35 out of 81 overtone (RRc) pulsators. Because of the observed period ratios, these newly detected periodicities must correspond to nonradial modes. Their beating with the primary radial pulsation leads to a slow amplitude and phase modulation, commonly referred to as the Blazhko effect. The incidence rate of Blazhko modulation in Omega Cen RRab stars (24 +/- 5%) is similar to that observed in the Galactic Bulge. In the case of Omega Cen RRc stars, the incidence rate of Blazhko effect is exceptionally high (38 +/- 5%), more than 3 times higher than in any other studied population. In addition to Blazhko variables, we have also identified two RR Lyr variables exhibiting first overtone/second overtone double-mode pulsations, and a triple-mode High Amplitude Delta Scuti variable.

P. Moskalik; A. Olech

2008-06-30T23:59:59.000Z

Note: This page contains sample records for the topic "waha lone star" 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

Photoionising feedback in star cluster formation  

E-Print Network (OSTI)

We present the first ever hydrodynamic calculations of star cluster formation that incorporate the effect of feedback from ionising radiation. In our simulations, the ionising source forms in the cluster core at the intersection of several dense filaments of inflowing gas. We show that these filaments collimate ionised outflows and suggest such an environmental origin for at least some observed outflows in regions of massive star formation. Our simulations show both positive feedback (i.e. promotion of star formation in neutral gas compressed by expanding HII regions) and negative feedback (i.e. suppression of the accretion flow in to the central regions). We show that the volume filling factor of ionised gas is very different in our simulations than would result from the case where the central source interacted with an azimuthally smoothed gas density distribution. As expected, gas density is the key parameter in determining whether clusters are unbound by photoionising radiation. Nevertheless, we find - on account of the acceleration of a small fraction of the gas to high velocities in the outflows - that the deposition in the gas of an energy that exceeds the binding energy of the cluster is not a sufficient criterion for unbinding the bulk of the cluster mass.

J. E. Dale; I. A. Bonnell; C. J. Clarke; M. R. Bate

2005-01-10T23:59:59.000Z

462

Nuclear Reaction Rates and Carbon Star Formation  

E-Print Network (OSTI)

We have studied how the third dredge-up and the carbon star formation in low-mass Asymptotic Giant Branch stars depends on certain key nuclear reaction rates. We find from a set of complete stellar evolution calculations of a 2Msun model with Z=0.01 including mass loss, that varying either the N14(p,g)O15 or the 3-alpha reaction rate within their uncertainties as given in the NACRE compilation results in dredge-up and yields that differ by a factor of 2. Model tracks with a higher rate for the 3-alpha rate and a lower rate for the N14(p,g)O15 reaction both show more efficient third dredge-up. New experimental results for the N14(p,g)O15 reaction rates are surveyed, yielding a rate which is about 40% lower than the tabulated NACRE rate, and smaller than NACRE's lower limit. We discuss the possible implications of the revised nuclear reaction stellar evolution calculations that aim to reproduce the observed carbon star formation at low mass, which requires efficient third dredge-up.

Falk Herwig; Sam M. Austin

2004-08-21T23:59:59.000Z

463

Find an ENERGY STAR service and product provider | ENERGY STAR Buildings &  

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

Find an ENERGY STAR service and product provider Find an ENERGY STAR service and product provider Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Learn the benefits Get started Use Portfolio Manager Save energy Stamp out energy waste Find cost-effective investments Engage occupants Purchase energy-saving products Put computers to sleep Get help from an expert SPP success stories

464

Step 3: Evaluate your target using ENERGY STAR tools | ENERGY STAR  

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

Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Why you should design to earn the ENERGY STAR Follow EPA's step-by-step process Step 1: Assemble a team Step 2: Set an energy performance target Step 3: Evaluate your target using ENERGY STAR tools Comparing Target Finder and Portfolio Manager EPA's Target Finder calculator Step 4: Design to be energy efficient

465

Vectren Energy Delivery of Ohio (Gas) - Energy Star Home Rebate |  

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

Vectren Energy Delivery of Ohio (Gas) - Energy Star Home Rebate Vectren Energy Delivery of Ohio (Gas) - Energy Star Home Rebate Vectren Energy Delivery of Ohio (Gas) - Energy Star Home Rebate < Back Eligibility Construction Installer/Contractor Residential Savings Category Heating & Cooling Home Weatherization Construction Commercial Weatherization Commercial Heating & Cooling Design & Remodeling Program Info State Ohio Program Type Utility Rebate Program Rebate Amount Full Adoption of Energy Star (Version 2.5) Standards: $750 Vectren Gold Star - HERS rating of 70 or less: $750 Furnace: $300 Boiler: $500 Tankless Water Heater: $150 Storage Water Heater: $50-$150 Programmable Thermostat: $20 Provider Vectren Energy Delivery of Ohio Vectren Energy Delivery of Ohio offers a flat rebate to builders of residential single-family Energy Star certified homes that receive gas

466

Energy Star for Hospitals 2011 Update: Progression or Regression?  

E-Print Network (OSTI)

The Energy Star performance rating system for buildings has achieved widespread adoption in the building sector as a standard benchmark for energy performance. In 2011, the U.S. EPA released an updated technical methodology for its Energy Star performance rating system for hospitals, shifting how the score is calculated. The new rating system, similar to the previous rating system, is still a poor metric for benchmarking hospitals and should be used with caution. The aim of this paper is to critique the methodology used in the Energy Star for Hospitals 2011 Update. The paper reviews the changes between the 2001 methodology and 2011 methodology, how Energy Star views usage of different fuel types in its score, and lastly items that did not change in the 2011 hospital methodology update which are still causing confusion amongst Energy Star users and are causing significant error in the Energy Star score calculations.

Travis, B.

2012-01-01T23:59:59.000Z

467

PNM - Energy Star Home Builder Rebate Program | Department of Energy  

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

PNM - Energy Star Home Builder Rebate Program PNM - Energy Star Home Builder Rebate Program PNM - Energy Star Home Builder Rebate Program < Back Eligibility Construction Residential Savings Category Heating & Cooling Home Weatherization Construction Commercial Weatherization Commercial Heating & Cooling Design & Remodeling Program Info Expiration Date 12/31/2012 State New Mexico Program Type Utility Rebate Program Rebate Amount Energy Star for Homes Version 2.5: $750/home Provider PNM PNM is offering home builders a rebate for each Energy Star-qualified home they build in PNM service areas. Every Energy Star-qualified home must include effective insulation and air sealing, high performance windows, doors and skylights, tight construction and ducts, and independent testing and inspection. The builder must arrange for a qualified Home Energy Rater

468

General Electric: ENERGY STAR Referral (PFSF5NFZ****) | Department of  

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

General Electric: ENERGY STAR Referral (PFSF5NFZ****) General Electric: ENERGY STAR Referral (PFSF5NFZ****) General Electric: ENERGY STAR Referral (PFSF5NFZ****) August 29, 2012 DOE referred the matter of General Electric ("GE") refrigerator-freezer model PFSF5NFZ**** to the U.S. Environmental Protection Agency, brand manager for the ENERGY STAR Program, for appropriate action after DOE testing showed that the model does not meet the ENERGY STAR specification. After referring this matter, DOE determined that GE was also correct that the test report calculations were incorrect given that the tested model had a variable anti-sweat heater. DOE revised its test reports accordingly; however the corrections did not impact the final determination. General Electric: ENERGY STAR Referral (PFSF5NFZ****) More Documents & Publications

469

Webinar: ENERGY STAR Hot Water Systems for High Performance Homes  

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

Star Hot Water Systems for High Performance Homes Star Hot Water Systems for High Performance Homes 1 | Building America Program www.buildingamerica.gov Buildings Technologies Program Date: September 30, 2011 ENERGY STAR ® Hot Water Systems for High Performance Homes Welcome to the Webinar! We will start at 11:00 AM Eastern. There is no call in number. The audio will be sent through your computer speakers. All questions will be submitted via typing. Video of presenters Energy Star Hot Water Systems for High Performance Homes 2 | Building America Program www.buildingamerica.gov Energy Star Hot Water Systems for High Performance Homes 3 | Building America Program www.buildingamerica.gov Building America Program: Introduction Building Technologies Program Energy Star Hot Water Systems for High Performance Homes

470

DOE Testing Reveals Samsung Refrigerator Does Not Meet Energy Star  

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

Testing Reveals Samsung Refrigerator Does Not Meet Energy Star Testing Reveals Samsung Refrigerator Does Not Meet Energy Star Requirements DOE Testing Reveals Samsung Refrigerator Does Not Meet Energy Star Requirements March 16, 2010 - 4:28pm Addthis DOE-initiated testing has revealed that a Samsung refrigerator (model RF26VAB), which the company had claimed was Energy Star compliant, consumed more energy than permitted by the Energy Star program. Test results for the Samsung model at issue show that, when tested in accordance with DOE's test procedure, it consumed between 7 and 11.4 percent more energy than the Energy Star requirement. Samsung is no longer manufacturing this model, although it may still be available from some retail outlets. Based on this testing, DOE is referring Samsung Model RF26VAB to the U.S.

471

Entergy Texas - Energy Star Homes Program for Builders | Department of  

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

Entergy Texas - Energy Star Homes Program for Builders Entergy Texas - Energy Star Homes Program for Builders Entergy Texas - Energy Star Homes Program for Builders < Back Eligibility Construction Residential Savings Category Heating & Cooling Home Weatherization Construction Commercial Weatherization Commercial Heating & Cooling Design & Remodeling Program Info State Texas Program Type Utility Rebate Program Rebate Amount Single-Family Homes - Tier I (ENERGY STAR V-2.0): $150 per home Single-Family Homes - Tier II (ENERGY STAR V-2.5): $300 per home Attached Homes: 50% of single-family incentive per housing unit Advanced Lighting Package: $50 per single-family home ENERGY STAR V-3.0 HVAC Check Lists: $150 per single-family home Provider Entergy Texas Entergy Texas offers an incentive to builders in its service territory for

472

MHK Technologies/OceanStar | Open Energy Information  

Open Energy Info (EERE)

OceanStar OceanStar < MHK Technologies Jump to: navigation, search << Return to the MHK database homepage OceanStar.jpg Technology Profile Primary Organization Bourne Energy Technology Resource Click here Wave Technology Type Click here Overtopping Technology Readiness Level Click here TRL 4 Proof of Concept Technology Description The OceanStar device captures the underlying pressure wave through a series of small turbine generators The OceanStar relies upon a proprietary energy efficient process to smooth out the pulse characteristics common to wave energy in order to be electrical grid friendly The OceanStars high level of scalability is essential to reach the large surface areas required to reach utility scale ocean power generation Technology Dimensions

473

ENERGY STAR Labeled Buildings and Plants | Open Energy Information  

Open Energy Info (EERE)

STAR Labeled Buildings and Plants STAR Labeled Buildings and Plants Jump to: navigation, search Name ENERGY STAR Labeled Buildings and Plants Data Format Excel Spreadsheet Geographic Scope United States TODO: Import actual dataset contents into OpenEI The ENERGY STAR Labeled Buildings and Plants is "a list of facilities that measurably cost less to operate and improve the quality of our environment."[1] It is produced by the United States Environmental Protection Agency. External links Dataset in Excel Format References ↑ "ENERGY STAR Labeled Buildings and Plants" Retrieved from "http://en.openei.org/w/index.php?title=ENERGY_STAR_Labeled_Buildings_and_Plants&oldid=298127" Categories: Datasets Articles with outstanding TODO tasks What links here Related changes

474

Portfolio Manager DataTrends | ENERGY STAR Buildings & Plants  

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

Portfolio Manager DataTrends Portfolio Manager DataTrends Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Find out who's partnered with ENERGY STAR Become an ENERGY STAR partner Find ENERGY STAR certified buildings and plants ENERGY STAR certification Featured research and reports Portfolio Manager DataTrends ENERGY STAR Snapshot Energy strategy for the future

475

General Electric: ENERGY STAR Referral (PFSF5NFZ****) | Department of  

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

General Electric: ENERGY STAR Referral (PFSF5NFZ****) General Electric: ENERGY STAR Referral (PFSF5NFZ****) General Electric: ENERGY STAR Referral (PFSF5NFZ****) August 29, 2012 DOE referred the matter of General Electric ("GE") refrigerator-freezer model PFSF5NFZ**** to the U.S. Environmental Protection Agency, brand manager for the ENERGY STAR Program, for appropriate action after DOE testing showed that the model does not meet the ENERGY STAR specification. After referring this matter, DOE determined that GE was also correct that the test report calculations were incorrect given that the tested model had a variable anti-sweat heater. DOE revised its test reports accordingly; however the corrections did not impact the final determination. General Electric: ENERGY STAR Referral (PFSF5NFZ****) More Documents & Publications

476

A WISE VIEW OF STAR FORMATION IN LOCAL GALAXY CLUSTERS  

SciTech Connect

We present results from a systematic study of star formation in local galaxy clusters using 22 {mu}m data from the Wide-field Infrared Survey Explorer (WISE). The 69 systems in our sample are drawn from the Cluster Infall Regions Survey, and all have robust mass determinations. The all-sky WISE data enable us to quantify the amount of star formation, as traced by 22 {mu}m, as a function of radius well beyond R{sub 200}, and investigate the dependence of total star formation rate upon cluster mass. We find that the fraction of star-forming galaxies increases with cluster radius but remains below the field value even at 3R{sub 200}. We also find that there is no strong correlation between the mass-normalized total specific star formation rate and cluster mass, indicating that the mass of the host cluster does not strongly influence the total star formation rate of cluster members.

Chung, Sun Mi; Gonzalez, Anthony H. [Department of Astronomy, University of Florida, Gainesville, FL 32611-2055 (United States); Eisenhardt, Peter R.; Stern, Daniel [Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States); Stanford, Spencer A. [Department of Physics, University of California, Davis, CA 95616 (United States); Brodwin, Mark [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Jarrett, Thomas, E-mail: schung@astro.ufl.edu [Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States)

2011-12-10T23:59:59.000Z

477

Chemical abundance studies of CP stars in open clusters  

E-Print Network (OSTI)

In stellar astrophysics, the study of the atmospheres of early-type stars plays a very special role. The atmospheres of these stars display a variety of different phenomena, such as the presence of large magnetic fields, strong surface convection, pulsation, diffusion of chemical elements. In particular, about 10% of early F-, A- and late B-type stars present chemical peculiarities, which rise as a result of diffusion. A detailed study of the evolution of the chemical peculiarities as traces of diffusion processes requires the precise knowledge of stellar ages and initial chemical composition. Open clusters provide these information: 1) it is possible to assume that all cluster members have approximately the same original chemical composition and age; 2) the age of stars belonging to open clusters can be determined with much higher accuracy than for field stars. For this reason chemically peculiar stars member of open clusters have been targeted to study the evolution of the chemical peculiarities primarily t...

Fossati, Luca

2013-01-01T23:59:59.000Z

478

Variable Stars in Large Magellanic Cloud Globular Clusters III: Reticulum  

E-Print Network (OSTI)

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

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

2013-01-01T23:59:59.000Z

479

Magnetic fields and radiative feedback in the star formation process  

E-Print Network (OSTI)

Star formation is a complex process involving the interplay of many physical effects, including gravity, turbulent gas dynamics, magnetic fields and radiation. Our understanding of the process has improved substantially in recent years, primarily as a result of our increased ability to incorporate the relevant physics in numerical calculations of the star formation process. In this contribution we present an overview of our recent studies of star cluster formation in turbulent, magnetised clouds using self-gravitating radiation-magnetohydrodynamics calculations (Price and Bate 2008, 2009). Our incorporation of magnetic fields and radiative transfer into the Smoothed Particle Hydrodynamics method are discussed. We highlight how magnetic fields and radiative heating of the gas around newborn stars can solve several of the key puzzles in star formation, including an explanation for why star formation is such a slow and inefficient process. However, the presence of magnetic fields at observed strengths in collaps...

Price, Daniel J

2010-01-01T23:59:59.000Z

480

Seismological studies of ZZ Ceti stars. I. The model grid and the application to individual stars  

E-Print Network (OSTI)

We calculate and explore an extensive adiabatic model grid for pulsating white dwarfs with H dominated atmospheres, the ZZ Ceti stars. We also compared the computed modes with the observed ones for five ZZ Ceti stars that are a representative sample of the whole class of pulsators. We describe our new approach for seismological studies, using the relative observed amplitudes to give weights for the periods in the fit and the external mass and temperature determinations as a guide. Our seismological study is clear evidence that seismology is indeed a powerful tool in the study of stellar structure and evolution.

Castanheira, B G

2007-01-01T23:59:59.000Z

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


481

Seismological studies of ZZ Ceti stars. I. The model grid and the application to individual stars  

E-Print Network (OSTI)

We calculate and explore an extensive adiabatic model grid for pulsating white dwarfs with H dominated atmospheres, the ZZ Ceti stars. We also compared the computed modes with the observed ones for five ZZ Ceti stars that are a representative sample of the whole class of pulsators. We describe our new approach for seismological studies, using the relative observed amplitudes to give weights for the periods in the fit and the external mass and temperature determinations as a guide. Our seismological study is clear evidence that seismology is indeed a powerful tool in the study of stellar structure and evolution.

B. G. Castanheira; S. O. Kepler

2007-12-12T23:59:59.000Z

482

Spitzer spectroscopy of carbon stars in the Small Magellanic Cloud  

E-Print Network (OSTI)

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

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

2006-11-02T23:59:59.000Z

483

THE RAVE SURVEY: RICH IN VERY METAL-POOR STARS  

Science Conference Proceedings (OSTI)

Very metal-poor stars are of obvious importance for many problems in chemical evolution, star formation, and galaxy evolution. Finding complete samples of such stars which are also bright enough to allow high-precision individual analyses is of considerable interest. We demonstrate here that stars with iron abundances [Fe/H] <-2 dex, and down to below -4 dex, can be efficiently identified within the Radial Velocity Experiment (RAVE) survey of bright stars, without requiring additional confirmatory observations. We determine a calibration of the equivalent width of the calcium triplet lines measured from the RAVE spectra onto true [Fe/H], using high spectral resolution data for a subset of the stars. These RAVE iron abundances are accurate enough to obviate the need for confirmatory higher-resolution spectroscopy. Our initial study has identified 631 stars with [Fe/H] {<=}-2, from a RAVE database containing approximately 200,000 stars. This RAVE-based sample is complete for stars with [Fe/H] {approx_lt}-2.5, allowing statistical sample analysis. We identify three stars with [Fe/H] {approx_lt}-4. Of these, one was already known to be 'ultra metal-poor', one is a known carbon-enhanced metal-poor star, but we obtain [Fe/H] = -4.0, rather than the published [Fe/H] = -3.3, and derive [C/Fe] = +0.9, and [N/Fe] = +3.2, and the third is at the limit of our signal-to-noise ratio. RAVE observations are ongoing and should prove to be a rich source of bright, easily studied, very metal-poor stars.

Fulbright, Jon P.; Wyse, Rosemary F. G.; Ruchti, Gregory R. [Department of Physics and Astronomy, Johns Hopkins University, 366 Bloomberg Center, 3400 North Charles Street, Baltimore, MD 21218 (United States); Gilmore, G. F. [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA (United Kingdom); Grebel, Eva [Astronomisches Rechen-Institut, Zentrum fuer Astronomie der Universitaet Heidelberg, Moenchhofstr. 12-14, D-69120 Heidelberg (Germany); Bienayme, O.; Siebert, A. [Observatoire de Strasbourg, 11 Rue de L'Universite, 67000 Strasbourg (France); Binney, J. [Rudolf Pierls Center for Theoretical Physics, University of Oxford, 1 Keble Road, Oxford OX1 3NP (United Kingdom); Bland-Hawthorn, J. [Anglo-Australian Observatory, P.O. Box 296, Epping, NSW 1710 (Australia); Campbell, R. [Western Kentucky University, Bowling Green, KY (United States); Freeman, K. C. [RSAA Australian National University, Mount Stromlo Observatory, Cotter Road, Weston Creek, Canberra, ACT 72611 (Australia); Gibson, B. K. [Jeremiah Horrocks Institute for Astrophysics and Super-computing, University of Central Lancashire, Preston (United Kingdom); Helmi, A. [Kapteyn Astronomical Institute, University of Groningen, Postbus 800, 9700 AV Groningen (Netherlands); Munari, U. [INAF Osservatorio Astronomico di Padova, Via dell'Osservatorio 8, Asiago I-36012 (Italy); Navarro, J. F.; Siviero, A. [University of Victoria, P.O. Box 3055, Station CSC, Victoria, BC V8W 3P6 (Canada); Parker, Q. A.; Reid, W. [Macquarie University, Sydney, NSW 2109 (Australia); Seabroke, G. M. [Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, RH5 6NT (United Kingdom); Steinmetz, M. [Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam (Germany)

2010-11-20T23:59:59.000Z

484

List of Legislation and Campaigns Leveraging ENERGY STAR | ENERGY...  

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

List of Legislation and Campaigns Leveraging ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings...

485

STAR Images: Image gallery from the Solenoidal Tracker at RHIC  

DOE Data Explorer (OSTI)

The primary physics task of STAR is to study the formation and characteristics of the quark-gluon plasma (QGP), a state of matter believed to exist at sufficiently high energy densities. STAR consists of several types of detectors, each specializing in detecting certain types of particles or characterizing their motion. These detectors allow final statements to be made about the collision. The gallery of STAR images makes available a small collection of event-generated images from Gold-Beam experiments, a simulation of TCP Drift, and a library of STAR instrument and construction photos. [See also DDE00093

The STAR Collaboration

486

University of Minnesota (NorthernSTAR Building America Partnership...  

Open Energy Info (EERE)

Partnership Type Incubator Partnering Center within NREL Electricity Resources & Building Systems Integration LinkedIn Connections University of Minnesota (NorthernSTAR Building...

487

Xcel Energy - Residential ENERGY STAR Rebate Program | Department of Energy  

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

Residential ENERGY STAR Rebate Program Residential ENERGY STAR Rebate Program Xcel Energy - Residential ENERGY STAR Rebate Program < Back Eligibility Construction Residential Savings Category Home Weatherization Commercial Weatherization Sealing Your Home Appliances & Electronics Heating & Cooling Construction Commercial Heating & Cooling Design & Remodeling Ventilation Heating Commercial Lighting Lighting Water Heating Cooling Maximum Rebate Ground Source Heat Pump: $1500 Program Info Funding Source Home Performance with ENERGY STAR State Colorado Program Type Utility Rebate Program Rebate Amount Air Sealing and Weatherstripping: $160 Attic Insulation and Bypass Sealing: $350 High Efficiency Lighting: $40 Wall Insulation: $800 Set Back Thermostat: $25 Furnaces: $170 - $200 Boiler: $160 Electric Heat Pump: $550

488

Energy Star Building Upgrade Value Calculator | Open Energy Information  

Open Energy Info (EERE)

Energy Star Building Upgrade Value Calculator Energy Star Building Upgrade Value Calculator Jump to: navigation, search Tool Summary LAUNCH TOOL Name: Energy Star Building Upgrade Value Calculator (for Office Properties) Agency/Company /Organization: ENERGY STAR Phase: "Evaluate Options and Determine Feasibility" is not in the list of possible values (Bring the Right People Together, Create a Vision, Determine Baseline, Evaluate Options, Develop Goals, Prepare a Plan, Get Feedback, Develop Finance and Implement Projects, Create Early Successes, Evaluate Effectiveness and Revise as Needed) for this property. User Interface: Spreadsheet Website: www.energystar.gov/index.cfm?c=comm_real_estate.building_upgrade_value The Building Upgrade Value Calculator allows practitioners to analyze the

489

Industries in focus | ENERGY STAR Buildings & Plants  

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

ENERGY STAR Energy Performance Indicators for plants ENERGY STAR Energy Performance Indicators for plants » Industries in focus Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section Get started with ENERGY STAR Make the business case Build an energy management program Measure, track, and benchmark Tools for benchmarking energy management practices Tools for tracking and benchmarking facility energy performance

490

How ENERGY STAR Helps Manufacturers Improve the Energy Performance...  

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

ENERGY STAR Helps Manufacturers Improve the Energy Performance of their Operations Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and...

491

Electrolux: ENERGY STAR Referral (EIDW6305***) | Department of...  

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

EIDW6305***) Electrolux: ENERGY STAR Referral (EIDW6305***) April 3, 2012 DOE referred the matter of Electrolux dishwasher model EIDW6305*** to the EPA for appropriate action after...

492

ENERGY STAR Challenge for Industry promotional posters | ENERGY...  

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

Challenge for Industry helpful tools and resources ENERGY STAR Challenge for Industry promotional posters Secondary menu About us Press room Contact Us Portfolio Manager Login...

493

Partners promoting ENERGY STAR and energy efficiency | ENERGY...  

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

promoting ENERGY STAR and energy efficiency Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new...

494

Building Technologies Office: ENERGY STAR Test Procedures and...  

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

Test Procedures and Verification to someone by E-mail Share Building Technologies Office: ENERGY STAR Test Procedures and Verification on Facebook Tweet about Building Technologies...

495

Directory of energy efficiency programs leveraging ENERGY STAR...  

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

Directory of energy efficiency programs leveraging ENERGY STAR Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings...

496

DIRECTORY OF ENERGY EFFICIENCY PROGRAMS LEVERAGING ENERGY STAR  

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

DIRECTORY OF ENERGY EFFICIENCY PROGRAMS LEVERAGING ENERGY STAR (UPDATED JANUARY 20, 2012) Utilities and state program sponsors across the country are incorporating benchmarking...

497

ENERGY STAR National Building Competition: 2010 summary | ENERGY...  

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

ENERGY STAR National Building Competition: 2010 summary Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings...

498

Dim Isolated Neutron Stars, Cooling and Energy Dissipation  

E-Print Network (OSTI)

The cooling and reheating histories of dim isolated neutron stars(DINs) are discussed. Energy dissipation due to dipole spindown with ordinary and magnetar fields, and due to torques from a fallback disk are considered as alternative sources of reheating which would set the temperature of the neutron star after the initial cooling era. Cooling or thermal ages are related to the numbers and formation rates of the DINs and therefore to their relations with other isolated neutron star populations. Interaction with a fallback disk, higher multipole fields and activity of the neutron star are briefly discussed.

M. Ali Alpar

2006-09-07T23:59:59.000Z

499

Award Recipient of the ENERGY STAR Challenge for Industry Gustine...  

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

the ENERGY STAR Challenge for Industry in 2010. This plant reached 12% reduction in energy intensity within two years of its baseline. The Gustine Plant achieved the...

500

ENERGY STAR Challenge for Industry: Statement of Energy Improvement...  

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

Challenge for Industry: Statement of Energy Improvement Use this form to document the energy intensity reduction of an industrial site that is participating in the ENERGY STAR...