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Sample records for brown young dallas

  1. Brown Dwarf Companions to Young Solar Analogs: An Adaptive Optics Survey Using Palomar and Keck

    E-Print Network [OSTI]

    Metchev, Stanimir

    Brown Dwarf Companions to Young Solar Analogs: An Adaptive Optics Survey Using Palomar and Keck to its present state, had it not been for the dedication and professionalism of the Palomar and Keck possibilities offered by the technology. Rich and Hal also helped me design the Palomar AO astrometric

  2. The BANYAN All-Sky Survey for Brown Dwarf Members of Young Moving Groups

    E-Print Network [OSTI]

    Gagné, Jonathan; Doyon, René; Faherty, Jacqueline K; Malo, Lison; Cruz, Kelle L; Artigau, Étienne; Burgasser, Adam J; Naud, Marie-Eve; Bouchard, Sandie; Gizis, John E; Albert, Loïc

    2015-01-01

    We describe in this work the BASS survey for brown dwarfs in young moving groups of the solar neighborhood, and summarize the results that it generated. These include the discovery of the 2MASS J01033563-5515561 (AB)b and 2MASS J02192210-3925225 B young companions near the deuterium-burning limit as well as 44 new low-mass stars and 69 new brown dwarfs with a spectroscopically confirmed low gravity. Among those, ~20 have estimated masses within the planetary regime, one is a new L4 $\\gamma$ bona fide member of AB Doradus, three are TW Hydrae candidates with later spectral types (L1-L4) than all of its previously known members and six are among the first contenders to low-gravity $\\geq$ L5 $\\beta$/$\\gamma$ brown dwarfs, reminiscent of WISEP J004701.06+680352.1, PSO J318.5338-22.8603 and VHS J125601.92-125723.9 b. Finally, we describe a future version of this survey, BASS-Ultracool, that will specifically target $\\geq$ L5 candidate members of young moving groups. First experimentations in designing the survey h...

  3. IEEE Dallas Engineering

    E-Print Network [OSTI]

    Yang, Jian

    2007 IEEE Dallas Engineering in Medicine and Biology Workshop #12; 2007 IEEE Dallas Engineering in Medicine and Biology Workshop Emerging Technologies for Healthcare OF THE IEEE ENGINEERING IN MEDICINE AND BIOLOGY SOCIETY i #12;Abstract- The lack of suitable scaffolding

  4. Young Low-Mass Stars and Brown Dwarfs in IC 348

    E-Print Network [OSTI]

    K. L. Luhman

    1999-05-21

    I present new results from a continuing program to identify and characterize the low-mass stellar and substellar populations in the young cluster IC 348 (1-10~Myr). Optical spectroscopy has revealed young objects with spectral types as late as M8.25. The intrinsic J-H and H-K colors of these sources are dwarf-like, whereas the R-I and I-J colors appear intermediate between the colors of dwarfs and giants. Furthermore, the spectra from 6500 to 9500 A are reproduced well with averages of standard dwarf and giant spectra, suggesting that such averages should be used in the classification of young late-type sources. An H-R diagram is constructed for the low-mass population in IC 348 (K6-M8). The presumably coeval components of the young quadruple system GG~Tau (White et al.) and the locus of stars in IC 348 are used as empirical isochrones to test the theoretical evolutionary models. For the models of Baraffe et al., an adjustment of the temperature scale to progressively warmer temperatures at later M types, intermediate between dwarfs and giants, brings all components of GG~Tau onto the same model isochrone and gives the population of IC 348 a constant age and age spread as a function of mass. When other observational constraints are considered, such as the dynamical masses of GM~Aur, DM~Tau, and GG~Tau~A, the models of Baraffe et al. are the most consistent with observations of young systems. With compatible temperature scales, the models of both D'Antona & Mazzitelli and Baraffe et al. suggest that the hydrogen burning mass limit occurs near M6 at ages of <10 Myr. Thus, several likely brown dwarfs are discovered in this study of IC 348, with masses down to ~20-30 M_J.

  5. Dallas Challenge Final Report 

    E-Print Network [OSTI]

    Medina, Gabriella; Leichtle, Stephanie; Garraway, Charlotte

    2015-05-20

    .............................................................................................. 45 Appendix ..................................................................................................................................................................... 54 List of Figures... Summary The project is an analysis of Dallas Challenge’s current image through a stakeholder assessment. Following the assessment, we will provide strategies and tactics that...

  6. A pulsation search among young brown dwarfs and very-low-mass stars

    SciTech Connect (OSTI)

    Cody, Ann Marie; Hillenbrand, Lynne A., E-mail: amc@ipac.caltech.edu [California Institute of Technology, Department of Astrophysics, MC 249-17, Pasadena, CA 91125 (United States)

    2014-12-01

    In 2005, Palla and Baraffe proposed that brown dwarfs (BDs) and very-low-mass stars (VLMSs; < 0.1 solar masses) may be unstable to radial oscillations during the pre-main-sequence deuterium burning phase. With associated periods of one to four hours, this potentially new class of pulsation offers unprecedented opportunities to probe the interiors and evolution of low-mass objects in the 1-15 million year age range. Following up on reports of short-period variability in young clusters, we designed a high-cadence photometric monitoring campaign to search for deuterium-burning pulsation among a sample of 348 BDs and VLMSs in the four young clusters ? Orionis, Chamaeleon I, IC 348, and Upper Scorpius. In the resulting light curves we achieved sensitivity to periodic signals of amplitude several millimagnitudes, on timescales from 15 minutes to two weeks. Despite the exquisite data quality, we failed to detect any periodicities below seven hours. We conclude that D-burning pulsations are not able to grow to observable amplitudes in the early pre-main sequence. In spite of the nondetection, we did uncover a rich set of variability behavior—both periodic and aperiodic—on day to week timescales. We present new compilations of variable sources from our sample, as well as three new candidate cluster members in Chamaeleon I.

  7. Frazier Courts, Dallas 

    E-Print Network [OSTI]

    Hall, B.

    2011-01-01

    in kind donors Ex: Valspar donates paint so Habitat requests that we receive low- VOC paint ESL-KT-11-11-24 CATEE 2011, Dallas, Texas, Nov. 7 ? 9, 2011 Completely sealed walls High quality, thermally efficient windows (Double pane, Low E... are also energy conscious & utilize green building methods Ex: HVAC installer tapes duct work so does not get contaminated during construction Dallas Habitat relies heavily on the cooperation & collaboration of paid vendors & gift...

  8. SUBSTELLAR OBJECTS IN NEARBY YOUNG CLUSTERS (SONYC). II. THE BROWN DWARF POPULATION OF {rho} OPHIUCHI

    SciTech Connect (OSTI)

    Geers, Vincent; Jayawardhana, Ray; Lee, Eve; Lafreniere, David [Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5S 3H4 (Canada); Scholz, Alexander [School of Cosmic Physics, Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2 (Ireland); Tamura, Motohide, E-mail: vcgeers@astro.utoronto.ca [National Astronomical Observatory, Osawa 2-21-2, Mitaka, Tokyo 181 (Japan)

    2011-01-01

    SONYC-Substellar Objects in Nearby Young Clusters-is a survey program to investigate the frequency and properties of brown dwarfs (BDs) down to masses below the deuterium-burning limit in nearby star-forming regions. In this second paper, we present results on the {approx}1 Myr old cluster {rho} Ophiuchi, combining our own deep optical- and near-infrared imaging using Subaru with photometry from the Two Micron All Sky Survey and the Spitzer Space Telescope. Of the candidates selected from iJK{sub s} photometry, we have confirmed three-including a new BD with a mass close to the deuterium limit-as likely cluster members through low-resolution infrared spectroscopy. We also identify 27 substellar candidates with mid-infrared excess consistent with disk emission, of which 16 are new and 11 are previously spectroscopically confirmed BDs. The high and variable extinction makes it difficult to obtain the complete substellar population in this region. However, current data suggest that its ratio of low-mass stars to BDs is similar to those reported for several other clusters, though higher than what was found for NGC 1333 in Scholz et al.

  9. Ozone induces glucose intolerance and systemic metabolic effects in young and aged brown Norway rats

    SciTech Connect (OSTI)

    Bass, V.; Gordon, C.J.; Jarema, K.A.; MacPhail, R.C.; Cascio, W.E.; Phillips, P.M.; Ledbetter, A.D.; Schladweiler, M.C.; Andrews, D.; Miller, D.; Doerfler, D.L.; Kodavanti, U.P.

    2013-12-15

    Air pollutants have been associated with increased diabetes in humans. We hypothesized that ozone would impair glucose homeostasis by altering insulin signaling and/or endoplasmic reticular (ER) stress in young and aged rats. One, 4, 12, and 24 month old Brown Norway (BN) rats were exposed to air or ozone, 0.25 or 1.0 ppm, 6 h/day for 2 days (acute) or 2 d/week for 13 weeks (subchronic). Additionally, 4 month old rats were exposed to air or 1.0 ppm ozone, 6 h/day for 1 or 2 days (time-course). Glucose tolerance tests (GTT) were performed immediately after exposure. Serum and tissue biomarkers were analyzed 18 h after final ozone for acute and subchronic studies, and immediately after each day of exposure in the time-course study. Age-related glucose intolerance and increases in metabolic biomarkers were apparent at baseline. Acute ozone caused hyperglycemia and glucose intolerance in rats of all ages. Ozone-induced glucose intolerance was reduced in rats exposed for 13 weeks. Acute, but not subchronic ozone increased ?{sub 2}-macroglobulin, adiponectin and osteopontin. Time-course analysis indicated glucose intolerance at days 1 and 2 (2 > 1), and a recovery 18 h post ozone. Leptin increased day 1 and epinephrine at all times after ozone. Ozone tended to decrease phosphorylated insulin receptor substrate-1 in liver and adipose tissues. ER stress appeared to be the consequence of ozone induced acute metabolic impairment since transcriptional markers of ER stress increased only after 2 days of ozone. In conclusion, acute ozone exposure induces marked systemic metabolic impairments in BN rats of all ages, likely through sympathetic stimulation. - Highlights: • Air pollutants have been associated with increased diabetes in humans. • Acute ozone exposure produces profound metabolic alterations in rats. • Age influences metabolic risk factors in aging BN rats. • Acute metabolic effects are reversible and repeated exposure reduces these effects. • Ozone metabolic effects are only slightly exacerbated in geriatric rats.

  10. City of Dallas Green Building Case Study 

    E-Print Network [OSTI]

    Basora, Z.

    2012-01-01

    Inspection City of Dallas Public Works Department City of Dallas Green Building Case Study CATEE CONFERENCE October 10, 2012 Dallas Building Inspection Take Aways ? Green Building Strategy Implementation is a process ? Awareness ? Education... Dallas Case Study 3 Dallas Building Inspection Municipal Green Building Program ? Adopted on January 22, 2003 ? all municipal projects over 10,000 s.f. to be LEED Silver Certified ? The City of Dallas has 21 LEED certified buildings, 9 gold, 11...

  11. MIS @ UT Dallas Creating Value Through IT -Driven Business Intelligence

    E-Print Network [OSTI]

    O'Toole, Alice J.

    Network Engineer III McDonald's IT Staff UT Dallas Computing Help Desk SAP America Senior Product North America Sales Associate Fidelity Investments Associate Systems Analyst Ernst & Young Forensic Technology and Discovery Services Walmart Inventory Associate Bank of America Project Consultant National

  12. Spitzer IRAC Observations of White Dwarfs. II. Massive Planetary and Cold Brown Dwarf Companions to Young and Old Degenerates

    E-Print Network [OSTI]

    J. Farihi; E. E. Becklin; B. Zuckerman

    2008-05-13

    This paper presents a sensitive and comprehensive IRAC 3-8 $\\mu$m photometric survey of white dwarfs for companions in the planetary mass regime with temperatures cooler than the known T dwarfs. The search focuses on descendents of intermediate mass stars with $M\\ga3$ $M_{\\odot}$ whose inner, few hundred AU regions cannot be probed effectively for massive planets and brown dwarfs by any alternative existing method. Furthermore, examination for mid-infrared excess explores an extensive range of orbital semimajor axes, including the intermediate 5-50 AU range poorly covered and incompletely accessible by other techniques at main sequence or evolved stars. Three samples of white dwarfs are chosen which together represent relatively young as well as older populations of stars: 9 open cluster white dwarfs, 22 high mass field white dwarfs, and 17 metal-rich field white dwarfs. In particular, these targets include: 7 Hyads and 4 field white dwarfs of similar age; 1 Pleiad and 19 field white dwarfs of similar age; van Maanen 2 and 16 similarly metal-rich white dwarfs with ages between 1 and 7 Gyr. No substellar companion candidates were identified at any star. By demanding a 15% minimum photometric excess at 4.5 $\\mu$m to indicate a companion detection, upper limits in the planetary mass regime are established at 34 of the sample white dwarfs, 20 of which have limits below 10 $M_{\\rm J}$ according to substellar cooling models. Specifically, limits below the minimum mass for deuterium burning are established at all Pleiades and Hyadeswhite dwarfs, as well as similarly young field white dwarfs, half a dozen of which receive limits at or below 5 $M_{\\rm J}$. Two IRAC epochs at vMa 2 rule out $T\\ga200$ K proper motion companions within 1200 AU.

  13. Prairie Creek Branch Public Library, Dallas 

    E-Print Network [OSTI]

    Meckfessel, R.

    2011-01-01

    ? 53 well geothermal / heat pump system ? greywater recapture and reuse ? 7.7 kw photovoltaic array key sustainability overview - energy and water ? compliance with City of Dallas iSWM program ? raised floor air distribution ? high...

  14. City of Dallas- Green Energy Purchasing

    Office of Energy Efficiency and Renewable Energy (EERE)

    Furthermore, the Dallas/Fort Worth International Airport is the highest-ranked airport for renewable energy use, separately ranking 7th on the Green Power Partner listing of local government gree...

  15. DENNIS J. MOORE 2015 Young Guns Award Recipient

    E-Print Network [OSTI]

    Rock, Chris

    DENNIS J. MOORE 2015 Young Guns Award Recipient Dennis J. Moore, CFP® , MBA has established himself. In addition, he was named the 2011 FPA DFW Young Gun. Dennis lives in Dallas with his wife, Aubrey, who

  16. Planck cold clumps in the $\\lambda$ Orionis complex: I. Discovery of an extremely young Class 0 protostellar object and a proto-brown dwarf candidate in a bright rimmed clump PGCC G192.32-11.88

    E-Print Network [OSTI]

    Liu, Tie; Kim, Kee-Tae; Wu, Yuefang; Lee, Chang Won; Lee, Jeong-Eun; Tatematsu, Kenichi; Choi, Minho; Juvela, Mika; Thompson, Mark; Goldsmith, Paul F; Liu, Sheng-yuan; Naomi, Hirano; Koch, Patrick; Henkel, Christian; Sanhueza, Patricio; He, JinHua; Rivera-Ingraham, Alana; Wang, Ke; Cunningham, Maria R; Tang, Ya-Wen; Lai, Shih-Ping; Yuan, Jinghua; Li, Di; Fuller, Gary; Kang, Miju; Luong, Quang Nguyen; Liu, Hauyu Baobab; Ristorcelli, Isabelle; Yang, Ji; Xu, Ye; Hirota, Tomoya; Mardones, Diego; Qin, Sheng-Li; Chen, Huei-Ru; Kwon, Woojin; Meng, FanYi; Zhang, Huawei; Kim, Mi-Ryang; Yi, Hee-Weon

    2015-01-01

    We are performing a series of observations with ground-based telescopes toward Planck Galactic cold clumps (PGCCs) in the $\\lambda$ Orionis complex in order to systematically investigate the effects of stellar feedback. In the particular case of PGCC G192.32-11.88, we discovered an extremely young Class 0 protostellar object (G192N) and a proto-brown dwarf candidate (G192S). G192N and G192S are located in a gravitationally bound bright-rimmed clump. The velocity and temperature gradients seen in line emission of CO isotopologues indicate that PGCC G192.32-11.88 is externally heated and compressed. G192N probably has the lowest bolometric luminosity ($\\sim0.8$ L$_{\\sun}$) and accretion rate (6.3$\\times10^{-7}$ M$_{\\sun}$~yr$^{-1}$) when compared with other young Class 0 sources (e.g. PACS Bright Red sources (PBRs)) in the Orion complex. It has slightly larger internal luminosity ($0.21\\pm0.01$ L$_{\\sun}$) and outflow velocity ($\\sim$14 km~s$^{-1}$) than the predictions of first hydrostatic cores (FHSCs). G192N...

  17. Energy Savings Report For Dallas County, July 2000 – June 2001 

    E-Print Network [OSTI]

    Claridge, D. E.; Baltazar-Cervantes, J. C.; Zhu, Y.

    2001-01-01

    This report presents the energy and dollar savings for the period July 2000 - June 2001 for 12 Dallas County facilities that have been retrofit by Enershop. The savings for this period total $745,046, which represent 73.2% of the audit estimated...

  18. Lamb customer satisfaction in two Texas cities - - Dallas and Houston 

    E-Print Network [OSTI]

    Maddock, Travis David

    2001-01-01

    An in-home lamb study evaluated consumer ratings from users of lamb (at least once per month) as influenced by cut (blade chop, rib chop, loin chop, and leg steak), demographics, preparation method, and degree of doneness. Consumers in Dallas...

  19. The University of Texas at Dallas Texas Hazardous Communication Act

    E-Print Network [OSTI]

    O'Toole, Alice J.

    The University of Texas at Dallas Texas Hazardous Communication Act Handbook #12;TEXAS HAZARDOUS IV. Texas Hazard Communication Act Exemptions V. Implementation A. Employee Rights Under the Act Explanation IX. Written Hazard Communication Program A. Manufacturers' Labels and Other Forms of Warning B

  20. Fermilab Today | Brown University Profile

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

    Brown University April 29, 2010 NAME: Brown University HOME TOWN: Providence, Rhode Island MASCOT: Bruno the Bear SCHOOL COLORS: Seal brown and cardinal red PARTICLE PHYSICS...

  1. Sevin Rosen Funds (Texas - Dallas) | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page| Open Energy Information Serbia-Enhancing Capacity for Low Emission DevelopmentLakes, NorthTennessee:Dallas) Jump to:

  2. Alternative Fuel Transit Buses: DART's (Dallas Area Rapid Transit) LNG Bus Fleet Final Results

    SciTech Connect (OSTI)

    Chandler, K.; Norton, P.; Clark, N.

    2000-11-07

    In 1998, Dallas Area Rapid Transit, a public transit agency in Dallas, Texas, began operating a large fleet of heavy-duty buses powered by liquefied natural gas. As part of a $16 million commitment to alternative fuels, DART operates 139 LNG buses serviced by two new LNG fueling stations.

  3. The Onset of Planet Formation in Brown Dwarf Disks

    E-Print Network [OSTI]

    D. Apai; I. Pascucci; J. Bouwman; A. Natta; Th. Henning; C. P. Dullemond

    2005-11-14

    The onset of planet formation in protoplanetary disks is marked by the growth and crystallization of sub-micron-sized dust grains accompanied by dust settling toward the disk mid-plane. Here we present infrared spectra of disks around brown dwarfs and brown dwarf candidates. We show that all three processes occur in such cool disks in a way similar or identical to that in disks around low- and intermediate-mass stars. These results indicate that the onset of planet formation extends to disks around brown dwarfs, suggesting that planet formation is a robust process occurring in most young circumstellar disks.

  4. Interview of Dan Brown

    E-Print Network [OSTI]

    Brown, Dan

    2008-06-09

    stream_source_info brown.txt.txt stream_content_type text/plain stream_size 14108 Content-Encoding UTF-8 stream_name brown.txt.txt Content-Type text/plain; charset=UTF-8 Dan Brown interviewed by Alan Macfarlane 10th January 2008... down ? the 3?- phosphate [there are four nucleosides in RNA with positions 2?-, 3?- and 5?- which can carry a phosphate group]; amazingly Waldo Cohn found that the methods used to separate metals in the atomic energy field could be used to separate...

  5. An ozone climatology of the Dallas-Fort Worth area and its relationship to meteorology 

    E-Print Network [OSTI]

    Nobis, Timothy Edward

    1998-01-01

    The Environmental protection agency has established a hics. National Ambient Air Quality Standard for surface ozone through the Clean Air Act and its amendments. The Dallas / Fort Worth area is in violation of these standards, and to date...

  6. Temperature and Violent Crime in Dallas, Texas: Relationships and Implications of Climate Change

    E-Print Network [OSTI]

    Gamble, Janet L; Hess, Jeremy J

    2012-01-01

    robbery (31.0%), forcible rape (6.7%), and murder (1.2%). 1crime data for aggravated assault, homicide, and rape andattempted rape in Dallas for 1993 to 1999, and daily

  7. Case Study Walnut Hill United Methodist Church - Dallas, Texas, Chiller Replacement Analysis 

    E-Print Network [OSTI]

    Phillips, J.

    1998-01-01

    In March of 1992 Walnut Hill United Methodist Church in Dallas, Tx. decided that their existing thermal storage and electric reciprocating chiller system were both in need of replacement. After analyzing several options, they chose to install 150...

  8. BROWN ALGAE Colpomenia sinuosa

    E-Print Network [OSTI]

    Sullivan, Matthew B.

    BROWN ALGAE Colpomenia sinuosa GREEN ALGAE Dictyosphaeria cavernosa Amphiroa fragilissima Gelidiopsis intricata Botryocladia pyriformis RED ALGAE CYANOBACTERIA Oscillitoria acuminata Schizothrix sp. "ALGAE"­ A DIVERSE ASSORTMENT OF LIFE FORMS Photosynthesis is performed by a taxonomically diverse

  9. Between Cool Stars and Hot Planets: Origins of Brown Dwarfs

    E-Print Network [OSTI]

    Ray Jayawardhana

    2003-10-28

    Brown dwarfs, which straddle the mass range between stars and planets, appear to be common both in the solar neighborhood and in star-forming regions. Their ubiquity makes the question of their origin an important one both for our understanding of brown dwarfs themselves as well as for theories on the formation of stars and planets. Studies of young sub-stellar objects could provide valuable insight into their formation and early evolution. Here I report on the latest results from our observational programs at Keck, VLT and Magellan on the disk and accretion properties of young brown dwarfs. We find compelling evidence that they undergo a T Tauri phase analogous to that of their stellar counterparts.

  10. Risk Assessment Sally Brown

    E-Print Network [OSTI]

    Brown, Sally

    or publicly owned treatment works) whose regulations and rule enforcement work to make sure that the risksRisk Assessment Sally Brown University of Washington Risk in our day to day routines One could argue that every thing that we do, every day is fraught with risks and that the safest approach is just

  11. Test Access Mechanism for Core Based SystemonChip The Univ. of Texas at Dallas

    E-Print Network [OSTI]

    Nourani, Mehrdad

    1 Test Access Mechanism for Core Based System­on­Chip M. Nourani The Univ. of Texas at Dallas Dept of TAM for SoC's. The basic goal is to develop a global design for test methodology and tool for testing as their interactions to one another. More specifically, it al­ lows at­speed testing and multi­core interaction during

  12. EXPERIMENTAL NON-DESTRUCTIVE TESTING OF FRP MATERIALS, INSTALLATION, AND PERFORMANCE, DALLAS COUNTY BRIDGE, MISSOURI, USA

    E-Print Network [OSTI]

    Maerz, Norbert H.

    EXPERIMENTAL NON-DESTRUCTIVE TESTING OF FRP MATERIALS, INSTALLATION, AND PERFORMANCE, DALLAS COUNTY provided the opportunity to use new and existing technologies to test the FRP materials installations alignment, FRP delamination, and FRP bond pull-off strength. Results of testing to date are presented

  13. Alabama Nuclear Profile - Browns Ferry

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

    Browns Ferry" "Unit","Summer capacity (mw)","Net generation (thousand mwh)","Summer capacity factor (percent)","Type","Commercial operation date","License expiration date"...

  14. Bridging Brown County Case Study Bridging Brown County Case Study

    E-Print Network [OSTI]

    Minnesota, University of

    and Finding a Future Summary and Background Communities in the rural Midwest typically understand and solve unique issues facing rural communities? In Brown County, Minnesota, the community developed. But we also belong to a larger rural community: the community formed by all residents of Brown County. We

  15. Hanbury Brown and Twiss Effect Anton Kapliy

    E-Print Network [OSTI]

    Hanbury Brown and Twiss Effect Anton Kapliy March 10, 2009 #12;Robert Hanbury Brown (1916 - 2002 figure: fermionic Helium #12;Partial list of sources ·http://faculty.virginia.edu/austen/HanburyBrownTwiss

  16. The physics of brown dwarfs

    E-Print Network [OSTI]

    Gilles Chabrier

    1999-02-01

    We briefly outline the physics underlying the mechanical and thermal properties of brown dwarfs, which characterizes their interiors and their atmospheres. We mention the most recent improvements realyzed in the theory of brown dwarfs and the connection with experimental and observational tests of this theory.

  17. Measured Cooling Performance of Two-story Homes in Dallas, Texas; Insulated Concrete Form Versus Frame Construction 

    E-Print Network [OSTI]

    Chasar, D.; Moyer, N.; Rudd, A. F.; Parker, D.; Chandra, S.

    2002-01-01

    Four occupied homes near Dallas, Texas were monitored to compare heating and cooling energy use. Two homes were built with typical wood frame construction, the other two with insulated concrete form (ICF) construction. Remote ...

  18. Petrologic and petrophysical evaluation of the Dallas Center Structure, Iowa, for compressed air energy storage in the Mount Simon Sandstone.

    SciTech Connect (OSTI)

    Heath, Jason E.; Bauer, Stephen J.; Broome, Scott Thomas; Dewers, Thomas A.; Rodriguez, Mark Andrew

    2013-03-01

    The Iowa Stored Energy Plant Agency selected a geologic structure at Dallas Center, Iowa, for evaluation of subsurface compressed air energy storage. The site was rejected due to lower-than-expected and heterogeneous permeability of the target reservoir, lower-than-desired porosity, and small reservoir volume. In an initial feasibility study, permeability and porosity distributions of flow units for the nearby Redfield gas storage field were applied as analogue values for numerical modeling of the Dallas Center Structure. These reservoir data, coupled with an optimistic reservoir volume, produced favorable results. However, it was determined that the Dallas Center Structure cannot be simplified to four zones of high, uniform permeabilities. Updated modeling using field and core data for the site provided unfavorable results for air fill-up. This report presents Sandia National Laboratories' petrologic and petrophysical analysis of the Dallas Center Structure that aids in understanding why the site was not suitable for gas storage.

  19. Changing the state of fairness : redeveloping Fair Park as a catalyst for the revitalization of South Dallas

    E-Print Network [OSTI]

    Di Mambro, Giuliana Siena

    2013-01-01

    This thesis studies Fair Park, a 277 acre public park located in Dallas, Texas. Fair Park represents prevalent planning challenges - the repurposing of sites that have outlived their initial uses and the reintegration of ...

  20. Modeling the per capita ecological footprint for Dallas County, Texas: Examining demographic, environmental value, land-use, and spatial influences 

    E-Print Network [OSTI]

    Ryu, Hyung Cheal

    2005-08-29

    This study addresses factors driving the variation in the per capita Ecological Footprint (EF) in Dallas County, Texas. A main hypothesis was that scientifically estimated demography, environmental values, spatial attributes, and land-use patterns...

  1. Spatial Ecology of and Public Attitudes toward Monk Parakeets Nesting on Electric Utility Structures in Dallas and Tarrant Counties, Texas 

    E-Print Network [OSTI]

    Reed, Janet Elaine

    2014-07-29

    with variables predicting participants’ beliefs and concerns (responses) for managing monk parakeets nesting and making too much noise near participants’ homes (Component 1a), Dallas and Tarrant counties, Texas, USA, September 2012–February 2013.... .............. 225 Table 5.14. Full model with variables predicting participants’ beliefs and concerns (responses) for managing monk parakeets nesting and making too much noise near participants’ homes (Component 2a), Dallas and Tarrant counties, Texas, USA...

  2. How's LEED doing?- Analyzing the Success of Dallas' Green Building Initiative 

    E-Print Network [OSTI]

    Basora, Z.; Meckfessel, B.

    2013-01-01

    : Clean Air Through Energy Efficiency Conference, San Antonio, Texas Dec. 16-18 City of Dallas Goals for LEED Program • Operating Costs: 30% energy reduction. • Education of citizens about benefits of sustainable design. • Leading the community... WEST BRANCH LIBRARY ESL-KT-13-12-09 CATEE 2013: Clean Air Through Energy Efficiency Conference, San Antonio, Texas Dec. 16-18 Data UTILITY INFORMATION • Utility consumption and cost were normalized and compared on per-square-foot basis. • Compiled...

  3. Descriptions and Uses of Soils of the Texas Agricultural Experiment Stations at Dallas and Prosper. 

    E-Print Network [OSTI]

    Hipp, Billy W.; Knowles, Tim C.; Simpson, Benny J.; Stringer, Billy R.; Hallmark, C. Tom

    1992-01-01

    organic matter in the surface layer. Vertisols are referred to as self mulching soils or cracking clays. Entisols show little or no evidence of horizon development. The soils of the Dallas Center developed mainly from chalk and interbedded marl under... Upper Cretaceous chalk and interbedded marl under tallgrass and mid-bunchgrass vegeta tion (U. S. Depart ment of Agriculture, 1969). The relief is nearly level to gently sloping with slopes ranging from 0 to 3 percent. Weathering of the marl...

  4. The Economic Benefits of Built Environment Supportive of Active Living in Dallas Tax Increment Financing Districts 

    E-Print Network [OSTI]

    Xu, Minjie

    2015-08-11

    of the most active and successfully practiced mechanisms to implement smart growth principles. This dissertation consists of three studies in the city of Dallas to examine different outcomes related to the study goals. In Chapter 2, I employed a quasi... collaboration in development decisions. Since then, smart growth has rapidly gained its popularity. Proponents of smart growth include urban and transportation planners, public health professions, environmentalists, and central city advocates, among others...

  5. Dallas area-wide intelligent transportation system plan. Draft research report, August 1992-August 1996

    SciTech Connect (OSTI)

    Carvell, J.D.; Seymour, E.J.; Walters, C.H.; Starr, T.R.; Balke, K.

    1996-07-01

    This report documents the development of a comprehensive plan for implementation of Intelligent Transportation Systems (ITS) in the Dallas Urban Area. The contract defined objectives: Develop a Broadly Based Steering Committee; Assess Existing Transportation Management Systems and Potential ITS Technology; Identify Institutional Issues and Legal Barriers; Develop an Implementable, Area-Wide Multi-Jurisdictional ITS Plan; and Develop Cost, Benefits, and an Implementation Plan.

  6. Charles L. Brown Department of Electrical & Computer

    E-Print Network [OSTI]

    Acton, Scott

    -imaging and -electronics, and superconducting electronics Every faculty member in the Charles L. Brown Department

  7. Controlling Brown Stomach Worms in Cattle by Management 

    E-Print Network [OSTI]

    Faries Jr., Floron C.

    2002-02-05

    be weaned and removed from the cow herd before the high risk of exposure to pasture larvae in the spring. Calves and young cattle are more susceptible to worms and pass more eggs in their manure than adult cattle. Older nursing calves are a major source... and adult worms in the stomachs of cattle. *Associate Professor and Extension Program Leader for Veterinary Medicine, The Texas A&M University System Good quality pasture with high protein content controls brown stomach worms in cattle. eggs passed...

  8. Hanbury Brown-Twiss Experiment with Coherent

    E-Print Network [OSTI]

    39 Chapter 2 Hanbury Brown-Twiss Experiment with Coherent Light This chapter was previously a theory that allows us #12;40 Hanbury Brown-Twiss Experiment with Coherent Light to construct processes

  9. Edited by Allison P. Brown Edited by Allison P. Brown

    E-Print Network [OSTI]

    Salzman, Daniel

    at SUNY Geneseo and the Monroe County Library System to identify trends in library publishing, seek outTube Channel by Kara Stock 34 The Library as a Community Publisher 39 Part 2 Trends & Essentials in ScholarlyLibrary Publishing Toolkit Edited by Allison P. Brown #12;Library Publishing Toolkit Edited

  10. 17 Years of Lithium Brown Dwarfs 10/21/12Ringberg Brown Dwarfs 1

    E-Print Network [OSTI]

    Joergens, Viki

    17 Years of Lithium Brown Dwarfs 10/21/12Ringberg Brown Dwarfs 1 #12;The Keck Search for Lithium 10/21/12Ringberg Brown Dwarfs 2 Lithium was not seen in objects which should have been comfortably into the brown "lithium dating". This adjustment in age meant that the inferred mass of PPl 15 rose to near the substellar

  11. Evaluation of the Dallas Thompson Riverscreen Site on the Touchet River.

    SciTech Connect (OSTI)

    Chamness, Mickie [Pacific Northwest National Laboratory

    2007-07-25

    Riverscreen irrigation pumps are a relatively new design in which the pump intake floats on the river surface, pulling water in only from the bottom side and surrounded by a self-cleaning screen. The Walla Walla County Conservation District recently started replacing old pump screens with the Riverscreen and was interested in whether the screens are protective of juvenile salmonids. Pacific Northwest National Laboratory evaluated approach velocities and operations at the Riverscreen installation on the Dallas Thompson property, approximately 3 mi. north of Touchet, Washington and 300 ft north of Hofer Dam, on June 18, 2007. Evaluation of this site consisted of underwater videography and water velocity measurements. The Dallas Thompson Riverscreen was pumping approximately 930 gpm during our evaluation, which is close to the maximum pumping rate for this model. Underwater videography showed only slow movement of water-borne particulates toward the pump intake, and the screen material was clean. All water velocity measurements were taken below the pump intake opening and between 3 to 6 in. from the screen face. All approach velocities (flow toward the screen and pump) were below National Marine Fisheries Service draft guidelines for juvenile fish screens.

  12. L. Frank Brown, Jr. Publications

    E-Print Network [OSTI]

    Yang, Zong-Liang

    (Upper Pennsylvanian), northern Stephens County, Texas: The University of Texas at Austin, Bureau., and Erxleben, A. W., 1973, Pennsylvanian depositional systems in North-Central Texas: a guide for interpretingL. Frank Brown, Jr. Publications July 8, 2008 Business address: The University of Texas at Austin

  13. A Comparison of Static and Dynamic Traffic Assignment Under Tolls: A Study of the Dallas-Fort Worth Network

    E-Print Network [OSTI]

    Kockelman, Kara M.

    A Comparison of Static and Dynamic Traffic Assignment Under Tolls: A Study of the Dallas-Fort Worth, most of the work in the literature uses static transportation models for analysis. The benefits comparison of static traffic assignment with the VISTA model, a simulation-based dynamic traffic assignment

  14. Brown DwarfBrown Dwarf Brown Dwarf White Dwarf White Dwarf White Dwarf

    E-Print Network [OSTI]

    Bechtold, Jill

    the mass needed for hydrogen fusion. Mass: StarPower Points: 2 Small dim barely detectable ball: 0.5 - 1.4 SM StarPower Points: 6 Medium size star with enough mass to support nuclear fusion Yellow Dwarf Small dim barely detectable ball of gas. When brown dwarf stars form they do not have

  15. Using Narrow Band Photometry to Classify Stars and Brown Dwarfs

    E-Print Network [OSTI]

    A. K. Mainzer; Ian S. McLean; J. L. Sievers; E. T. Young

    2003-12-05

    We present a new system of narrow band filters in the near infrared that can be used to classify stars and brown dwarfs. This set of four filters, spanning the H band, can be used to identify molecular features unique to brown dwarfs, such as H2O and CH4. The four filters are centered at 1.495 um (H2O), 1.595 um (continuum), 1.66 um (CH4), and 1.75 um (H2O). Using two H2O filters allows us to solve for individual objects' reddenings. This can be accomplished by constructing a color-color-color cube and rotating it until the reddening vector disappears. We created a model of predicted color-color-color values for different spectral types by integrating filter bandpass data with spectra of known stars and brown dwarfs. We validated this model by making photometric measurements of seven known L and T dwarfs, ranging from L1 - T7.5. The photometric measurements agree with the model to within +/-0.1 mag, allowing us to create spectral indices for different spectral types. We can classify A through early M stars to within +/-2 spectral types, late-type M and L dwarfs to within +/-0.3 spectral types and T dwarfs to within +/-0.1 spectral types 1-sigma. Thus, we can distinguish between a T1 and a T3 dwarf. The four physical bands can be converted into two reddening-free indices, mu1 and mu2, and an extinction, AV, for the individual object. This technique, which is equivalent to extremely low resolution spectroscopy, can be used to survey large areas to provide rough spectral classifications for all the stars in the area, ranging down to the coolest brown dwarfs. It should prove particularly useful in young clusters where reddening can be high.

  16. Farm Boys' and Girls' Education Encampment at the State Fair of Texas, Dallas, October 14th to 29th, 1916: A Week of Practical Education and Pleasure Combined. 

    E-Print Network [OSTI]

    Anonymous,

    1916-01-01

    week. 4. Sutlicient money for personal incidental expenses. ~ · Any girl whodesires, may send these articles by prepaid express to Miss Bernice Carter, care of Farmer Girls' Encampment, State Fair of Texas, Dallas, Texas. UNIFORMS The State Fair...

  17. Edmund G. Brown Jr. LIGHTING CALIFORNIA'S FUTURE

    E-Print Network [OSTI]

    Edmund G. Brown Jr. Governor LIGHTING CALIFORNIA'S FUTURE: SMART LIGHT-EMITTING DIODE LIGHTING's Future: Smart LightEmitting Diode Lighting in Residential Fans. California Energy Commission, PIER

  18. Systems and Professional Development - David Brown, Director...

    Energy Savers [EERE]

    Workload DOE's Certified Workforce Acquisition Workload The Holy Grail of Contract and Project Management More... Workshop 2015 - BrownSystems & Professional Development.pdf...

  19. Searching for Weather in Brown Dwarfs

    E-Print Network [OSTI]

    C. G. Tinney; A. J. Tolley

    1998-11-17

    We have used an innovative tuneable filter technique to carry out a search for the variability signatures of meterological processes in the atmospheres of two nearby brown dwarfs. We find no evidence for variability in the L-type brown dwarf DENIS-PJ1228-1547 in an observations spanning approximately half a rotation period (3 hours), and evidence for variability in the M-type brown dwarf LP 944-20 in multiple observations spanning approximately one third of a rotation period (1.5 hours).

  20. MICROLENSING BINARIES WITH CANDIDATE BROWN DWARF COMPANIONS

    SciTech Connect (OSTI)

    Shin, I.-G.; Han, C. [Department of Physics, Institute for Astrophysics, Chungbuk National University, Cheongju 371-763 (Korea, Republic of); Gould, A.; Skowron, J. [Department of Astronomy, Ohio State University, 140 W. 18th Ave., Columbus, OH 43210 (United States); Udalski, A.; Szymanski, M. K.; Kubiak, M.; Soszynski, I.; Pietrzynski, G.; Poleski, R.; Ulaczyk, K.; Pietrukowicz, P.; Kozlowski, S.; Wyrzykowski, L. [Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa (Poland); Sumi, T. [Department of Earth and Space Science, Osaka University, Osaka 560-0043 (Japan); Dominik, M. [SUPA, University of St. Andrews, School of Physics and Astronomy, North Haugh, St. Andrews KY16 9SS (United Kingdom); Beaulieu, J.-P. [Institut d'Astrophysique de Paris, UMR7095 CNRS-Universite Pierre and Marie Curie, 98 bis boulevard Arago, F-75014 Paris (France); Tsapras, Y. [Las Cumbres Observatory Global Telescope Network, 6740B Cortona Dr., Suite 102, Goleta, CA 93117 (United States); Bozza, V. [Dipartimento di Fisica 'E. R. Caianiello', Universita degli Studi di Salerno, Via S. Allende, I-84081 Baronissi (Italy); Abe, F. [Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya 464-8601 (Japan); Collaboration: OGLE Collaboration; MOA Collaboration; muFUN Collaboration; and others

    2012-12-01

    Brown dwarfs are important objects because they may provide a missing link between stars and planets, two populations that have dramatically different formation histories. In this paper, we present the candidate binaries with brown dwarf companions that are found by analyzing binary microlensing events discovered during the 2004-2011 observation seasons. Based on the low mass ratio criterion of q < 0.2, we found seven candidate events: OGLE-2004-BLG-035, OGLE-2004-BLG-039, OGLE-2007-BLG-006, OGLE-2007-BLG-399/MOA-2007-BLG-334, MOA-2011-BLG-104/OGLE-2011-BLG-0172, MOA-2011-BLG-149, and MOA-201-BLG-278/OGLE-2011-BLG-012N. Among them, we are able to confirm that the companions of the lenses of MOA-2011-BLG-104/OGLE-2011-BLG-0172 and MOA-2011-BLG-149 are brown dwarfs by determining the mass of the lens based on the simultaneous measurement of the Einstein radius and the lens parallax. The measured masses of the brown dwarf companions are 0.02 {+-} 0.01 M {sub Sun} and 0.019 {+-} 0.002 M {sub Sun} for MOA-2011-BLG-104/OGLE-2011-BLG-0172 and MOA-2011-BLG-149, respectively, and both companions are orbiting low-mass M dwarf host stars. More microlensing brown dwarfs are expected to be detected as the number of lensing events with well-covered light curves increases with new-generation searches.

  1. NOx, SOx and CO2 Emissions Reduction from Continuous Commissioning® (CC®) Measures at the Rent-A-Car Facility in the Dallas-Fort Worth International Airport 

    E-Print Network [OSTI]

    Baltazar-Cervantes, J. C.; Haberl, J. S.; Yazdani, B.

    2006-10-27

    The Energy Systems Laboratory (ESL) at the Texas Engineering Experiment Station, Texas A&M University System was contracted to fulfill a Continuous Commissioning® (CC®)project on the Rent-a-Car facility (RAC) of the Dallas-Fort Worth International...

  2. BANDO PER IL RECLUTAMENTO DI UN RICERCATORE CON RAPPORTO DI LAVORO A TEMPO DETERMINATO CO FINANZIATO DALLA REGIONE LAZIO PER IL SETTORE S/D

    E-Print Network [OSTI]

    Di Pillo, Gianni

    FINANZIATO DALLA REGIONE LAZIO PER IL SETTORE S/D BIO/09 PRESSO IL DIPARTIMENTO DI FISIOLOGIA E FARMACOLOGIA "VITTORIO ERSPAMER" Il Direttore del Dipartimento di Fisiologia e Farmacologia "Vittorio Erspamer" Visto il Regione Lazio Viste le Delibere del Consiglio del Dipartimento di Fisiologia e Farmacologia "Vittorio

  3. FIA-12-0009- In the Matter of Cynthia Brown

    Broader source: Energy.gov [DOE]

    Cynthia Brown filed an Appeal regarding a request she filed under the Freedom of Information Act. In December 2011, Ms. Brown filed a request for records regarding her late mother.

  4. Non-equilibrium Chemistry in Brown Dwarf Atmospheres

    E-Print Network [OSTI]

    Metchev, Stanimir

    Non-equilibrium Chemistry in Brown Dwarf Atmospheres PHY688 Aaron Jackson April 27, 2009 #12 and convection #12;Non-equilibrium Chemistry In the context of Brown Dwarf Atmospheres, the relevant chemical;Outline What is non-equilibrium chemistry in the context of Brown Dwarfs? What is the observational

  5. Hanbury BrownTwiss effect with partially coherent electromagnetic beams

    E-Print Network [OSTI]

    Visser, Taco D.

    Hanbury Brown­Twiss effect with partially coherent electromagnetic beams Gaofeng Wu1,2 and Taco D fluctuations (the Hanbury Brown­Twiss effect) at two points in the same cross section of a random electro; (260.5430) Polarization. http://dx.doi.org/10.1364/OL.39.002561 Ever since Hanbury Brown­Twiss (HBT

  6. Update 2-10 Martin J. Brown

    E-Print Network [OSTI]

    procurement, logistics and travel policy and oversight to the Department. Brown was a Rear Admiral in the Navy from 2004 - 2007 and served as the Competition Advocate General of the Navy and was the Deputy Assistant Secretary of the Navy (Acquisition Management) for the Assistant Secretary of the Navy (Research

  7. Chemistry of Atmospheric Brown Carbon Alexander Laskin,*,

    E-Print Network [OSTI]

    Nizkorodov, Sergey

    Chemistry of Atmospheric Brown Carbon Alexander Laskin,*, Julia Laskin,*, and Sergey A. Nizkorodov fraction of atmospheric aerosol and has profound effects on air quality, atmospheric chemistry, and climate of radiation through Earth's atmosphere. The cloud albedo effect, Special Issue: 2015 Chemistry in Climate

  8. Radial Velocity Variability of Field Brown Dwarfs

    E-Print Network [OSTI]

    Prato, L; Rice, E L; McLean, I S; Kirkpatrick, J D; Burgasser, A J; Kim, S S

    2015-01-01

    We present paper six of the NIRSPEC Brown Dwarf Spectroscopic Survey, an analysis of multi-epoch, high-resolution (R~20,000) spectra of 25 field dwarf systems (3 late-type M dwarfs, 16 L dwarfs, and 6 T dwarfs) taken with the NIRSPEC infrared spectrograph at the W. M. Keck Observatory. With a radial velocity precision of ~2 km/s, we are sensitive to brown dwarf companions in orbits with periods of a few years or less given a mass ratio of 0.5 or greater. We do not detect any spectroscopic binary brown dwarfs in the sample. Given our target properties, and the frequency and cadence of observations, we use a Monte Carlo simulation to determine the detection probability of our sample. Even with a null detection result, our 1 sigma upper limit for very low mass binary frequency is 18%. Our targets included 7 known, wide brown dwarf binary systems. No significant radial velocity variability was measured in our multi-epoch observations of these systems, even for those pairs for which our data spanned a significant ...

  9. Africa House PATRICK BROWN, Faculty Director

    E-Print Network [OSTI]

    Hayden, Nancy J.

    Africa House PATRICK BROWN, Faculty Director LOKANGAKA LOSAMBE, Faculty Director PIERRETTE LUMUMBA of African cultures' role in the world. Africa House will be a valuable program in helping students develop component, Africa House offers students shared experiences as well as opportunities for participation

  10. Disks around Brown Dwarfs and Cool Stars

    E-Print Network [OSTI]

    Daniel Apai; Kevin Luhman; Michael Liu

    2007-02-10

    We review the current picture of disks around cool stars and brown dwarfs, including disk fractions, mass estimates, disk structure and dispersal, accretion, dust composition, and the debris disk phase. We discuss these in the framework of recent planet formation models.

  11. A companion to AB Pic at the planet/brown dwarf boundary

    E-Print Network [OSTI]

    G. Chauvin; A. -M. Lagrange; B. Zuckerman; C. Dumas; D. Mouillet; I. Song; J. -L. Beuzit; P. Lowrance; M. S. Bessell

    2005-04-29

    We report deep imaging observations of the young, nearby star AB Pic, a member of the large Tucana-Horologium as sociation. We have detected a faint, red source 5.5" South of the star with JHK colors compatible with that of a young substellar L dwarf. Follow-up observations at two additional epochs confirm, with a confidence level of 4.7sigma, that the faint red object is a companion to AB Pic rather than it being a stationary background object. A low resolution K-band spectrum indicates an early-L spectral type for the companion. Finally, evolutionary model predictions based on the JHK photometry of AB Pic b indicate a mass of 13 to 14 MJup if its age is ~30Myr. Is AB Pic b a massive planet or a minimum mass brown dwarf?

  12. 9/25/10 12:27 PMLEED certification efforts remain strong -Dallas Business Journal Page 1 of 2http://www.bizjournals.com/dallas/stories/2010/08/02/story3.html?s=industry&b=1280721600%5E3731231&t=printable

    E-Print Network [OSTI]

    sessions early in the design process to encourage them to set energy-efficient targets that the design team building, sustainability as keys to success even in economic downturn Dallas Business Journal - by Lena. Revenue from green building projects made up half of the $240 million total gross revenue for HKS in 2009

  13. Foreword to Special Issue: Papers from the 50th Annual Meeting of the APS Division of Plasma Physics, Dallas, Texas, 2008

    SciTech Connect (OSTI)

    Bhattacharjee, Amitava; Davidson, Ronald C.

    2009-05-15

    The year 2008 marked the 50th Anniversary of the Division of Plasma Physics (DPP) of the American Physical Society. This Special Issue presents many of the Review, Tutorial, and Invited papers that were presented at the 2008 Annual Meeting of the DPP, which was held 17-21 November, in Dallas, Texas. We are very pleased that many of the speakers have submitted an archival-quality version of their presentation for peer review and publication in Physics of Plasmas.

  14. MEMORANDUM FROM: THOMAS E. BROWN, DIRECTOR OFFICE OF CONTRACT...

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

    ,2008 MEMORANDUM FROM: THOMAS E. BROWN, DIRECTOR OFFICE OF CONTRACT MANAGEMENT OFFICE OF PROCUREMENT AND ASSISTANCE MANAGEMENT SUBJECT: Contract Change Order Administration of...

  15. Mid-infrared followup of cold brown dwarfs: diversity in age, mass and metallicity

    SciTech Connect (OSTI)

    Saumon, Didier; Leggett, Sandy K; Burningham, Ben; Marley, Mark S; Waren, S J; Jones, H R A; Pinfield, D J; Smart, R L

    2009-01-01

    We present new Spitzer IRAC [3.6], [4.5], [5.8] and [8.0] photometry of nine very late-type T dwarfs. Combining this with previously published photometry, we investigate trends with type and color that are useful for both the planning and interpretation of infrared surveys designed to discover the coldest T or Y dwarfs. Brown dwarfs with effective temperature (T{sub eff}) below 700 K emit more than half their flux at wavelengths longer than 3 {micro}m, and the ratio of the mid-infrared flux to the near-infrared flux becomes very sensitive to T{sub eff} at these low temperatures. We confirm that the color H (1.6 {micro}m) - [4.5] is a good indicator of T{sub eff} with a relatively weak dependence on metallicity and gravity. Conversely, the colors H - K (2.2 {micro}m) and [4.5] - [5.8] are sensitive to metallicity and gravity. Thus near- and mid-infrared photometry provide useful indicators of the fundamental properties of brown dwarfs, and if temperature and gravity are known, then mass and age can be reliably determined from evolutionary models. There are twelve dwarfs currently known with H - [4.5] > 3.0, and {approx} 500 < T{sub eff} K {approx}< 800, which we examine in detail. The ages of the dwarfs in the sample range from very young (0.1 - 1.0 Gyr) to relatively old (3 - 12 Gyr). The mass range is possibly as low as 5 Jupiter masses to up to 70 Jupiter masses, i.e. near the hydrogen burning limit. The metallicities also span a large range, from [m/H]= -0.3 to [m/H]= +0.2. The small number of T8 - T9 dwarfs found in the UKIRT Infrared Deep Sky Survey to date appear to be predominantly young low-mass dwarfs. Accurate mid-infrared photometry of cold brown dwarfs is essentially impossible from the ground, and extensions to the mid-infrared space missions warm-Spitzer and WISE are desirable in order to obtain the vital mid-infrared data for cold brown dwarfs, and to discover more of these rare objects.

  16. Women @ Energy: Nancy Brown | Department of Energy

    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX E LIST OFAMERICA'S FUTURE.Energy Wind Power Today,CarolKarenWomenNancy Brown Women @

  17. Light brown apple moth’s arrival in California worries commodity groups

    E-Print Network [OSTI]

    Varela, Lucia G.; Johnson, Marshall W; Strand, Larry; Wilen, Cheryl A; Pickel, Carolyn

    2008-01-01

    control of light brown apple moth, Epi- phyas postvittana (2007a. Light brown apple moth host list. www.cdfa.ca.gov/p. CDFA. 2007b. Light brown apple moth project: Advisories.

  18. ORIGINAL RESEARCH Introgression of Brown Norway Chromosome 1 onto the Fawn

    E-Print Network [OSTI]

    Helmstetter, Fred J.

    ORIGINAL RESEARCH Introgression of Brown Norway Chromosome 1 onto the Fawn Hooded Hypertensive (FHH) and Brown Norway (BN) parent strains with a Brown Norway chromosome 1 substitution on the FHH

  19. Publications of Richard E. Brown Refereed Journal Articles

    E-Print Network [OSTI]

    Status of Office Equipment in the USA." Energy. vol. 31, no. 14. (also LBNL-57470). November. pp. 2823-2838. Brown, Richard E., and Jonathan G. Koomey. 2003. "Electricity Use in California: Past Trends and Present, Bruce Nordman, Richard E. Brown, Maryann Piette, Michael Ting, and Alan Meier. 2002. "Electricity Used

  20. BrownMap: Enforcing Power Budget in Shared Data Centers

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    BrownMap: Enforcing Power Budget in Shared Data Centers Akshat Verma, Pradipta De, Vijay Mann, we investigate mechanisms to ensure that a shared data center can operate within a power budget). We present the BrownMap methodology that is able to ensure that data centers can deal both

  1. Boiler Gold Rush Prof. Johnny Brown (MATH 700)

    E-Print Network [OSTI]

    Brown, Johnny E.

    Boiler Gold Rush Prof. Johnny Brown (MATH 700) jeb@math.purdue.edu #12;#12;#12;David McCullough, Jr help Always be prepared #12;Boiler Gold Rush Prof. Johnny Brown (MATH 700) jeb@math.purdue.edu #12;

  2. Biosorption of Trivalent Chromium on the Brown Seaweed Biomass

    E-Print Network [OSTI]

    Volesky, Bohumil

    Biosorption of Trivalent Chromium on the Brown Seaweed Biomass Y E O U N G - S A N G Y U N , D O N brown alga Ecklonia biomass as a model system. Titration of the biomass revealed that it contains that various biosorbents are able to effectively remove chromium (4-11). Some of the biomass types have

  3. Novel Solvent System for Post Combustion CO{sub 2} Capture Brown...

    Office of Scientific and Technical Information (OSTI)

    COsub 2 Capture Brown, Alfred; Brown, Nathan 20 FOSSIL-FUELED POWER PLANTS Clean Coal Technology Coal - Environmental (Carbon Capture) Clean Coal Technology Coal -...

  4. Abiotic and biotic factors affecting light brown apple moth, Epiphyas postvittana, in California

    E-Print Network [OSTI]

    Buergi, Linda Patricia

    2012-01-01

    mortality of lightbrown apple moth. In: O’Callaghan, M. (tryoni and the light brown apple moth Epiphyas postvittanaof the light brown apple moth, Epiphyas postvittana (

  5. Home sweet home: Texas A&M AgriLife opens the first WaterSense-labeled house in Dallas-Fort Worth 

    E-Print Network [OSTI]

    Lee, Leslie

    2013-01-01

    2013 Story by Leslie Lee Photo by Leslie Lee, Texas Water Resources Institute. Home sweet home Texas A&M AgriLife opens the ?rst WaterSense-labeled house in Dallas-Fort Worth On any given evening in the ????s, a?er a long day of working...-foot ?oor plan, the ??-year-old home wouldn?t have looked like much of an a?raction. But today, a?er a water-minded renovation of the once-abandoned house, the thousands of visitors who have toured it this year would probably disagree. ?e ???? version...

  6. Potsdam Thinkshop Poster Proceedings, p. 4345 Rotational periods of very young brown dwarfs in Cha I

    E-Print Network [OSTI]

    Joergens, Viki

    telescope at ESO. We performed aperture photometry and calculated differential magnitudes by means for unevenly spaced data as in our case. The algorithm phase folds the data with a trial period and calculates modulates the total brightness of the star and leads to periodic light vari- Correspondence to: viki@mpe.mpg

  7. Genome sequence of the Brown Norway rat yields insights into

    E-Print Network [OSTI]

    Payseur, Bret

    Genome sequence of the Brown Norway rat yields insights into mammalian evolution Rat Genome Norway (BN) rat strain. The sequence represents a high-quality `draft' covering over 90% of the genome

  8. Quiescent X-ray emission from an evolved brown dwarf ?

    E-Print Network [OSTI]

    B. Stelzer

    2004-09-27

    I report on the X-ray detection of Gl569Bab. During a 25ksec Chandra observation the binary brown dwarf is for the first time spatially separated in X-rays from the flare star primary Gl569A. Companionship to Gl569A constrains the age of the brown dwarf pair to ~300-800 Myr. The observation presented here is only the second X-ray detection of an evolved brown dwarf. About half of the observing time is dominated by a large flare on Gl569Bab, the remainder is characterized by weak and non-variable emission just above the detection limit. This emission -- if not related to the afterglow of the flare -- represents the first detection of a quiescent corona on a brown dwarf, representing an important piece in the puzzle of dynamos in the sub-stellar regime.

  9. Molecular insights into the niche of harmful brown tides

    E-Print Network [OSTI]

    Wurch, Louie L. (Louie Lorne)

    2011-01-01

    Recurrent brown tide blooms caused by the harmful alga Alureococcus anophagefferens have decimated coastal ecosystems and shellfisheries along the Eastern U.S and South Africa. The exact mechanisms controlling bloom ...

  10. Intern experience at Brown & Root, Inc.: an internship report 

    E-Print Network [OSTI]

    Kibbee, Stephen Edward, 1951-

    2013-03-13

    To document that the objectives of the internship were met, the report examines the organizational approach at Brown & Root and then describes seven major job assignments that were completed by the author during ...

  11. Edmund G. Brown, Jr. ENERGY-EFFICIENT COMMUNITY

    E-Print Network [OSTI]

    Virginia Lew Office Manager ENERGY EFFICINECY RESEARCH OFFICE Laurie ten Hope Deputy Director ENERGYEdmund G. Brown, Jr. Governor ENERGY-EFFICIENT COMMUNITY DEVELOPMENT IN CALIFORNIA: CHULA VISTA PIERFINALPROJECTREPORTPrepared For: California Energy Commission Public Interest Energy Research Program Prepared By: National

  12. PIECEWISELINEAR DIFFUSION PROCESSES Sid Browne and Ward Whitt

    E-Print Network [OSTI]

    Whitt, Ward

    PIECEWISE­LINEAR DIFFUSION PROCESSES by Sid Browne and Ward Whitt Graduate School of Business AT&T Bell Laboratories Columbia University Murray Hill, NJ 07974­0636 New York, NY 10027 May 17, 1994 #12

  13. MiR-193b-365, a brown fat enriched microRNA cluster, is essential for brown fat differentiation

    E-Print Network [OSTI]

    Sun, Lei

    Mammals have two principal types of fat. White adipose tissue primarily serves to store extra energy as triglycerides, whereas brown adipose tissue is specialized to burn lipids for heat generation and energy expenditure ...

  14. Parallaxes of Brown Dwarfs at USNO

    E-Print Network [OSTI]

    H. C. Harris; C. C. Dahn; F. J. Vrba; H. H. Guetter; B. Canzian; A. A. Henden; S. E. Levine; C. B. Luginbuhl; A. K. B. Monet; D. G. Monet; J. R. Pier; R. C. Stone; R. L. Walker

    2002-07-31

    Trigonometric parallaxes have been measured by Dahn et al. (2002) for 28 cool dwarfs and brown dwarfs, including 17 L dwarfs and three T dwarfs. Broadband CCD and near-IR photometry (VRIz*JHK) have been obtained for these objects and for 24 additional late-type dwarfs. These data have been supplemented with astrometry and photometry from the literature, including parallaxes for the brighter companions of ten L and two T dwarfs. The absolute magnitudes and colors are reviewed here. The I-J color and the spectral type are both good predictors of absolute magnitude for late-M and L dwarfs. M_J becomes monotonically fainter with I-J color and with spectral type through late-L dwarfs, then brightens for early-T dwarfs. In contrast, the J-K color correlates poorly with absolute magnitude for L dwarfs. Using several other parameters from the literature (Li detection, H-alpha emission strength, projected rotation velocity, and tangential velocity), we fail to uncover any measurable parameter that correlates with the anomalous J-K color.

  15. Sponsorship Packet Young Alumni Night

    E-Print Network [OSTI]

    Arnold, Jonathan

    Sponsorship Packet 2015 Young Alumni Night at SweetWater Brewing Company #12;UGA Young Alumni Night at SweetWater Brewing Company 2015 Sponsorship Opportunities Silver Sponsor - $500 Logo on UGA Young Alumni at SweetWater Brewing Company 2015 Sponsorship Opportunities (company or individual name as it should

  16. A review of "Thomas Browne" edited by Kevin Killeen 

    E-Print Network [OSTI]

    Black, Joseph L.

    2015-01-01

    vision of Christ all mark him as a student of John Donne and a hyperbolic advocate of Christianity. It is time to recognize his achievement and restore him to the canon of great seventeenth-century English poets. Kevin Killeen, ed. Thomas Browne. 21st... admired, had been largely relegated by the academy to the category of literary curiosity (according to the editors of Sir Thomas Browne: The World Proposed) and increasingly in danger of disappearing from the teaching canon. This volume’s editor, Kevin...

  17. Non-equilibrium chemistry in the atmospheres of brown dwarfs

    E-Print Network [OSTI]

    D. Saumon; M. S. Marley; K. Lodders; R. S. Freedman

    2002-07-02

    Carbon monoxide and ammonia have been detected in the spectrum of Gl 229B at abundances that differ substantially from those obtained from chemical equilibrium. Vertical mixing in the atmosphere is a mechanism that can drive slowly reacting species out of chemical equilibrium. We explore the effects of vertical mixing as a function of mixing efficiency and effective temperature on the chemical abundances in the atmospheres of brown dwarfs and on their spectra. The models compare favorably with the observational evidence and indicate that vertical mixing plays an important role in brown dwarf atmospheres.

  18. From Nash and Brown to Maynard Smith: Equilibria, Dynamics, and ESS

    E-Print Network [OSTI]

    Hofbauer, Josef

    From Nash and Brown to Maynard Smith: Equilibria, Dynamics A-1090 Vienna, Austria Abstract Nash's three, and the Brown-von Neumann-Nash dynamics. We prove that an equilibrium which is evolutionarily stable as d

  19. Effects of Brown v. Board of Education on the growth of social psychology 

    E-Print Network [OSTI]

    Bryant, William Howard McKinley

    1995-01-01

    This study probed the effects of Brown v. Board of Education on the growth of social psychology and psychology in general. Brown v. Board of Education, the 1954 landmark case that made segregation illegal and ended the ...

  20. Flowing with the Tide:Epiphytic Host-Specificity and Phenotypic Plasticity of the Brown Alga Padina boryana

    E-Print Network [OSTI]

    Flynn, Sierra Michelle

    2011-01-01

    PLASTICITY OF THE BROWN ALGA PADINA BORYANA SIERRA M. FLYNN94720 USA Abstract. Epiphytic algae form complex communitiesmacroalgae hosts. The brown alga Padina boryana acts as a

  1. TransferRule Induction for ExampleBased Translation Ralf D. Brown

    E-Print Network [OSTI]

    Brown, Ralf

    ­Based Machine Translation (EBMT) systems such as those of Veale and Way (1997) and the author (Brown, 1999) have

  2. Value of Cotton: Address Before the Farmers Congress, College Station, Texas, August 3, 1915, by Nathan Adams, Cashier, American National Exchange Bank, Dallas, Texas. Cotton Supply and Demand, August 2, 1915, Letter to Hon. D. W. Lewis, Farmers Union Convention, Houston, Texas. 

    E-Print Network [OSTI]

    Adams, Nathan; Ousley, Clarence

    1915-01-01

    AND MECHANICAL. COLLEGE OF TEXAS. AUGUST, 1915. EXTENSION SERVICE BULLBTIN B 7. VALUE OF COTTON Address Before Farmers Congress, College Sta- tion, Texas, August 3, 1915, by Nathan Adams, Cashier, American National Exchange Bank, Dallas, Texas. Address...-operating. VALUE OF COTTON. Address by Nathan Adams, Cashier, American National Exchange Bank, Dallas, Texas, Before Texas Farmers' Congress, College Station, Texas, August 3, 1915. Mr. President, Ladies and Gentlemen: It affords me a great deal of pleasure...

  3. Photoprotection in the brown alga Macrocystis pyrifera: Evolutionary implications Ernesto Garcia-Mendoza a,

    E-Print Network [OSTI]

    Govindjee

    Photoprotection in the brown alga Macrocystis pyrifera: Evolutionary implications Ernesto Garcia xxxx Keywords: Brown algae Evolution Macrocystis pyrifera Non-photochemical quenching Photoprotection-photochemical quenching, NPQ) in the brown alga Macrocystis pyrifera with that of Ficus sp., a higher plant to examine

  4. Toward Systems Biology in Brown Algae to Explore Acclimation and Adaptation to the Shore Environment

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    Toward Systems Biology in Brown Algae to Explore Acclimation and Adaptation to the Shore,2 Catherine Boyen,1,2 and Anne Siegel4,5 Abstract Brown algae belong to a phylogenetic lineage distantly siliculosus as a model organism for brown algae has represented a framework in which several omics techniques

  5. Light brown apple moth (LBAM) (Epiphyas postvittana) is an important invasive leafroller pest

    E-Print Network [OSTI]

    Ishida, Yuko

    Light brown apple moth (LBAM) (Epiphyas postvittana) is an important invasive leafroller pest for Light Brown Apple Moth IN CALIFORNIA NURSERIES Eggs are not easily observed by nursery scouts or other the head. Male light brown apple moths caught in pheromone traps. e wing-color pattern of males can

  6. Commparison of the Hanbury Brown-Twiss effect for bosons and fermions

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    1 Commparison of the Hanbury Brown-Twiss effect for bosons and fermions T. Jeltes1 , J. M. Mc-sud, Campus Polytechnique RD 128, 91127 Palaiseau Cedex, France. Fifty years ago, Hanbury Brown and Twiss (HBT atoms7,8,9,10,11,12,13 . It goes back to the discovery by Hanbury Brown and Twiss1 , that photons

  7. ccsd00001341 Hanbury-Brown Twiss correlations to probe the population

    E-Print Network [OSTI]

    ccsd­00001341 (version 1) : 23 Mar 2004 Hanbury-Brown Twiss correlations to probe the population Hanbury- Brown and Twiss correlations. The superpoissonian and poissonian photon statistics of thermal.50.Td,42.50.-p,42.50.Ar 1 #12; The seminal experiment of Hanbury-Brown and Twiss (HBT)[1], consisted

  8. The Hanbury Brown Twiss effect for atomic matter waves Christoph I. Westbrook and Denis Boiron

    E-Print Network [OSTI]

    Boyer, Edmond

    The Hanbury Brown Twiss effect for atomic matter waves Christoph I. Westbrook and Denis Boiron This paper discusses our recent work on developing the matter wave analogs to the Hanbury Brown Twiss light in the famous experiments of Robert Hanbury Brown and Richard Twiss (HBT) [4]. Although the effect

  9. Hanbury BrownTwiss Correlations to Probe the Population Statistics of GHz Photons Emitted by Conductors

    E-Print Network [OSTI]

    Plaçais, Bernard

    Hanbury Brown­Twiss Correlations to Probe the Population Statistics of GHz Photons Emitted of GHz photons in quantum circuits, using Hanbury Brown and Twiss correlations. The super The seminal experiment of Hanbury Brown and Twiss (HBT) [1], consisted in two detectors correlating the power

  10. Application of the Hanbury BrownTwiss effect to scattering from quasi-homogeneous media

    E-Print Network [OSTI]

    Visser, Taco D.

    Application of the Hanbury Brown­Twiss effect to scattering from quasi-homogeneous media David: Hanbury Brown-Twiss effect Scattering Born approximation Quasi-homogeneous media Inverse scattering a b scattering media, is studied by the use of the Hanbury Brown­Twiss effect. In particular the two

  11. Bagels: Plain & Cinnamon Raisin Cereal: Cinnamon Chex, Brown

    E-Print Network [OSTI]

    Wenderholm, Elaine

    Free Meal * Gluten Free Friendly Options Spring 2015 Alfredo Sauce Brown Rice Pasta Cheese Ravioli Gluten Free Meals or Menu Planning? Contact our Registered Dietitian, Sarah Formoza at x3284 or Email sarah.formoza@oswego.edu Gluten Free Diet = No Wheat, Rye, Barley or Malt Ask a Manager: Product

  12. Air Traffic Control Using Virtual Stationary Automata Matthew D. Brown

    E-Print Network [OSTI]

    Lynch, Nancy

    Air Traffic Control Using Virtual Stationary Automata by Matthew D. Brown B.S., Massachusetts by . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Arthur C. Smith Chairman, Department Committee on Graduate Students #12;Air Traffic Control Using Virtual of Engineering Abstract As air travel has become an essential part of modern life, the air traffic control system

  13. INDIUM--2000 38.1 By Robert D. Brown, Jr.

    E-Print Network [OSTI]

    INDIUM--2000 38.1 INDIUM By Robert D. Brown, Jr. Domestic survey data and table were prepared by Carolyn F. Crews, statistical assistant. Indium production in the United States during 2000 was confined, were the major producers of indium metal and indium products in 2000. A number of smaller firms also

  14. Hydroliquefaction of Big Brown lignite in supercritical fluids 

    E-Print Network [OSTI]

    Chen, Hui

    1996-01-01

    Big Brown lignite was liquefied in a fixed bed tube reactor. Three solvents were used in the liquefaction studies, toluene, cyclohexane and methanol. Two co-solvents, tetralin and water were used with toluene. The effects of the solvents and co...

  15. Computer Science The George R. Brown School of Engineering

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    145 Computer Science The George R. Brown School of Engineering Chair Keith Cooper Professors Robert Chemistry) Professor James Tour #12;146 DEPARTMENTS / Computer Science Computer science is concerned to produce solutions to real-world computational problems. Computer science is the intellectual discipline

  16. Computer Science The George R. Brown School of Engineering

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    135 Computer Science The George R. Brown School of Engineering Chair Moshe Y. Vardi Professors Science Computer science is concerned with the study of computers and computing, focusing on algorithms. Computer science is the intellectual discipline underlying information technology, which is widely accepted

  17. Computer Science The George R. Brown School of Engineering

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    139 Computer Science The George R. Brown School of Engineering Degrees Offered: BA, BSCS, MCS, MS, and PhD Computer science is concerned with the study of computers and computing, focusingonalgorithms to real-world computational problems. Computer science is the intellectual discipline underlying

  18. Computer Science The George R. Brown School of Engineering

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    145 Computer Science The George R. Brown School of Engineering Chair Keith Cooper Professors Robert Tour researCh Professor Peter Druschel #12;146 Departments/ Computer Science Eight courses for a total Intermediate Programming COMP 280 Mathematics of Computer Science COMP 314 Applied Algorithms and Data

  19. Computer Science The George R. Brown School of Engineering

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    141 Computer Science The George R. Brown School of Engineering Degrees Offered: BA, BSCS, MCS, MS, and PhD Computer science is concerned with the study of computers and computing, focusingonalgorithmsTour #12;142 DEPARTMENTS/ Computer Science body of knowledge can be used to produce solutions to real

  20. Computer Science The George R. Brown School of Engineering

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    153 Computer Science The George R. Brown School of Engineering Chair Joe Warren Professors Robert S'Malley with Chemistry Professor James Tour researCh Professor Peter Druschel #12;154 Departments/ Computer Science Six Matrix Analysis Math and Science Courses Degrees Offered: BA, BSCS, MCS, MS, and PhD Computer science

  1. Nonparametric Regression in Exponential Families Lawrence D. Brown1

    E-Print Network [OSTI]

    Zhou, Harrison Huibin

    Nonparametric Regression in Exponential Families Lawrence D. Brown1 , T. Tony Cai2 and Harrison H. Zhou3 University of Pennsylvania and Yale University Abstract Most results in nonparametric regression we consider nonparametric regression in exponential families which include, for example, Poisson

  2. Nonparametric Regression in Exponential Families Lawrence D. Brown1

    E-Print Network [OSTI]

    Brown, Lawrence D.

    Nonparametric Regression in Exponential Families Lawrence D. Brown1 , T. Tony Cai1 and Harrison H. Zhou2 University of Pennsylvania and Yale University Abstract Most results in nonparametric regression we consider nonparametric regression in exponential families with the main focus on the natural

  3. GEORGE E. BROWN, JR. NETWORK FOR EARTHQUAKE ENGINEERING SIMULATION (NEES)

    E-Print Network [OSTI]

    Grether, Gregory

    , Los Angeles Proposal Writing Guide 1 In he University of California, Los Angeles George E. Brown, Jr that would have occurred for any specified base-level acceleration time history (assuming the properties the completion of testing. Wireless field data acquisition system that efficiently transmits data in wireless

  4. Astronomy Advisory Panel Richard Bower, Michael Brown, Anthony

    E-Print Network [OSTI]

    Crowther, Paul

    over 10 years Many UK science areas: dark energy/matter, galactic structure, transients, solar systemAstronomy Advisory Panel Richard Bower, Michael Brown, Anthony Challinor, Chris Evans, Paul O;High priority - maintain innovation Provide science for VLT, ALMA, E-ELT, SKA, GAIA, JWST, Euclid

  5. Software Reuse in High Performance Computing Shirley Browne

    E-Print Network [OSTI]

    Dongarra, Jack

    Software Reuse in High Performance Computing Shirley Browne University of Tennessee 107 Ayres Hall high performance computing architectures in the form of distributed memory mul­ tiprocessors have and cost of programming applications to run on these machines. Economical use of high performance computing

  6. Software Reuse in High Performance Computing Shirley Browne

    E-Print Network [OSTI]

    Dongarra, Jack

    Software Reuse in High Performance Computing Shirley Browne University of Tennessee 107 Ayres Hall high performance computing architectures in the form of distributed memorymul- tiprocessors have become of programming applications to run on these machines. Economical use of high performance computing and subsequent

  7. INDIUM--2001 37.1 By Robert D. Brown, Jr.

    E-Print Network [OSTI]

    INDIUM--2001 37.1 INDIUM By Robert D. Brown, Jr. Domestic survey data and tables were prepared in New York and Rhode Island, were the major producers of indium metal and indium products in 2001 products. Domestic consumption in 2001 was estimated by the U.S. Geological Survey to have increased

  8. GERMANIUM--2001 32.1 By Robert D. Brown, Jr.

    E-Print Network [OSTI]

    GERMANIUM--2001 32.1 GERMANIUM By Robert D. Brown, Jr. Domestic survey data and table were prepared. In 2001, the domestic germanium industry consisted of two zinc mining operations in Alaska and Tennessee of germanium was estimated to have remained about the same in 2001. The USGS estimated domestic germanium

  9. INDIUM--1999 37.1 By Robert D. Brown

    E-Print Network [OSTI]

    INDIUM--1999 37.1 INDIUM By Robert D. Brown Domestic survey data and tables were prepared by Carolyn F. Crews, statistical assistant. Indium production in the United States during 1999 was confined, were the major producers of indium metal and indium products in 1999. A number of smaller firms also

  10. GERMANIUM--1999 32.1 By Robert D. Brown

    E-Print Network [OSTI]

    GERMANIUM--1999 32.1 GERMANIUM By Robert D. Brown Domestic survey data and table were prepared. In 1999, the domestic germanium industry consisted of two zinc mining operations in Alaska and Tennessee in 1999, but U.S. consumption has remained steady for 3 years. The USGS estimated domestic germanium

  11. Lunchtime Brown Bag Discussions in Education Summary Fall '03

    E-Print Network [OSTI]

    Colorado at Boulder, University of

    R., P Beale, S Robertson, A Hasenfratz 9/17 - David Hammer (U Maryland) - epistemology in physics 10 / 9 others At least 25 different faculty from the physics department attended the brown bag sessions. Significant interest from other departments (APS, Engineering, Math) in various programs, particularly

  12. THE PLANE OF THE KUIPER BELT Michael E. Brown

    E-Print Network [OSTI]

    Brown, Michael E.

    THE PLANE OF THE KUIPER BELT Michael E. Brown Division of Geological and Planetary Sciences of the Kuiper belt. The derived plane has an inclination with respect to the ecliptic of 1 .86 and an ascending node of 81 .6, with a 1 error in pole position of the plane of 0 .37. The plane of the Kuiper belt

  13. The largest Kuiper belt objects Michael E. Brown

    E-Print Network [OSTI]

    Brown, Michael E.

    The largest Kuiper belt objects Michael E. Brown California Institute of Technology ABSTRACT While for the first decade of the study of the Kuiper belt, a gap existed between the sizes of the relatively small and faint Kuiper belt objects (KBOs) that were being studied and the largest known KBO, Pluto, recent years

  14. Karine Chesnel Brigham Young University

    E-Print Network [OSTI]

    Hart, Gus

    Exam committee at BYU Physics department Society member: American Physical Society (APS), The MineralsKarine Chesnel Brigham Young University Department of Physics & Astronomy N 319 ESC Provo, Utah, Department of Physics and Astronomy, Brigham Young University, Utah, USA 2007 (Jan-Dec): Visiting Researcher

  15. DE0823$-$49 is a juvenile binary brown dwarf at 20.7 pc

    E-Print Network [OSTI]

    Sahlmann, J; Martín, E L; Lazorenko, P F; Gagliuffi, D C Bardalez; Mayor, M; Ségransan, D; Queloz, D; Udry, S

    2015-01-01

    Astrometric monitoring of the nearby early-L dwarf DE0823$-$49 has revealed a low-mass companion in a 248-day orbit that was announced in an earlier work. Here, we present new astrometric and spectroscopic observations that allow us to characterise the system in detail. The optical spectrum shows LiI-absorption indicative of a young age and/or substellar mass for the primary component. The near-infrared spectrum is best reproduced by a binary system of brown dwarfs with spectral types of L1.5 $+$ L5.5 and effective temperatures of $2150\\pm100$ K and $1670\\pm140$ K. To conform with the photocentric orbit size measured with astrometry and the current understanding of substellar evolution, the system must have an age in the 80--500 Myr range. Evolutionary models predict component masses in the ranges of $M_1\\simeq0.028-0.063\\,M_\\odot$ and $M_2\\simeq0.018-0.045\\,M_\\odot$ with a mass ratio of $q\\simeq0.64-0.74$. Multi-epoch radial velocity measurements unambiguously establish the three-dimensional orbit of the sys...

  16. Helicopter Brown-Out costs the US approximately $100 M per year in casualties/fatalities and signifi-

    E-Print Network [OSTI]

    Helicopter Brown-Out costs the US approximately $100 M per year in casualties be used not only for mitigation but also to predict and avoid brown-out conditions. Helicopter Brown) data from RADARSAT-2 is analyzed for detection of soils susceptible to helicopter brown-out. He

  17. Magnetic complexity as an explanation for bimodal rotation populations among young stars

    E-Print Network [OSTI]

    Garraffo, Cecilia; Cohen, Ofer

    2015-01-01

    Observations of young open clusters have revealed a bimodal distribution of fast and slower rotation rates that has proven difficult to explain with predictive models of spin down that depend on rotation rates alone. The Metastable Dynamo Model proposed recently by Brown, employing a stochastic transition probability from slow to more rapid spin down regimes, appears to be more successful but lacks a physical basis for such duality. Using detailed 3D MHD wind models computed for idealized multipole magnetic fields, we show that surface magnetic field complexity can provide this basis. Both mass and angular momentum losses decline sharply with increasing field complexity. Combined with observation evidence for complex field morphologies in magnetically active stars, our results support a picture in which young, rapid rotators lose angular momentum in an inefficient way because of field complexity. During this slow spin-down phase, magnetic complexity is eroded, precipitating a rapid transition from weak to str...

  18. IDENTIFYING THE YOUNG LOW-MASS STARS WITHIN 25 pc. II. DISTANCES, KINEMATICS, AND GROUP MEMBERSHIP

    SciTech Connect (OSTI)

    Shkolnik, Evgenya L.; Anglada-Escude, Guillem; Liu, Michael C.; Bowler, Brendan P.; Weinberger, Alycia J.; Boss, Alan P.; Reid, I. Neill; Tamura, Motohide

    2012-10-10

    We have conducted a kinematic study of 165 young M dwarfs with ages of {approx}<300 Myr. Our sample is composed of stars and brown dwarfs with spectral types ranging from K7 to L0, detected by ROSAT and with photometric distances of {approx}<25 pc assuming that the stars are single and on the main sequence. In order to find stars kinematically linked to known young moving groups (YMGs), we measured radial velocities for the complete sample with Keck and CFHT optical spectroscopy and trigonometric parallaxes for 75 of the M dwarfs with the CAPSCam instrument on the du Pont 2.5 m Telescope. Due to their youthful overluminosity and unresolved binarity, the original photometric distances for our sample underestimated the distances by 70% on average, excluding two extremely young ({approx}<3 Myr) objects found to have distances beyond a few hundred parsecs. We searched for kinematic matches to 14 reported YMGs and identified 10 new members of the AB Dor YMG and 2 of the Ursa Majoris group. Additional possible candidates include six Castor, four Ursa Majoris, two AB Dor members, and one member each of the Her-Lyr and {beta} Pic groups. Our sample also contains 27 young low-mass stars and 4 brown dwarfs with ages {approx}<150 Myr that are not associated with any known YMG. We identified an additional 15 stars that are kinematic matches to one of the YMGs, but the ages from spectroscopic diagnostics and/or the positions on the sky do not match. These warn against grouping stars together based only on kinematics and that a confluence of evidence is required to claim that a group of stars originated from the same star-forming event.

  19. AA Dor - An Eclipsing sdOB - Brown Dwarf Binary

    E-Print Network [OSTI]

    Thomas Rauch

    2003-11-25

    AA Dor is an eclipsing, close, post common-envelope binary consisting of a sdOB primary star and an unseen secondary with an extraordinary small mass - formally a brown dwarf. The brown dwarf may have been a former planet which survived a common envelope phase and has even gained mass. A recent determination of the components' masses from results of NLTE spectral analysis and subsequent comparison to evolutionary tracks shows a discrepancy to masses derived from radial-velocity and the eclipse curves. Phase-resolved high-resolution and high-SN spectroscopy was carried out in order to investigate on this problem. We present results of a NLTE spectral analysis of the primary, an analysis of its orbital parameters, and discuss possible evolutionary scenarios.

  20. Cloudy with a Chance of Iron: Weather on Brown Dwarfs

    SciTech Connect (OSTI)

    Burgasser, Adam (UCLA) [UCLA

    2003-08-06

    Brown dwarfs are a recently discovered, yet long-contemplated, class of 'star' which bridges the gap between classical stars like the Sun and giant planets like Jupiter. The atmospheres of these objects, with observed temperatures as low as 700 K and pressures of 1-10 bar, are such that the condensation of refractory elements - iron rain and mineral snow - can occur. This has raised the possibility of meteorological phenomena occurring on these objects in the form of clouds and possibly even 'storms'. I present observed evidence for these meteorological effects and the first simple models to use 'cloud coverage' as an explanation for the observed and unexpected brightening of brown dwarfs as they cool over a narrow temperature range. I will show how the tools of planetary atmospheric science (e.g., studies of the Earth's meteorology) can provide a context for studying the atmospheres of these more distant astrophysical objects.

  1. Turnover Rates in Insular Biogeography: Effect of Immigration on Extinction Author(s): James H. Brown and Astrid Kodric-Brown

    E-Print Network [OSTI]

    Brown, James H.

    . Brown and Astrid Kodric-Brown Source: Ecology, Vol. 58, No. 2 (Mar., 1977), pp. 445-449 Published by, turnover rate is directly related to the distance between an island and the source of colonizing species: Arizona; biogeography; colonization; extinction; insular biogeography; island; turnover. INTRODUCTION More

  2. BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 33, Part 1 CONTENTS Tertiary Geologic History Geology of the Deadman Canyon 7112-Minute Quadrangle, Carbon County, Utah, Utah. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .James Douglas Smith 135 Geology

  3. Ross Woods and Dr. Shane A. Brown Department of Civil Engineering Washington State University

    E-Print Network [OSTI]

    Collins, Gary S.

    Ross Woods and Dr. Shane A. Brown Department of Civil Engineering · Washington State University al. 2007). Other Findings: · Increased Interest in careers in Science, Technology, Engineering

  4. Moderator: Doug Brown, VP CIPS Alberta 04/12/2012 Computer Science Industry Day 2012

    E-Print Network [OSTI]

    Habib, Ayman

    Moderator: Doug Brown, VP CIPS Alberta 04/12/2012 Computer Science Industry, CIO, Alberta Electric System Operator (AESO) Marlo Nielsen, Sr. Recruiting

  5. ATMOSPHERIC CIRCULATION OF BROWN DWARFS: JETS, VORTICES, AND TIME VARIABILITY

    SciTech Connect (OSTI)

    Zhang, Xi; Showman, Adam P.

    2014-06-10

    A variety of observational evidence demonstrates that brown dwarfs exhibit active atmospheric circulations. In this study we use a shallow-water model to investigate the global atmospheric dynamics in the stratified layer overlying the convective zone on these rapidly rotating objects. We show that the existence and properties of the atmospheric circulation crucially depend on key parameters including the energy injection rate and radiative timescale. Under conditions of strong internal heat flux and weak radiative dissipation, a banded flow pattern comprised of east-west jet streams spontaneously emerges from the interaction of atmospheric turbulence with the planetary rotation. In contrast, when the internal heat flux is weak and/or radiative dissipation is strong, turbulence injected into the atmosphere damps before it can self-organize into jets, leading to a flow dominated by transient eddies and isotropic turbulence instead. The simulation results are not very sensitive to the form of the forcing. Based on the location of the transition between jet-dominated and eddy-dominated regimes, we suggest that many brown dwarfs may exhibit atmospheric circulations dominated by eddies and turbulence (rather than jets) due to the strong radiative damping on these worlds, but a jet structure is also possible under some realistic conditions. Our simulated light curves capture important features from observed infrared light curves of brown dwarfs, including amplitude variations of a few percent and shapes that fluctuate between single-peak and multi-peak structures. More broadly, our work shows that the shallow-water system provides a useful tool to illuminate fundamental aspects of the dynamics on these worlds.

  6. THE BROWN DWARF KINEMATICS PROJECT (BDKP). III. PARALLAXES FOR 70 ULTRACOOL DWARFS

    SciTech Connect (OSTI)

    Faherty, Jacqueline K.; Shara, Michael M.; Cruz, Kelle L.; Burgasser, Adam J.; Walter, Frederick M.; Van der Bliek, Nicole; Vrba, Frederick J.; Anglada-Escude, Guillem

    2012-06-10

    We report parallax measurements for 70 ultracool dwarfs (UCDs) including 11 late-M, 32 L, and 27 T dwarfs. In this sample, 14 M and L dwarfs exhibit low surface gravity features, 6 are close binary systems, and 2 are metal-poor subdwarfs. We combined our new measurements with 114 previously published UCD parallaxes and optical-mid-IR photometry to examine trends in spectral-type/absolute magnitude, and color-color diagrams. We report new polynomial relations between spectral type and M{sub JHK}. Including resolved L/T transition binaries in the relations, we find no reason to differentiate between a 'bright' (unresolved binary) and a 'faint' (single source) sample across the L/T boundary. Isolating early T dwarfs, we find that the brightening of T0-T4 sources is prominent in M{sub J} where there is a [1.2-1.4] mag difference. A similar yet dampened brightening of [0.3-0.5] mag happens at M{sub H} and a plateau or dimming of [-0.2 to -0.3] mag is seen in M{sub K} . Comparison with evolutionary models that vary gravity, metallicity, and cloud thickness verifies that for L into T dwarfs, decreasing cloud thickness reproduces brown dwarf near-IR color-magnitude diagrams. However we find that a near constant temperature of 1200 {+-}100 K along a narrow spectral subtype of T0-T4 is required to account for the brightening and color-magnitude diagram of the L-dwarf/T-dwarf transition. There is a significant population of both L and T dwarfs which are red or potentially 'ultra-cloudy' compared to the models, many of which are known to be young indicating a correlation between enhanced photospheric dust and youth. For the low surface gravity or young companion L dwarfs we find that 8 out of 10 are at least [0.2-1.0] mag underluminous in M{sub JH} and/or M{sub K} compared to equivalent spectral type objects. We speculate that this is a consequence of increased dust opacity and conclude that low surface gravity L dwarfs require a completely new spectral-type/absolute magnitude polynomial for analysis.

  7. MOA-2007-BLG-197: Exploring the brown dwarf desert

    E-Print Network [OSTI]

    Ranc, C; Albrow, M D; Kubas, D; Bond, I A; Batista, V; Beaulieu, J -P; Bennett, D P; Dominik, M; Dong, Subo; Fouqué, P; Gould, A; Greenhill, J; Jørgensen, U G; Kains, N; Menzies, J; Sumi, T; Bachelet, E; Coutures, C; Dieters, S; Prester, D Dominis; Donatowicz, J; Gaudi, B S; Han, C; Hundertmark, M; Horne, K; Kane, S R; Lee, C -U; Marquette, J -B; Park, B -G; Pollard, K R; Sahu, K C; Street, R; Tsapras, Y; Wambsganss, J; Williams, A; Zub, M; Abe, F; Fukui, A; Itow, Y; Masuda, K; Matsubara, Y; Muraki, Y; Ohnishi, K; Rattenbury, N; Saito, To; Sullivan, D J; Sweatman, W L; Tristram, P J; Yock, P C M; Yonehara, A

    2015-01-01

    We present the analysis of MOA-2007-BLG-197Lb, the first brown dwarf companion to a Sun-like star detected through gravitational microlensing. The event was alerted and followed-up photometrically by a network of telescopes from the PLANET, MOA, and uFUN collaborations, and observed at high angular resolution using the NaCo instrument at the VLT. From the modelling of the microlensing light curve, we derived the binary lens separation in Einstein radius units (s~1.13) and a mass ratio of (4.732+/-0.020)x10^{-2}. Annual parallax, lens orbital motion and finite source effects were included in the models. To recover the lens system's physical parameters, we combined the resulting light curve best-fit parameters with (J,H,Ks) magnitudes obtained with VLT NaCo and calibrated using IRSF and 2MASS data. We derived a lens total mass of 0.86+/-0.04 Msun and a lens distance of 4.2+/-0.3 kpc. We find that the companion of MOA-2007-BLG-197L is a brown dwarf of 41+/-2 Mjup observed at a projected separation of 4.3+/-0.1 A...

  8. GENOMIC DNA ISOLATION FROM GREEN AND BROWN ALGAE (CAULERPALES AND FUCALES) FOR MICROSATELLITE LIBRARY CONSTRUCTION1

    E-Print Network [OSTI]

    Borges, Rita

    NOTE GENOMIC DNA ISOLATION FROM GREEN AND BROWN ALGAE (CAULERPALES AND FUCALES) FOR MICROSATELLITE A method for isolating high-quality DNA is pre- sented for the green algae Caulerpa sp. (C. racemosa, C. prolifera, and C. taxifolia) and the brown alga Sargassum muticum. These are introduced, and in- vasive

  9. Light brown apple moth Epiphyas postvittana Michigan State University's invasive species factsheets

    E-Print Network [OSTI]

    Isaacs, Rufus

    Light brown apple moth Epiphyas postvittana Michigan State University's invasive species factsheets University IPM Program and M. Philip of Michigan Department of Agriculture. The light brown apple moth and agricultural commodities. Michigan risk maps for exotic plant pests. Other common names apple leafroller

  10. Pollution-induced behavioural effects in the brown bullhead (Ameiurus nebulosus)

    E-Print Network [OSTI]

    Neff, Bryan D.

    Pollution-induced behavioural effects in the brown bullhead (Ameiurus nebulosus) Ross D. Breckels on biodiversity. Thus, it is important to understand the nature of pollution- induced change in aquatic ecosystems. We show that brown bullheads (Ameiurus nebulosus) may have evolved in response to chronic pollution

  11. Optical Flow Estimation using Laplacian Mesh Energy Wenbin Li Darren Cosker Matthew Brown Rui Tang

    E-Print Network [OSTI]

    Martin, Ralph R.

    Optical Flow Estimation using Laplacian Mesh Energy Wenbin Li Darren Cosker Matthew Brown Rui Tang.p.cosker,m.brown,r.tang}@bath.ac.uk Abstract In this paper we present a novel non-rigid optical flow algorithm for dense image correspondence and non-rigid registration. The algorithm uses a unique Laplacian Mesh Energy term to encourage local

  12. Movements of Brown Shrimp, Penaeus aztecus, and Pink Shrimp, P. duorarum, Relative to the

    E-Print Network [OSTI]

    Movements of Brown Shrimp, Penaeus aztecus, and Pink Shrimp, P. duorarum, Relative to the U.S.-Mexico Border in the Western Gulf of Mexico PETER F. SHERIDAN, FRANK J. PATELLA, Jr., NEAL BAXTER, and DENNIS A of Mexico. Annual U.S. landings of brown shrimp off Texas averaged 13,800 metric tons (t) between 1970

  13. Surprising migration and population size dynamics in ancient Iberian brown bears (Ursus arctos)

    E-Print Network [OSTI]

    Surprising migration and population size dynamics in ancient Iberian brown bears (Ursus arctos United States and northern Mexico, few bears remain in some areas in northern United States, and the species is extinct in Mexico (3). As in the Americas, the brown bear is abundant in the northern parts

  14. D. E. BROWN, R. PAUL SINGH, and R. J. COFFELT A System to Singulate

    E-Print Network [OSTI]

    D. E. BROWN, R. PAUL SINGH, and R. J. COFFELT A System to Singulate and Align Squid for Packaging time. A machine to skin and eviscerate L. opa/escens has been recently developed by Singh and Brown into this machine one by one, mantle first. An orientation device (Brooks and Singh, 1979) was used to feed squid

  15. Capping the Brown Energy Consumption of Internet Services at Low Cost

    E-Print Network [OSTI]

    Bianchini, Ricardo

    energy" (produced via carbon-intensive means) relative to renewable or "green" energy. This paper their brown energy consumption and lever- age green energy, while respecting their SLAs and minimizing energy-intensive energy as "brown" energy, in contrast with "green" or renewable energy.) We argue that placing caps

  16. Hurricane, Habitat Degradation, and Land Loss Effects on Brown Pelican Nesting Colonies

    E-Print Network [OSTI]

    Karubian, Jordan

    Hurricane, Habitat Degradation, and Land Loss Effects on Brown Pelican Nesting Colonies Scott T.J., and Leberg, P.L., 2013. Hurricane, habitat degradation, and land loss effects on Brown Pelican nesting colonies of coastal avifauna are perennially threatened by hurricanes, land loss, and environmental

  17. The Tropical Brown Alga Lobophora variegata (Lamouroux) Womersley: A Prospective Bioindicator for Ag Contamination in Tropical Coastal Waters

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    The Tropical Brown Alga Lobophora variegata (Lamouroux) Womersley: A Prospective Bioindicator determined in the brown alga Lobophora variegata, using radiotracer techniques. Results indicate that this widely distributed alga could be a useful bioindicator species for surveying silver contamination

  18. hal-00080649,version2-30Nov2006 Theory for a Hanbury Brown Twiss experiment with a

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    hal-00080649,version2-30Nov2006 Theory for a Hanbury Brown Twiss experiment with a ballistically there is no interaction between the particles. This fact was clearly demonstrated in the celebrated Hanbury Brown Twiss

  19. QER- Comment of Allen Young

    Broader source: Energy.gov [DOE]

    There is much that I can say about energy policy, but most important to me is the have no new infrastructure for fossil fuels, especially a proposed Kinder Morgan "northeast extension" pipeline through beautiful countryside in Massachusetts. There needs to be focus on renewables, plus conservation and efficiency. Allen Young

  20. Research Councils UK Engaging Young

    E-Print Network [OSTI]

    Rambaut, Andrew

    Research Councils UK Engaging Young People with Cutting Edge Research: a guide for researchers and teachers #12;Information for Researchers pages 1-8 Information for Teachers pages 9-14 Resources for Researchers and Teachers pages 15-20 #12;Research Councils UK (RCUK) support a portfolio of successful

  1. FIRE Diagnostics Kenneth M. Young

    E-Print Network [OSTI]

    first evaluation of plasmas where alpha-particle heating dominates. K. M. Young 5/2/00 #12;Simplified° Vacuum Vessel Test Cell Floor Quartz coherent fiber optic bundles Radiation Shielding Enclosure Detector Enclosure Probes Basement Floor Shielding for fiber bundles CL TFTR Escaping Alpha Diagnostic TFTR K. M

  2. YOUNG GEOLOGY GEOLOGY OF THE

    E-Print Network [OSTI]

    Seamons, Kent E.

    YOUNG GEOLOGY UNIVERSITY May, 1962 GEOLOGY OF THE SOUTHERN WASATCH MOUNTAINS AND VICIN~IM,UTAH C O ....................J. Keith Rigby 80 Economic Geology of North-Central Utah ...,............... Kcnneth C.Bdodc 85 Rod Log ........................Lehi F. Hintze, J. Ka# Ri&, & ClydeT. Hardy 95 Geologic Map of Southern

  3. Owning Hazard, A Tragedy Barbara Young Welke*

    E-Print Network [OSTI]

    Barrett, Jeffrey A.

    693 Owning Hazard, A Tragedy Barbara Young Welke* In Memory of Frances Young Welke (March 21, 1992 in the ownership of hazard from the individuals who suffered injury, to the enterprises involved in manufacturing

  4. The Brown-dwarf Atmosphere Monitoring (BAM) Project II: Multi-epoch monitoring of extremely cool brown dwarfs

    E-Print Network [OSTI]

    Rajan, A; Wilson, P A; Bulger, J; De Rosa, R J; Ward-Duong, K; Morley, C; Pont, F; Windhorst, R

    2015-01-01

    With the discovery of Y dwarfs by the WISE mission, the population of field brown dwarfs now extends to objects with temperatures comparable to those of Solar System planets. To investigate the atmospheres of these newly identified brown dwarfs, we have conducted a pilot study monitoring an initial sample of three late T-dwarfs (T6.5, T8 and T8.5) and one Y-dwarf (Y0) for infrared photometric variability at multiple epochs. With J-band imaging, each target was observed for a period of 1.0h to 4.5h per epoch, which covers a significant fraction of the expected rotational period. These measurements represent the first photometric monitoring for these targets. For three of the four targets (2M1047, Ross 458C and WISE0458), multi-epoch monitoring was performed, with the time span between epochs ranging from a few hours to ~2 years. During the first epoch, the T8.5 target WISE0458 exhibited variations with a remarkable min-to-max amplitude of 13%, while the second epoch light curve taken ~2 years later did not not...

  5. Rheological properties of water-coal slurries based on brown coal in the presence of sodium lignosulfonates and alkali

    SciTech Connect (OSTI)

    D.P. Savitskii; A.S. Makarov; V.A. Zavgorodnii

    2009-07-01

    The effect of the oxidized surface of brown coal on the structural and rheological properties of water-coal slurries was found. The kinetics of structure formation processes in water-coal slurries based on as-received and oxidized brown coal was studied. The effect of lignosulfonate and alkali additives on the samples of brown coal was considered.

  6. PHYSICAL REVIEW B 89, 045137 (2014) Hanbury Brown and Twiss correlations of Cooper pairs in helical liquids

    E-Print Network [OSTI]

    Choi, Mahn-Soo

    2014-01-01

    PHYSICAL REVIEW B 89, 045137 (2014) Hanbury Brown and Twiss correlations of Cooper pairs in helical; published 29 January 2014) We propose a Hanbury Brown and Twiss (HBT) experiment of Cooper pairs on the edge a Hanbury Brown and Twiss (HBT) experiment of Cooper pairs on the edge channels of quantum spin Hall

  7. ccsd-00001341(version1):23Mar2004 Hanbury-Brown Twiss correlations to probe the population

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    ccsd-00001341(version1):23Mar2004 Hanbury-Brown Twiss correlations to probe the population the first study of the statistics of GHz photons in quantum circuits, using Hanbury- Brown and Twiss experiment of Hanbury-Brown and Twiss (HBT)[1], consisted in two detec- tors correlating the power

  8. ATWS at Browns Ferry Unit One - accident sequence analysis

    SciTech Connect (OSTI)

    Harrington, R.M.; Hodge, S.A.

    1984-07-01

    This study describes the predicted response of Unit One at the Browns Ferry Nuclear Plant to a postulated complete failure to scram following a transient occurrence that has caused closure of all Main Steam Isolation Valves (MSIVs). This hypothetical event constitutes the most severe example of the type of accident classified as Anticipated Transient Without Scram (ATWS). Without the automatic control rod insertion provided by scram, the void coefficient of reactivity and the mechanisms by which voids are formed in the moderator/coolant play a dominant role in the progression of the accident. Actions taken by the operator greatly influence the quantity of voids in the coolant and the effect is analyzed in this report. The progression of the accident sequence under existing and under recommended procedures is discussed. For the extremely unlikely cases in which equipment failure and wrongful operator actions might lead to severe core damage, the sequence of emergency action levels and the associated timing of events are presented.

  9. ATWS analysis for Browns Ferry Nuclear Plant Unit 1

    SciTech Connect (OSTI)

    Dallman, R.J.; Jouse, W.C.

    1985-01-01

    Analyses of postulated Anticipated Transients Without Scram (ATWS) were performed at the Idaho National Engineering Laboratory (INEL). The Browns Ferry Nuclear Plant Unit 1 (BFNP1) was selected as the subject of this work because of the cooperation of the Tennessee Valley Authority (TVA). The work is part of the Severe Accident Sequence Analysis (SASA) Program of the US Nuclear Regulatory Commission (NRC). A Main Steamline Isolation Valve (MSIV) closure served as the transient initiator for these analyses, which proceeded a complete failure to scram. Results from the analyses indicate that operator mitigative actions are required to prevent overpressurization of the primary containment. Uncertainties remain concerning the effectiveness of key mitigative actions. The effectiveness of level control as a power reduction procedure is limited. Power level resulting from level control only reduce the Pressure Suppression Pool (PSP) heatup rate from 6 to 4F/min.

  10. RAMONA-3B application to Browns Ferry ATWS

    SciTech Connect (OSTI)

    Slovik, G.C.; Neymotin, L.; Cazzoli, E.; Saha, P.

    1984-01-01

    This paper discusses two preliminary MSIV clsoure ATWS calculations done using the RAMONA-3B code and the work being done to create the necessary cross section sets for the Browns Ferry Unit 1 reactor. The RAMONA-3B code employs a three-dimensional neutron kinetics model coupled with one-dimensional, four equation, nonhomogeneous, nonequilibrium thermal hydraulics. To be compatible with 3-D neutron kinetics, the code uses parallel coolant channels in the core. It also includes a boron transport model and all necessary BWR components such as jet pump, recirculation pump, steam separator, steamline with safety and relief valves, main steam isolation valve, turbine stop valve, and turbine bypass valve. A summary of RAMONA-3B neutron kinetics and thermal hydraulics models is presented in the Appendix.

  11. New Zealand lessons may aid efforts to control light brown apple moth in California

    E-Print Network [OSTI]

    Varela, Lucia G.; Walker, James T.S.; Lo, Peter L; Rogers, David J

    2010-01-01

    1975. Integrated control of apple pests in New Zealand. 1.of the light brown apple moth Epiphyas postvittana (Walker),685–92. Dumbleton L J. 1932. The apple leaf-roller (Tortrix

  12. Tracking a medically important spider: climate change, ecological niche modeling, and the brown recluse (Loxosceles reclusa)

    E-Print Network [OSTI]

    Selden, Paul A.; Saupe, Erin E.; Pape?, Monica; Vetter, Richard S.

    2011-03-01

    Most spiders use venom to paralyze their prey and are commonly feared for their potential to cause injury to humans. In North America, one species in particular, Loxosceles reclusa (brown recluse spider, Sicariidae), causes the majority of necrotic...

  13. Cholinergic neurons in the dorsomedial hypothalamus regulate mouse brown adipose tissue metabolism

    E-Print Network [OSTI]

    Jeong, Jae Hoon; Lee, Dong Kun; Blouet, Clémence; Ruiz, Henry H.; Buettner, Christoph; Chua, Streamson Jr; Schwartz, Gary J.; Jo, Young-Hwan

    2015-04-11

    Objective: Brown adipose tissue (BAT) thermogenesis is critical in maintaining body temperature. The dorsomedial hypothalamus (DMH) integrates cutaneous thermosensory signals and regulates adaptive thermogenesis. Here, we study the function...

  14. An Archaeological Survey for the Brookesmith Special Utility District Water Line Project in Brown County, Texas 

    E-Print Network [OSTI]

    Moore, William

    2015-07-30

    with the Texas Agricultural Experiment Station. Henderson, Jerry 1999 An Archaeological Survey of Proposed Water System Improvements, Brookesmith Special Utility District, Brown County, Texas. Texas Water Development Board. Hoffrichter, Norma, and Beth...

  15. Conjectured Security of the ANSI-NIST Elliptic Curve RNG Daniel R. L. Brown

    E-Print Network [OSTI]

    International Association for Cryptologic Research (IACR)

    Conjectured Security of the ANSI-NIST Elliptic Curve RNG Daniel R. L. Brown March 29, 2006 Abstract An elliptic curve random number generator (ECRNG) has been proposed in ANSI and NIST draft standards

  16. Craig Brown | Center for Gas SeparationsRelevant to Clean Energy...

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

    Smit, Berend; Long, Jeffrey R.; Brown, Craig M. Critical Factors Driving the High Volumetric Uptake of Methane in Cu-3(btc)(2). J. Amer. Chem. Soc., 137, 10816-10825 (2015)....

  17. Studying Young Stars with Large Spectroscopic Surveys

    E-Print Network [OSTI]

    Martell, Sarah L

    2015-01-01

    Galactic archaeology is the study of the history of star formation and chemical evolution in the Milky Way, based on present-day stellar populations. Studies of young stars are a key anchor point for Galactic archaeology, since quantities like the initial mass function and the star formation rate can be studied directly in young clusters and star forming regions. Conversely, massive spectroscopic Galactic archaeology surveys can be used as a data source for young star studies.

  18. Young Women's Conference in Science, Technology, Engineering...

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

    Education Organization Contact Us Programs Young Women's Conference in Science, Technology, Engineering & Mathematics Due to an overwhelming response, registration for the 2015...

  19. Adam Young | Argonne Leadership Computing Facility

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

    Young Guest Researcher Argonne National Laboratory 9700 S. Cass Avenue Building 240 Wkstn. 4D15 Argonne, IL 60439 younga@anl...

  20. Fingering convection and cloudless models for cool brown dwarf atmospheres

    E-Print Network [OSTI]

    Tremblin, P; Mourier, P; Baraffe, I; Chabrier, G; Drummond, B; Homeier, D; Venot, O

    2015-01-01

    This work aims to improve the current understanding of the atmospheres of brown dwarfs, especially cold ones with spectral type T and Y, whose modeling is a current challenge. Silicate and iron clouds are believed to disappear at the photosphere at the L/T transition, but cloudless models fail to reproduce correctly the spectra of T dwarfs, advocating for the addition of more physics, e.g. other types of clouds or internal energy transport mechanisms. We use a one-dimensional (1D) radiative/convective equilibrium code ATMO to investigate this issue. This code includes both equilibrium and out-of-equilibrium chemistry and solves consistently the PT structure. Included opacity sources are H2-H2, H2-He, H2O, CO, CO2, CH4, NH3, K, Na, and TiO, VO if they are present in the atmosphere. We show that the spectra of Y dwarfs can be accurately reproduced with a cloudless model if vertical mixing and NH3 quenching are taken into account. T dwarf spectra still have some reddening in e.g. J - H compared to cloudless mode...

  1. A new parallax measurement for the coldest known brown dwarf

    SciTech Connect (OSTI)

    Luhman, K. L.; Esplin, T. L., E-mail: kluhman@astro.psu.edu [Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802 (United States)

    2014-11-20

    WISE J085510.83–071442.5 was recently discovered as the coldest known brown dwarf based on four epochs of images from the Wide-field Infrared Survey Explorer and the Spitzer Space Telescope. We have improved the accuracy of its parallax measurement by obtaining two additional epochs of Spitzer astrometry. We derive a parallactic distance of 2.31 ± 0.08 pc, which continues to support its rank as the fourth closest known system to the Sun when compared to WISE J104915.57–531906.1 AB (2.02 ± 0.02 pc) and Wolf 359 (2.386 ± 0.012 pc). The new constraint on the absolute magnitude at 4.5 ?m indicates an effective temperature of 235-260 K based on four sets of theoretical models. We also show the updated positions of WISE J085510.83–071442.5 in two color-magnitude diagrams. Whereas Faherty and coworkers cited its location in M {sub W2} versus J – W2 as evidence of water clouds, we find that those data can be explained instead by cloudless models that employ non-equilibrium chemistry.

  2. RAMONA-3B application to Browns Ferry ATWS

    SciTech Connect (OSTI)

    Slovik, G.C.; Neymotin, L.Y.; Saha, P.

    1985-01-01

    The Anticipated Transient Without Scram (ATWS) is known to be a dominant accident sequence for possible core melt in a Boiling Water Reactor (BWR). A recent Probabilistic Risk Assessment (PRA) analysis for the Browns Ferry nuclear power plant indicates that ATWS is the second most dominant transient for core melt in BWR/4 with Mark I containment. The most dominant sequence being the failure of long term decay heat removal function of the Residual Heat Removal (RHR) system. Of all the various ATWS scenarios, the Main Steam Isolation Valve (MSIV) closure ATWS sequence was chosen for present analysis because of its relatively high frequency of occurrence and its challenge to the residual heat removal system and containment integrity. The objective of this paper is to discuss four MSIV closure ATWS calculations using the RAMONA-3B code. The paper is a summary of a report being prepared for the USNRC Severe Accident Sequence Analysis (SASA) program which should be referred to for details. 10 refs., 20 figs., 3 tabs.

  3. Baghouse Slipstream Testing at TXU's Big Brown Station

    SciTech Connect (OSTI)

    John Pavlish; Jason Laumb; Robert Jensen; Jeffery Thompson; Christopher Martin; Mark Musich; Brandon Pavlish; Stanley Miller; Lucinda Hamre

    2007-04-30

    Performing sorbent testing for mercury control at a large scale is a very expensive endeavor and requires months of planning and careful execution. Even with good planning, there are plant limitations on what operating/design parameters can be varied/tested and when. For parameters that cannot be feasibly tested at the full scale (lower/higher gas flow, different bag material, cleaning methods, sorbents, etc.), an alternative approach is used to perform tests on a slipstream unit using flue gas from the plant. The advantage that a slipstream unit provides is the flexibility to test multiple operating and design parameters and other possible technology options without risking major disruption to the operation of the power plant. Additionally, the results generated are expected to simulate full-scale conditions closely, since the flue gas used during the tests comes directly from the plant in question. The Energy & Environmental Research Center developed and constructed a mobile baghouse that allows for cost-effective testing of impacts related to variation in operating and design parameters, as well as other possible mercury control options. Multiple sorbents, air-to-cloth ratios, bag materials, and cleaning frequencies were evaluated while flue gas was extracted from Big Brown when it fired a 70% Texas lignite-30% Powder River Basin (PRB) blend and a 100% PRB coal.

  4. X-ray emitting young stars in the Orion Nebula

    E-Print Network [OSTI]

    Eric D. Feigelson; Patrick Broos; James A. Gaffney III; Gordon Garmire; Lynne A. Hillenbrand; Steven H. Pravdo; Leisa Townsley; Yohko Tsuboi

    2002-03-19

    The Orion Nebula Cluster and the molecular cloud in its vicinity have been observed with the ACIS-I detector on board the Chandra X-ray Observatory with 23 hours exposure. We detect 1075 X-ray sources: 91% are spatially associated with known stellar members of the cluster, and 7% are newly identified deeply embedded cloud members. This provides the largest X-ray study of a pre-main sequence stellar population. We examine here the X-ray properties of Orion young stars as a function of mass. Results include: (a) the discovery of rapid variability in the O9.5 31 M_o star \\theta^2A Ori, and several early B stars, inconsistent with the standard model of X-ray production in small wind shocks; (b) support for the hypothesis that intermediate-mass mid-B through A type stars do not themselves produce significant X-ray emission; (c) confirmation that low-mass G- through M-type T Tauri stars exhibit powerful flaring but typically at luminosities considerably below the `saturation' level; (d) confirmation that the presence or absence of a circumstellar disk has no discernable effect on X-ray emission; (e) evidence that T Tauri plasma temperatures are often very high with T >= 100 MK, even when luminosities are modest and flaring is not evident; and (f) detection of the largest sample of pre-main sequence very low mass objects showing high flaring levels and a decline in magnetic activity as they evolve into L- and T-type brown dwarfs.

  5. Feeding Young Horses For Sound Development 

    E-Print Network [OSTI]

    Gibbs, Pete G.; Potter, Gary D.

    2005-05-25

    Feeding Young Horses for Sound Development B-5043 05-05 Feeding Young Horses for Sound Development Pete G. Gibbs Professor and Extension Horse Specialist Department Of Animal Science Equine Sciences Program The Texas A&M University System Gary D...

  6. Astrometry and Photometry for Cool Dwarfs and Brown Dwarfs

    E-Print Network [OSTI]

    C. C. Dahn; H. C. Harris; F. J. Vrba; H. H. Guetter; B. Canzian; A. A. Henden; S. E. Levine; C. B. Luginbuhl; A. K. B. Monet; D. G. Monet; J. R. Pier; R. C. Stone; R. L. Walker; A. J. Burgasser; J. E. Gizis; J. D. Kirkpatrick; J. Liebert; I. N. Reid

    2002-05-03

    Trigonometric parallax determinations are presented for 28 late type dwarfs and brown dwarfs, including eight M dwarfs with spectral types between M7 and M9.5, 17 L dwarfs with spectral types between L0 and L8, and three T dwarfs. Broadband photometry at CCD wavelengths (VRIz) and/or near-IR wavelengths (JHK) are presented for these objects and for 24 additional late-type dwarfs. Supplemented with astrometry and photometry from the literature, including ten L and two T dwarfs with parallaxes established by association with bright, usually HIPPARCOS primaries, this material forms the basis for studying various color-color and color-absolute magnitude relations. The I-J color is a good predictor of absolute magnitude for late-M and L dwarfs. M_J becomes monotonically fainter with I-J color and with spectral type through late-L dwarfs, then brightens for early-T dwarfs. The combination of zJK colors alone can be used to classify late-M, early-L, and T dwarfs accurately, and to predict their absolute magnitudes, but is less effective at untangling the scatter among mid- and late-L dwarfs. The mean tangential velocity of these objects is found to be slightly less than that for dM stars in the solar neighborhood, consistent with a sample with a mean age of several Gyr. Using colors to estimate bolometric corrections, and models to estimate stellar radii, effective temperatures are derived. The latest L dwarfs are found to have T_eff ~ 1360 K.

  7. Variability in a Young, L/T Transition Planetary-Mass Object

    E-Print Network [OSTI]

    Biller, Beth A; Bonavita, Mariangela; Buenzli, Esther; Baxter, Claire; Crossfield, Ian J M; Allers, Katelyn; Liu, Michael C; Bonnefoy, Mickaël; Deacon, Niall; Brandner, Wolfgang; Schlieder, Joshua E; Dupuy, Trent; Kopytova, Taisiya; Manjavacas, Elena; Allard, France; Homeier, Derek; Henning, Thomas

    2015-01-01

    As part of our ongoing NTT SoFI survey for variability in young free-floating planets and low mass brown dwarfs, we detect significant variability in the young, free-floating planetary mass object PSO J318.5-22, likely due to rotational modulation of inhomogeneous cloud cover. A member of the 23$\\pm$3 Myr $\\beta$ Pic moving group, PSO J318.5-22 has T$_\\mathrm{eff}$ = 1160$^{+30}_{-40}$ K and a mass estimate of 8.3$\\pm$0.5 M$_{Jup}$ for a 23$\\pm$3 Myr age. PSO J318.5-22 is intermediate in mass between 51 Eri b and $\\beta$ Pic b, the two known exoplanet companions in the $\\beta$ Pic moving group. With variability amplitudes from 7-10$\\%$ in J$_{S}$ at two separate epochs over 3-5 hour observations, we constrain the rotational period of this object to $>$5 hours. In K$_{S}$, we marginally detect a variability trend of up to 3$\\%$ over a 3 hour observation. This is the first detection of weather on an extrasolar planetary mass object. Among L dwarfs surveyed at high-photometric precision ($<$3$\\%$) this is the...

  8. Anglers needed - Save young salmon and reel in cash

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

    Power Administration funds the program. Pikeminnow represent about 80 percent of all fish that kill young salmon. So these young salmon need your help. Each angler counts. The...

  9. CHARACTERIZATION OF THE NEARBY L/T BINARY BROWN DWARF WISE J104915.57-531906.1 AT 2 pc FROM THE SUN

    SciTech Connect (OSTI)

    Kniazev, A. Y.; Vaisanen, P.; Potter, S. B.; Crawford, S.; Gulbis, A. A. S.; Muzic, K.; Mehner, A.; Boffin, H. M. J.; Melo, C.; Ivanov, V. D.; Girard, J.; Mawet, D.; Schmidtobreick, L.; Kurtev, R.; Borissova, J.; Huelamo, N.; Minniti, D.; Ishibashi, K.; Beletsky, Y.; Buckley, D. A. H.; and others

    2013-06-20

    WISE J104915.57-531906.1 is a L/T brown dwarf binary located 2 pc from the Sun. The pair contains the closest known brown dwarfs and is the third closest known system, stellar or sub-stellar. We report comprehensive follow-up observations of this newly uncovered system. We have determined the spectral types of both components (L8 {+-} 1, for the primary, agreeing with the discovery paper; T1.5 {+-} 2 for the secondary, which was lacking spectroscopic type determination in the discovery paper) and, for the first time, their radial velocities (V{sub rad} {approx} 23.1, 19.5 km s{sup -1}) using optical spectra obtained at the Southern African Large Telescope and other facilities located at the South African Astronomical Observatory (SAAO). The relative radial velocity of the two components is smaller than the range of orbital velocities for theoretically predicted masses, implying that they form a gravitationally bound system. We report resolved near-infrared JHK{sub S} photometry from the Infrared Survey Facility telescope at the SAAO which yields colors consistent with the spectroscopically derived spectral types. The available kinematic and photometric information excludes the possibility that the object belongs to any of the known nearby young moving groups or associations. Simultaneous optical polarimetry observations taken at the SAAO 1.9 m give a non-detection with an upper limit of 0.07%. For the given spectral types and absolute magnitudes, 1 Gyr theoretical models predict masses of 0.04-0.05 M{sub Sun} for the primary, and 0.03-0.05 M{sub Sun} for the secondary.

  10. The effect of frequency on Young`s modulus and seismic wave attenuation

    SciTech Connect (OSTI)

    Price, R.H. [Sandia National Labs., Albuquerque, NM (United States). YMP Performance Assessment Applications Dept.; Martin, R.J. III; Haupt, R.W. [New England Research, Inc., White River Junction, VT (United States)

    1994-07-01

    Laboratory experiments were performed to measure the effect of frequency, water-saturation, and strain amplitude on Young`s modulus and seismic wave attenuation on rock cores recovered on or near the site of a potential nuclear waste repository at Yucca Mountain, Nevada. The purpose of this investigation is to perform the measurements using four techniques: cyclic loading, waveform inversion, resonant bar, and ultrasonic velocity. The measurements ranged in frequency between 10{sup {minus}2} and 10{sup 6} Hz. For the dry specimens Young`s modulus and attenuation were independent of frequency; that is, all four techniques yielded nearly the same values for modulus and attenuation. For saturated specimens, a frequency dependence for both Young`s modulus and attenuation was observed. In general, saturation reduced Young`s modulus and increased seismic wave attenuation. The effect of strain amplitude on Young`s modulus and attenuation was measured using the cyclic loading technique at a frequency of 10{sup {minus}1} Hz. The effect of strain amplitude in all cases was small. For some rocks, such as the potential repository horizon of the Topopah Spring Member tuff (TSw2), the effect of strain amplitude on both attenuation and modulus was minimal.

  11. BANYAN. VII. A New Population of Young Substellar Candidate Members of Nearby Moving Groups from the BASS Survey

    E-Print Network [OSTI]

    Gagné, Jonathan; Cruz, Kelle L; Lafrenière, David; Doyon, René; Malo, Lison; Burgasser, Adam J; Naud, Marie-Eve; Artigau, Étienne; Bouchard, Sandie; Gizis, John E; Albert, Loïc

    2015-01-01

    [Abbreviated] We present the results of a near-infrared (NIR) spectroscopic follow-up survey of 182 M4-L7 low-mass stars and brown dwarfs (BDs) from the BANYAN All-Sky Survey (BASS) for candidate members of nearby, young moving groups (YMGs). We confirm signs of low-gravity for 42 new BD discoveries with estimated masses between 8-75 $M_{Jup}$ and identify previously unrecognized signs of low gravity for 24 known BDs. This allows us to refine the fraction of low-gravity dwarfs in the high-probability BASS sample to $\\sim$82%. We use this unique sample of 66 young BDs, supplemented with 22 young BDs from the literature, to construct new empirical NIR absolute magnitude and color sequences for low-gravity BDs. We obtain a spectroscopic confirmation of low-gravity for 2MASS J14252798-3650229, which is a new $\\sim$27 $M_{Jup}$, L4 $\\gamma$ bona fide member of AB Doradus. We identify a total of 19 new low-gravity candidate members of YMGs with estimated masses below 13 $M_{Jup}$, seven of which have kinematically ...

  12. The field brown dwarf LP 944-20 and the Castor moving group

    E-Print Network [OSTI]

    I. Ribas

    2003-01-06

    A reliable age estimation for the field brown dwarf LP 944-20 is accomplished through the analysis of its kinematic properties. The space velocities of this star strongly suggest its membership in the so-called Castor moving group. LP 944-20 can be sensibly assumed to have the group's age, which is estimated to be ~320 Myr, and metal content, which is found to be roughly solar. With these new constrains and the available photometry and lithium abundance, current brown dwarf models are put to a test. Using the IR magnitudes and the lithium diagnostics, the models are able to provide a reasonable description of the brown dwarf's properties (to within a few sigma) but yield an age which is roughly 50% larger than our estimate. Possible reasons for this discrepancy are discussed.

  13. Effects of pretreatment in steam on the pyrolysis behavior of Loy Yang brown coal

    SciTech Connect (OSTI)

    Cai Zeng; George Favas; Hongwei Wu; Alan L. Chaffee; Jun-ichiro Hayashi; Chun-Zhu Li [Monash University, Vic. (Australia). CRC for Clean Power from Lignite, Department of Chemical Engineering

    2006-02-01

    Dewatering/drying of Victorian brown coal will be an integral part of future brown coal utilization processes aimed at the reduction of greenhouse gas emissions. This study aims to investigate the effects of the thermal pretreatment of brown coal in the presence of steam/water on its subsequent pyrolysis behavior. A Victorian (Loy Yang) brown coal was thermally pretreated in pressurized steam and inert atmospheres. The pyrolysis behavior of these pretreated coal samples was investigated in a wire-mesh reactor. While the pretreatment in steam at temperatures higher than 250{sup o}C increased the char yield of the steam-treated coal, it did not affect the overall pyrolysis char yield at 1000{sup o} C s{sup -1} if the weight loss during the pretreatment in steam was also considered. However, the tar yield decreased significantly after the pretreatment in the presence of steam. The UV-fluorescence spectroscopy of tars revealed that the release of large aromatic systems from the steam-treated coal was only affected by the pretreatment in steam if the treatment temperature was very high (e.g. 350{sup o}C). The loss of NaCl and the use of high pressure during the pretreatment of brown coal in steam were not the main reasons for the changes in the observed tar yield. The hydrolysis of O-containing structures such as ethers, esters, and carboxylates during the pretreatment in the presence of steam plays an important role in the fates of these O-containing structures during pretreatment and subsequent pyrolysis, leading to changes in the pyrolysis behavior of the brown coal. 36 refs., 8 figs.

  14. ATMOSPHERIC CHEMISTRY IN GIANT PLANETS, BROWN DWARFS, AND LOW-MASS DWARF STARS. II. SULFUR AND PHOSPHORUS

    E-Print Network [OSTI]

    ATMOSPHERIC CHEMISTRY IN GIANT PLANETS, BROWN DWARFS, AND LOW-MASS DWARF STARS. II. SULFUR AND PHOSPHORUS Channon Visscher, Katharina Lodders, and Bruce Fegley, Jr. Planetary Chemistry Laboratory to model sulfur and phosphorus chemistry in giant planets, brown dwarfs, and extrasolar giant planets (EGPs

  15. PHYSICAL REVIEW C VOLUME 49, NUMBER 1 JANUARY 1994 Hanbury-Brown --Twiss analysis in a solvable model

    E-Print Network [OSTI]

    Bertsch George F.

    PHYSICAL REVIEW C VOLUME 49, NUMBER 1 JANUARY 1994 Hanbury-Brown --Twiss analysis in a solvable of meson correlations by Hanbury-~rown --Twiss interferometry is tested with a simple model of meson the correlation function depends on the Bose symmetry of the particles as in the Hanbury-Brown --Twiss (HBT

  16. Species Diversity of Seed-Eating Desert Rodents in Sand Dune Habitats Author(s): James H. Brown

    E-Print Network [OSTI]

    Brown, James H.

    Species Diversity of Seed-Eating Desert Rodents in Sand Dune Habitats Author(s): James H. Brown DIVERSITY OF SEED-EATING DESERT RODENTS IN SAND DUNE HABITATS' JAMES H. BROWN Department of Biology, University of Utah, Salt Lake City 84112 Abstract.The seed-eatingrodent faunas were sampled on 18 dunes

  17. Operational taxonomy and (paleo-)autecology of round, brown, spiny dinoflagellate cysts from the Quaternary of high northern latitudes

    E-Print Network [OSTI]

    Pedersen, Tom

    Operational taxonomy and (paleo-)autecology of round, brown, spiny dinoflagellate cysts from determination key taxonomy paleoecology Round brown spiny dinoflagellate cysts from high latitudes a synthesis of descriptions with remarks on the mor- phology, taxonomy, nomenclature and ecology of cysts from

  18. Huff & Brown | Teaching Therac Integrating Ethics Into a Computing Curriculm: A Case Study of the Therac-25

    E-Print Network [OSTI]

    Wright, Dawn Jeannine

    Huff & Brown | Teaching Therac 1 Integrating Ethics Into a Computing Curriculm: A Case Study of the Therac-25 Chuck Huff1 and Richard Brown2 Abstract Almost all computer ethics courses use cases to some the computer science major, and in particular in the course Ethical Issues in Software Design. We then present

  19. Limits to the potential distribution of light brown apple moth in Arizona–California based on climate suitability and host plant availability

    E-Print Network [OSTI]

    Gutierrez, Andrew Paul; Mills, Nicholas J.; Ponti, Luigi

    2010-01-01

    503–531 Dumbleton LJ (1932) The apple leaf roller (TortrixJW (1937) The light-brown apple moth (Tortrix post- vittana,distribution of light brown apple moth in Arizona–California

  20. NATIONAL PRESS RELEASE I PARIS I 30 AUGUST 2013 Brown algae contain phlorotannins, aromatic (phenolic) compounds that are unique in the plant

    E-Print Network [OSTI]

    Canet, Léonie

    NATIONAL PRESS RELEASE I PARIS I 30 AUGUST 2013 Brown algae contain phlorotannins, aromatic elucidated the key step in the production of these compounds in Ectocarpus siliculosus, a small brown alga phlorotannins from brown algae for use in industry was a complex process, and the biosynthesis pathways

  1. Reassessing U.S. nuclear weapons policy Harold Brown[1] and John Deutch[2

    E-Print Network [OSTI]

    Deutch, John

    1 Reassessing U.S. nuclear weapons policy Harold Brown[1] and John Deutch[2] The end of the Cold of terrorism and the risks of nuclear proliferation, call for a reassessment of the role of nuclear weapons the goal of the complete elimination of nuclear weapons as a practical means of mobilizing more resolute

  2. EIS-0435: Modification of the Groton Generation Station Interconnection Agreement, Brown County, South Dakota

    Broader source: Energy.gov [DOE]

    This EIS evaluates the environmental impacts of a proposal for DOE's Western Area Power Administration to modify its Large Generator Connection Agreement for the Groton Generation Station in Brown County, South Dakota. The modification would allow Basin Electric Power Cooperative, which operates the generation station, to produce power above the current operating limit of 50 average megawatts.

  3. STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION

    E-Print Network [OSTI]

    1 STATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY ENERGY RESOURCES CONSERVATION AND DEVELOPMENT COMMISSION In the matter of: Preparation of the 2013 of the 2013 IEPR Scoping Order follows. Background Public Resources Code Section 25302 requires the Energy

  4. STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION

    E-Print Network [OSTI]

    STATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION 1516 Ninth Street Sacramento, California 95814 Main website: www.energy.ca.gov Notice of Availability 2011 Integrated Energy Policy Report [CEC-100-2011-001-CMF / Docket # 11-IEP-1] The 2011

  5. STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION

    E-Print Network [OSTI]

    STATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION 1516 Ninth Street Sacramento, California 95814 Main website: www.energy.ca.gov Notice of Availability Overall Program Guidebook for the Renewable Energy Program, Fourth Edition Publication No. CEC-300

  6. STATE OF CALIFORNIA --THE NATURAL RESOURCES AGENCY Edmund G. Brown, Jr., Governor CALIFORNIA ENERGY COMMISSION

    E-Print Network [OSTI]

    these laws, the Energy Commission is charged with certifying eligible renewable energy resources that may to the state's RPS under statute. Many of the RPS-eligible renewable energy resources may qualify for fundingSTATE OF CALIFORNIA -- THE NATURAL RESOURCES AGENCY Edmund G. Brown, Jr., Governor CALIFORNIA

  7. STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION

    E-Print Network [OSTI]

    STATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION 1516 Ninth Street Sacramento, California 95814 Main website: www.energy.ca.gov Notice of Availability Developing Renewable Generation on State Property Installing Renewable Energy on State Buildings

  8. STATE OF CALIFORNIA --NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY COMMISSION

    E-Print Network [OSTI]

    STATE OF CALIFORNIA -- NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor CALIFORNIA ENERGY as eligible renewable energy resources for the RPS and describes how the Energy Commission tracks and verifies COMMISSION 1516 Ninth Street Sacramento, California 95814 Main website: www.energy.ca.gov Notice

  9. Minimax design of vibration absorbers for linear damped systems Brandon Brown, Tarunraj Singh

    E-Print Network [OSTI]

    Singh, Tarunraj

    Minimax design of vibration absorbers for linear damped systems Brandon Brown, Tarunraj Singh à Department of Mechanical and Aerospace Engineering, State University of New York at Buffalo, Buffalo, NY addresses the issue of design of a passive vibration absorber in the presence of uncertainties

  10. Compost Tips for the Home Gardener1 Sydney Park Brown2

    E-Print Network [OSTI]

    Jawitz, James W.

    ENH1065 Compost Tips for the Home Gardener1 Sydney Park Brown2 1. This document is ENH1065, one. Nick T. Place, dean for UF/IFAS Extension. What Is Compost? Compost is a dark, crumbly material created. Compost is not completely decomposed (like humus); it will contain small pieces of debris that can

  11. Hot Dry Rock Geothermal Energy Development in the USA David Duchane and Donald Brown

    E-Print Network [OSTI]

    1 Hot Dry Rock Geothermal Energy Development in the USA by David Duchane and Donald Brown Los of the world's store of geothermal energy. The real potential for growth in the use of geothermal energy lies-engineered geothermal reservoir in hot, crystalline rock by the application of hydraulic fracturing techniques

  12. STATE OF CALIFORNIA NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor April 25, 2011

    E-Print Network [OSTI]

    , 2011 PON-10-604 GRANT SOLICITATION APPLICATION PACKAGE Buy Down Incentives for Natural Gas and PropaneSTATE OF CALIFORNIA ­ NATURAL RESOURCES AGENCY EDMUND G. BROWN JR., Governor Addendum 3 April 25 Vehicles The purpose of this addendum is to clarify the minimum requirements needed for the original

  13. METHANE AND ETHANE ON THE BRIGHT KUIPER BELT OBJECT 2005 FY9 M. E. Brown,1

    E-Print Network [OSTI]

    Brown, Michael E.

    METHANE AND ETHANE ON THE BRIGHT KUIPER BELT OBJECT 2005 FY9 M. E. Brown,1 K. M. Barkume,1 G. A indicates the clear presence of ethane, an expected product of UV photolysis of methane. No evidence for N2 of 2005 FY9 that leads to large methane grains, abundant sites for ethane formation through UV photolysis

  14. The First Hundred Brown Dwarfs Discovered by the Wide-field Infrared Survey Explorer (WISE)

    E-Print Network [OSTI]

    Bochanski, John J.

    We present ground-based spectroscopic verification of 6 Y dwarfs (see also Cushing et al.), 89 T dwarfs, 8 L dwarfs, and 1 M dwarf identified by the Wide-field Infrared Survey Explorer (WISE). Eighty of these are cold brown ...

  15. Computer simulation of three-arm star polymers Scott Brown, Grzegorz Szamel*

    E-Print Network [OSTI]

    Szamel, Grzegorz

    14 Computer simulation of three-arm star polymers Scott Brown, Grzegorz Szamel* Department) . In this paper we describe a computer simulation study of three-arm star polymers in the melt. It is believed) have argued that large (spatial) scale diffusive motions are enabled by an "arm-retraction" mechanism

  16. The Static Di#eHellman Problem Daniel R. L. Brown Robert P. Gallant

    E-Print Network [OSTI]

    International Association for Cryptologic Research (IACR)

    The Static Di#e­Hellman Problem Daniel R. L. Brown Robert P. Gallant dbrown@certicom.com rgallant a function that solves a special case of the Di#e­Hellman prob­ lem, called the static Di#e­Hellman problem the static Di#e­Hellman problem for Q (SDHPQ ). Thus the SDHPQ function solves certain instances of the Di

  17. Spectra of Tukey types of ultrafilters on Boolean algebras Jennifer A. Brown and Natasha Dobrinen

    E-Print Network [OSTI]

    Dobrinen, Natasha

    The structure of Tukey types of ultrafilters on is the subject of much recent and ongoing research. This line in this research stems from the connection via Stone duality between Tukey types of ultrafilters on and cofinalSpectra of Tukey types of ultrafilters on Boolean algebras Jennifer A. Brown and Natasha Dobrinen

  18. Electrical Engineering Graduate Handbook Charles L. Brown Department of Electrical & Computer Engineering

    E-Print Network [OSTI]

    Zhigilei, Leonid V.

    1 Electrical Engineering Graduate Handbook 2014-2015 Charles L. Brown Department of Electrical outlines the policies and procedures of the graduate program of the Department of Electrical and Computer from the Chairman Electrical engineers continue to provide technological leadership for developments

  19. Abbott, Albert G., Professor, Genetics and Biochemistry. BS, University of Connecticut, 1976; PhD, Brown

    E-Print Network [OSTI]

    Stuart, Steven J.

    of Connecticut, 1976; PhD, Brown University, 1980 Abbott, Sherrie Wilder, Lecturer, School of Nursing. BSN, Emory Abramovitch, Rudolph A., Professor, Chemistry. BS, Alexandria University (Egypt), 1950; PhD, 1953, DSc, 1964 (England), 1962; MS, Clemson University, 1963; PhD, Nottingham Trent University (England), 1967 Adams

  20. Short communication Control of brown rot of stone fruits by brief heated water immersion treatments

    E-Print Network [OSTI]

    Crisosto, Carlos H.

    Short communication Control of brown rot of stone fruits by brief heated water immersion treatments, this treatment reduced decay incidence from 100 to less than 5% on fruit stored at 20 C and from 73 to 28% on cold-stored fruit. Therefore, brief immersion in heated water can be an effective approach to manage

  1. Capping the Brown Energy Consumption of Internet Services at Low Cost

    E-Print Network [OSTI]

    Capping the Brown Energy Consumption of Internet Services at Low Cost Kien T. Le Ricardo Bianchini Thu D. Nguyen Rutgers University Ozlem Bilgir Margaret Martonosi Princeton University #12;Energy Electricity sources Coal Natural Gas Nuclear Renewables Others 100 105 110 115 120 Nigeria Data Centers Czech

  2. Estimated Impacts on Ex-Vessel Brown Shrimp Prices and Value as a Result of the

    E-Print Network [OSTI]

    Estimated Impacts on Ex-Vessel Brown Shrimp Prices and Value as a Result of the Texas Closure Regulation JOHN R. POFFENBERGER Introduction Changes in commodity prices may result from any regulatory shrimp landings in Texas and therefore could be expected to affect ex-vessel or dockside prices

  3. Towards Availability Benchmarks: A Case Study of Software RAID Systems Aaron Brown and David A. Patterson

    E-Print Network [OSTI]

    California at Berkeley, University of

    Towards Availability Benchmarks: A Case Study of Software RAID Systems Aaron Brown and David A neglected the areas of availability, maintainability, and evolutionary growth, areas that have recently introduce a general methodology for bench- marking the availability of computer systems. Our methodology

  4. Accepting Failure: Availability through Repair-centric System Design Aaron Brown

    E-Print Network [OSTI]

    California at Berkeley, University of

    1 Accepting Failure: Availability through Repair-centric System Design Aaron Brown Qualifying Exam Proposal 3 April 2001 Abstract Motivated by the lack of rapid improvement in the availability of Internet server systems, we introduce a new philosophy for designing highly-available systems that better reflects

  5. Palatability of beef from young bulls 

    E-Print Network [OSTI]

    Riley, Ray Renfrow

    1981-01-01

    Palatability of Beef from Young Bulls. (December 1981) Ray Renfrow Riley, B. S. , Texas ASM University Co-Chairmen of Advisory Committee: Dr. J. W, Savell Dr. G. C. Smrth Electrical stimulation (ES), subcutaneous fat thickness and carcass masculinity... such matched steers were not different (P&. 05) - n overall palatability than steaks from ES young bulls. Steaks from U. S. Choice steers and from U. S. Good steers or bulls that had at least. 7. 62 mm fat thickness did not differ (P&. 05) in 39 of 42...

  6. Young Persons Guide to BCPL Programming

    E-Print Network [OSTI]

    Mullins, Robert

    Young Persons Guide to BCPL Programming on the Raspberry Pi Part 1 by Martin Richards mr:07:33 BST 2015 Abstract The Raspberry Pi is a credit card sized computer with versions costing between £20 to learn to write, compile and run BCPL programs on the Raspberry Pi in as little as one or two days, even

  7. SPRING/SUMMER 2012 ANDREW YOUNG SCHOOL

    E-Print Network [OSTI]

    Frantz, Kyle J.

    for supporting our students. Another is the new university-wide Honors College. Assistant Dean Cynthia Searcy has three times a year for alumni, friends, faculty and staff of the AndrewYoung School of Policy Studies Cynthia Searcy Assistant Dean for Academic Programs Avani Raval Promotion, Events, Facilities & Safety

  8. Growing Young Trees in the Greening Era

    E-Print Network [OSTI]

    Ma, Lena

    winter · If possible, consider electric pumps and computer controls to be able to irrigate in small doses · Irrigation · Fertilization · Weed Control · Pest Management · Disease Management #12;The Young Tree Paradox and economic return = FLUSH!!! #12;Irrigation · Critical ­ restriction of canopy development is the first

  9. , UNIVERSITY Brigham Young University Geology Studies

    E-Print Network [OSTI]

    Seamons, Kent E.

    , UNIVERSITY #12;Brigham Young University Geology Studies Volume 1 5 - 1968 Part 2 Studies for Students No. 1 Guide to the Geology of the Wasatch Mountain Front, Between Provo Canyon and Y Mountain, Northeast of Provo, Utah by J. Keith Rigby and Lehi F. Hintze #12;A publication of the Department of Geology

  10. An equivalent form of Young's inequality with upper bound

    E-Print Network [OSTI]

    E. Minguzzi

    2008-08-05

    Young's integral inequality is complemented with an upper bound to the remainder. The new inequality turns out to be equivalent to Young's inequality, and the cases in which the equality holds become particularly transparent in the new formulation.

  11. Registration for the 2015 Conference for Young Women in STEM...

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

    Registration for the 2015 Conference for Young Women in STEM is OPEN October 15, 2014 The 2015 Young Women's Conference in STEM will be held on Thursday, March 19, 2015 at...

  12. A T8.5 BROWN DWARF MEMBER OF THE {xi} URSAE MAJORIS SYSTEM

    SciTech Connect (OSTI)

    Wright, Edward L.; Mace, Gregory; McLean, Ian S. [UCLA Astronomy, P.O. Box 951547, Los Angeles, CA 90095-1547 (United States); Skrutskie, M. F.; Nelson, M. J.; Borish, H. J. [Department of Astronomy, University of Virginia, Charlottesville, VA 22904 (United States); Kirkpatrick, J. Davy; Gelino, Christopher R.; Griffith, Roger L.; Jarrett, Tom [Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States); Marsh, Kenneth A. [School of Physics and Astronomy, Cardiff University, Cardiff CF243AA (United Kingdom); Mainzer, Amanda K.; Eisenhardt, Peter R. [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109-8001 (United States); Tobin, John J. [National Radio Astronomy Observatory, Charlottesville, VA 22903 (United States); Cushing, Michael C., E-mail: wright@astro.ucla.edu [Department of Physics and Astronomy, MS 111, University of Toledo, 2801 W. Bancroft St., Toledo, OH 43606-3328 (United States)

    2013-03-15

    The Wide-field Infrared Survey Explorer has revealed a T8.5 brown dwarf (WISE J111838.70+312537.9) that exhibits common proper motion with a solar-neighborhood (8 pc) quadruple star system-{xi} Ursae Majoris. The angular separation is 8.'5, and the projected physical separation is Almost-Equal-To 4000 AU. The sub-solar metallicity and low chromospheric activity of {xi} UMa A argue that the system has an age of at least 2 Gyr. The infrared luminosity and color of the brown dwarf suggests the mass of this companion ranges between 14 and 38 M{sub J} for system ages of 2 and 8 Gyr, respectively.

  13. A T8.5 Brown Dwarf Member of the Xi Ursae Majoris System

    E-Print Network [OSTI]

    Wright, Edward L; Kirkpatrick, J Davy; Gelino, Christopher R; Griffith, Roger L; Marsh, Kenneth A; Jarrett, Tom; Nelson, M J; Borish, H J; Mace, Gregory; Mainzer, Amanda K; Eisenhardt, Peter R; McLean, Ian S; Tobin, John J; Cushing, Michael C

    2012-01-01

    The Wide-field Infrared Survey Explorer has revealed a T8.5 brown dwarf (WISE J111838.70+312537.9) that exhibits common proper motion with a solar-neighborhood (8 pc) quadruple star system - Xi Ursae Majoris. The angular separation is 8.5 arc-min, and the projected physical separation is about 4000 AU. The sub-solar metallicity and low chromospheric activity of Xi UMa A argue that the system has an age of at least 2 Gyr. The infrared luminosity and color of the brown dwarf suggests the mass of this companion ranges between 28 and 58 Jupiter masses for system ages of 2 and 8 Gyr respectively.

  14. An Imaging Survey for Extrasolar Planets around 45 Close, Young Stars with SDI at the VLT and MMT

    E-Print Network [OSTI]

    Beth A. Biller; Laird M. Close; Elena Masciadri; Eric Nielsen; Rainer Lenzen; Wolfgang Brandner; Donald McCarthy; Markus Hartung; Stephan Kellner; Eric Mamajek; Thomas Henning; Douglas Miller; Matthew Kenworthy; Craig Kulesa

    2007-05-01

    We present the results of a survey of 45 young (planets. As part of the survey, we observed 54 objects total, of which 45 were close, young stars, 2 were somewhat more distant (planets, and 4 were older, very nearby (cool brown dwarfs and gas giant planets. In our VLT data, we achieved H band contrasts > 10 mag (5 sigma) at a separation of 0.5" from the primary star on 45% of our targets and H band contrasts of > 9 mag at a separation of 0.5'' on 80% of our targets. With this degree of attenuation, we should be able to image (5sigma detection) a 5 M_{Jup} planet 15 AU from a 70 Myr K1 star at 15 pc or a 5 M_{Jup} planet at 2 AU from a 12 Myr M star at 10 pc. We believe that our SDI images are the highest contrast astronomical images ever made from ground or space for methane rich companions planets at semi-major axes of 20-40 AU. Thus, our completeness levels are sufficient to significantly test theoretical planet distributions. From our survey null result, we can rule out (at the 98% confidence/2.0sigma level) a model planet population using a planet distribution where N(a) $\\propto$ constant out to a distance of 45 AU (further model assumptions discussed within).

  15. Jefferson Lab Activities Group Invites Young and Not-So-Young...

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

    Holiday Events Holiday Party on Dec. 12 for Jefferson Lab Children and the Young at Heart The JAG Holiday Party is scheduled for Saturday, Dec. 12, 10 a.m.-1 p.m. in the CEBAF...

  16. Methane, carbon monoxide, and ammonia in brown dwarfs and self-luminous giant planets

    SciTech Connect (OSTI)

    Zahnle, Kevin J.; Marley, Mark S. E-mail: Mark.S.Marley@NASA.gov

    2014-12-10

    We address disequilibrium abundances of some simple molecules in the atmospheres of solar composition brown dwarfs and self-luminous extrasolar giant planets using a kinetics-based one-dimensional atmospheric chemistry model. Our approach is to use the full kinetics model to survey the parameter space with effective temperatures between 500 K and 1100 K. In all of these worlds, equilibrium chemistry favors CH{sub 4} over CO in the parts of the atmosphere that can be seen from Earth, but in most disequilibrium favors CO. The small surface gravity of a planet strongly discriminates against CH{sub 4} when compared to an otherwise comparable brown dwarf. If vertical mixing is like Jupiter's, the transition from methane to CO occurs at 500 K in a planet. Sluggish vertical mixing can raise this to 600 K, but clouds or more vigorous vertical mixing could lower this to 400 K. The comparable thresholds in brown dwarfs are 1100 ± 100 K. Ammonia is also sensitive to gravity, but, unlike CH{sub 4}/CO, the NH{sub 3}/N{sub 2} ratio is insensitive to mixing, which makes NH{sub 3} a potential proxy for gravity. HCN may become interesting in high-gravity brown dwarfs with very strong vertical mixing. Detailed analysis of the CO-CH{sub 4} reaction network reveals that the bottleneck to CO hydrogenation goes through methanol, in partial agreement with previous work. Simple, easy to use quenching relations are derived by fitting to the complete chemistry of the full ensemble of models. These relations are valid for determining CO, CH{sub 4}, NH{sub 3}, HCN, and CO{sub 2} abundances in the range of self-luminous worlds we have studied, but may not apply if atmospheres are strongly heated at high altitudes by processes not considered here (e.g., wave breaking).

  17. A Review of "Sir Thomas Browne: The World Proposed" edited by Reid Barbour and Claire Preston 

    E-Print Network [OSTI]

    Black, Joseph

    2011-01-01

    of the most important topics for readers of Milton. Reid Barbour and Claire Preston, eds. Sir Thomas Browne: The World Proposed. Oxford: Oxford University Press, 2008. xii + 368 pp. + 3 illus. $120.00. Review by joseph l. black, university of massachusetts..., not only Religio Medici (Brooke Conti), Pseudodoxia Epidemica (William N. West and Kevin Killeen), Urne-Buriall (Achsah Guibbory), and Garden of Cyrus (Kathryn Murphy), but also Letter to a Friend (Claire Preston) and Repertorium (Jonathan F.S. Post...

  18. Liquid metallic hydrogen and the structure of brown dwarfs and giant planets

    E-Print Network [OSTI]

    W. B. Hubbard; T. Guillot; J. I. Lunine; A. Burrows; D. Saumon; M. S. Marley; R. S. Freedman

    1997-03-02

    Electron-degenerate, pressure-ionized hydrogen (usually referred to as metallic hydrogen) is the principal constituent of brown dwarfs, the long-sought objects which lie in the mass range between the lowest-mass stars (about eighty times the mass of Jupiter) and the giant planets. The thermodynamics and transport properties of metallic hydrogen are important for understanding the properties of these objects, which, unlike stars, continually and slowly cool from initial nondegenerate (gaseous) states. Within the last year, a brown dwarf (Gliese 229 B) has been detected and its spectrum observed and analyzed, and several examples of extrasolar giant planets have been discovered. The brown dwarf appears to have a mass of about forty to fifty Jupiter masses and is now too cool to be fusing hydrogen or deuterium, although we predict that it will have consumed all of its primordial deuterium. This paper reviews the current understanding of the interrelationship between its interior properties and its observed spectrum, and also discusses the current status of research on the structure of giant planets, both in our solar system and elsewhere.

  19. Analytical and characterization studies of organic and inorganic species in brown coal

    SciTech Connect (OSTI)

    G. Domazetis; M. Raoarun; B.D. James; J. Liesegang; P.; J. Pigram; N. Brack [La Trobe University, Vic. (Australia). Department of Chemistry

    2006-08-15

    Detailed studies have been carried out on the distribution of organic functional groups and inorganic species in as-received (ar) and acid-washed (aw) brown coals using elemental analysis, energy dispersive X-ray analysis (SEM-EDX), X-ray photoelectron spectroscopy (XPS), and Time-of-flight-secondary ion mass spectrometry (TOF-SIMS). Surface concentrations of the various carbon groups, organic oxygen, and inorganic hydroxide were obtained using XPS, but oxygen from clay and quartz, if present, interfered with organic oxygen determinations for the coals. A comparison of ar and aw coals using XPS and SEM-EDX is provided in terms of inorganic and organic sulfur groups. Chloride in these coals is present mainly as acid extractable forms, but small amounts of chloride in the organic matrix were indicated by the elemental analysis of ultra low-ash coals. TOF-SIMS fragments from brown coals were indicative of polymers consisting mainly of single aromatic groups linked by hydrocarbons with carboxyl and phenol functional groups. Sulfur fragments were from inorganic sulfur, thiols, organo-sulfates, and S-N-organic species. Numerous fragments containing organically bound chloride were observed. Fragments of the inorganic species Na, Mg, Al, Si, K, Ca, Ti, Cr, Fe, Mn, Ni, Cu, and Ga were also observed. Environmentally undesirable species, particularly from organo-sulfur and organo-chloride groups in brown coal, are likely to emerge from processes that heat coal-water mixture. 54 refs., 3 figs., 10 tabs.

  20. BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 26, Part 4

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 26, Part 4 The Fossil Vertebrates of Utah Salt Lake Gty, Utah 84102 W .E. Miller Deparlment~of Geology and Zoology Bngham Young Unrwerrrly Provo of Geology Brigham Young University Provo, Utah 84602 Editors W. Kenneth Hamblln Cynthia M. Gardner Issue

  1. Quality characteristics of young bovine carcasses 

    E-Print Network [OSTI]

    Bellinger, John Wayne

    1978-01-01

    ) May 1978 442834 1 1. 1 ABSTRACT Quality Characteristics of Young Bovine Carcasses. (May 1978) John Wayne Bellinger B. S. , Texas A&M University Co-Chairmen of Advisory Committee: Dr. G C. Smith Dr Z. L. Carpenter A total of 305 carcasses... longissimus muscle steaks. ACKNOWLEDGMENTS The author greatly appreciates the encouragement and inspiration given by Drs. G. C. Smith and Z. L. Carpenter throughout his coursework and research. Their guidance and suggestions will always be remembered...

  2. NEW YOUNG STAR CANDIDATES IN CG4 AND Sa101

    SciTech Connect (OSTI)

    Rebull, L. M.; Laine, S.; Laher, R.; Legassie, M.; Hoette, V.; Kim, J. S.; Foster, M.; Mallory, C. R.; McCarron, K.; Sherry, W. H.

    2011-07-15

    The CG4 and Sa101 regions together cover a region of {approx}0.5 deg{sup 2} in the vicinity of a 'cometary globule' that is part of the Gum Nebula. There are seven previously identified young stars in this region; we have searched for new young stars using mid- and far-infrared data (3.6-70 {mu}m) from the Spitzer Space Telescope, combined with ground-based optical data and near-infrared data from the Two Micron All Sky Survey. We find infrared excesses in all six of the previously identified young stars in our maps and identify 16 more candidate young stars based on apparent infrared excesses. Most (73%) of the new young stars are Class II objects. There is a tighter grouping of young stars and young star candidates in the Sa101 region, in contrast to the CG4 region, where there are fewer young stars and young star candidates, and they are more dispersed. Few likely young objects are found in the 'fingers' of the dust being disturbed by the ionization front from the heart of the Gum Nebula.

  3. Double Conscious Brother in the Veil Toward an Intellectual Biography of Sterling A. Brown

    E-Print Network [OSTI]

    Tidwell, John E.

    1998-09-01

    green Better'n most. "I kin talk out dis worl' As you folks all know, An' I'm good wid de women, Dey'll tell you so . . . V "An' I says to all de Bishops, What is hearin' my song— Ef de cap fits you, brother, Put it on." —Sterling Allen Brown... to the [Aran Islands] as a poet, seeking the real quality of the folk, not as a social scientist amassing statistics. His poetic insight availed, he has left us unforgettable pictures of the dignity of these inarticulate people, their courage in the teeth...

  4. Trenton strata in western Illinois Basin, Brown and Schuyler Counties, Illinois

    SciTech Connect (OSTI)

    Pochel, R.M.

    1984-12-01

    Trenton strata in the western Illinois basin are very good prospects for oil exploration. Much drilling has been done in the area but, as yet, no producing wells have been completed. Oil stains and some tars have been found in some samples from most wells. The Trenton in the area of Brown and Schuyler Counties is a fine-grained limestone that underlies the Maquoketa Shale at an average depth of 800 ft (244 m). Because of its position near the edge of the Illinois basin, the stratigraphy varies considerably and inconsistencies are present in most samples viewed.

  5. Genetic analysis of hybridization and introgression between wild mongoose and brown lemurs

    E-Print Network [OSTI]

    Pastorini, Jennifer; Zaramody, Alphonse; Curtis, Deborah J.; Nievergelt, Caroline M.; Mundy, Nicholas I.

    2009-02-05

    :32 http://www.biomedcentral.com/1471-2148/9/32 been found across the animal kingdom, including insects [7], fish [8], amphibians [9], birds [10,11], carnivores [12], and monkeys [13-15]. Among the Malagasy lemurs, a few cases of hybridization between... , and nectar [31]. The most important potential competitor for mongoose lemurs at Anjamena is E. f. rufus, as it not only shares food resources (fruit and leaves) with E. mongoz but also exhib- its a similar activity pattern [26]. Brown lemurs at Anja- mena...

  6. Harold Brown, 1992 | U.S. DOE Office of Science (SC)

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration would likeUniverse (Journalvivo Low-Dose Lowï‚—34OctoberK West60Harnessing theHarold Brown, 1992

  7. SEARCHING FOR YOUNG M DWARFS WITH GALEX

    SciTech Connect (OSTI)

    Shkolnik, Evgenya L.; Weinberger, Alycia J.; Liu, Michael C.; Dupuy, Trent; Reid, I. Neill E-mail: alycia@dtm.ciw.edu E-mail: tdupuy@ifa.hawaii.edu

    2011-01-20

    The census of young moving groups in the solar neighborhood is significantly incomplete in the low-mass regime. We have developed a new selection process to find these missing members based on the Galaxy Evolution Explorer (GALEX) All-Sky Imaging Survey (AIS). For stars with spectral types {approx}>K5 (R - J {approx}> 1.5) and younger than {approx}300 Myr, we show that near-UV (NUV) and far-UV (FUV) emission is greatly enhanced above the quiescent photosphere, analogous to the enhanced X-ray emission of young low-mass stars seen by ROSAT but detectable to much larger distances with GALEX. By combining GALEX data with optical (HST Guide Star Catalog) and near-IR (2MASS) photometry, we identified an initial sample of 34 young M dwarf candidates in a 1000 deg{sup 2} region around the {approx}10 Myr TW Hydra Association (TWA). Low-resolution spectroscopy of 30 of these found 16 which had H{alpha} in emission, which were then followed up at high resolution to search for spectroscopic evidence of youth and to measure their radial velocities. Four objects have low surface gravities, photometric distances and space motions consistent with TWA, but the non-detection of Li indicates that they may be too old to belong to this moving group. One object (M3.5, 93 {+-} 19 pc) appears to be the first known accreting low-mass member of the {approx}15 Myr Lower Centaurus Crux OB association. Two objects exhibit all the characteristics of the known TWA members, and thus we designate them as TWA 31 (M4.2, 110 {+-} 11 pc) and TWA 32 (M6.3, 53 {+-} 5 pc). TWA 31 shows extremely broad (447 km s{sup -1}) H{alpha} emission, making it the sixth member of TWA found to have ongoing accretion. TWA 32 is resolved into a 0.''6 binary in Keck laser guide star adaptive optics imaging. Our search should be sensitive down to spectral types of at least M4-M5 in TWA and thus the small numbers of new member is puzzling. This might indicate TWA has an atypical mass function or that the presence of lithium absorption may be too restrictive a criteria for selecting young low-mass stars.

  8. YoungHo Shin | Argonne National Laboratory

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power AdministrationRobust,Field-effectWorkingLos Alamos verifies largest single|Yejun FengResultscurrent |YoungHo

  9. The Anderson/Sargent Dallas Show House

    SciTech Connect (OSTI)

    2008-07-08

    This case study describes development of a net zero energy home featuring high efficiency air and duct sealing, solar thermal and photovoltaic systems, and water conservation.

  10. THE UNIVERSITY OF TEXAS AT DALLAS

    E-Print Network [OSTI]

    O'Toole, Alice J.

    engineering and electronics. With a focus on nanoscale materials and phenomena, the research is at the cutting manufacturing, nanosize coatings and materials for biomedical applications. High level funding (~$12M/y) from (chemical companies, tool makers and microelectronics companies) and foreign governments, often with state

  11. Dallas, Texas: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX ECoopButtePower VenturesInformation9) WindGrid Project) | OpenCoop IncTexas:

  12. Dallas, Texas: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX E LIST OFAMERICA'SHeavy Electricals Ltd BHELEurope LimitedDakshidin Ltd Jump to:Jump to:

  13. Brown - leaves

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 OutreachProductswsicloudwsiclouddenDVA N C E D B L OBransen Plasma Asher An O2Brookhaven Site Office EA /LASE

  14. Brown - leaves

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 OutreachProductswsicloudwsiclouddenDVA N C E D B L OBransen Plasma Asher An O2Brookhaven Site Office EA

  15. Young Physicist from Syracuse University Receives Jefferson Lab...

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

    Physicist from Syracuse University Receives Jefferson Lab's 2014 Thesis Prize Beminiwattha Rakitha Beminiwattha NEWPORT NEWS, VA, June 6, 2014 - A young researcher, who worked on...

  16. Three Young Scientists Earn DOE Graduate Research Grants at Jefferson...

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

    accomplishments have earned three young scientists funds to conduct part of their thesis research at the U.S. Department of Energy's Thomas Jefferson National Accelerator...

  17. Young Womens Conference attracts more attendees in 2014! | Princeton...

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

    Gallery: The 2014 Young Women's Conference is Science, Engineering, Technology, and Mathematics attracted students from all over New Jersey With almost 400 students, 50,...

  18. Pluto's Seasons: New Predictions for New Horizons L. A. Young

    E-Print Network [OSTI]

    Young, Leslie A.

    (2012) and Young (in prep). Energy balance for the world that New Horizons will encounter in 2015, and our ability to relate this snapshot to preceding

  19. Structure and Stratigraphy Beneath a Young Phreatic Vent: South...

    Open Energy Info (EERE)

    Structure and Stratigraphy Beneath a Young Phreatic Vent: South Inyo Crater, Long Valley Caldera, California Jump to: navigation, search OpenEI Reference LibraryAdd to library...

  20. DISCOVERY OF A ?250 K BROWN DWARF AT 2 pc FROM THE SUN

    SciTech Connect (OSTI)

    Luhman, K. L.

    2014-05-10

    Through a previous analysis of multi-epoch astrometry from the Wide-field Infrared Survey Explorer (WISE), I identified WISE J085510.83–071442.5 as a new high proper motion object. By combining astrometry from WISE and the Spitzer Space Telescope, I have measured a proper motion of 8.1 ± 0.1'' yr{sup –1} and a parallax of 0.454 ± 0.045'' (2.20{sub ?0.20}{sup +0.24} pc) for WISE J085510.83–071442.5, giving it the third highest proper motion and the fourth largest parallax of any known star or brown dwarf. It is also the coldest known brown dwarf based on its absolute magnitude at 4.5 ?m and its color in [3.6]-[4.5]. By comparing M {sub 4.5} with the values predicted by theoretical evolutionary models, I estimate an effective temperature of 225-260 K and a mass of 3-10 M {sub Jup} for the age range of 1-10 Gyr that encompasses most nearby stars.

  1. Assessment and use of Loy Yang brown coal for power generation

    SciTech Connect (OSTI)

    Ottrey, A.; Woskoboenko, F. [HRL Technology Pty Ltd., Mulgrave, Victoria (Australia); Draper, I.; Fitzclarence, N. [Loy Yang Power Ltd., Traralgon, Victoria (Australia)

    1996-12-31

    The Loy Yang brown coal resource in the Latrobe Valley of Victoria has been extensively characterized in respect of: the extent, distribution and structure of the resource; the variations in properties throughout the resource; and evaluation of the behavior of the coal during processing. The resource characterization program involved an extensive borehole drilling program, backed by geological modelling and comprehensive material characterization (chemical, physical and petrological). Evaluation of the behavior of the coal has involved theoretical modelling, laboratory-scale investigations, pilot-scale combustion tests and observations on full-scale boilers. The Loy Yang open cut mine currently annually supplies 26 million tonne (Mt) of brown coal to: the 4 x 4500 MW units operated by Loy Yang Power Ltd.; the 2 x 500 MW units operated by Edison Mission Ltd.; and a steam-fluidized bed dryer operated by Dry Coal Australia Pty Ltd. (a joint venture between Lurgi and Australian Char Pty Ltd.). This paper highlights significant features of Loy Yang Power`s operations in the mine and the power station, with particular emphasis on ash fouling and slagging behavior.

  2. Antagonist effect between violaxanthin and de-epoxidated pigments in nonphotochemical quenching induction in the qE deficient brown alga

    E-Print Network [OSTI]

    Govindjee

    induction in the qE deficient brown alga Macrocystis pyrifera Héctor Ocampo-Alvarez a , Ernesto GarcíaZ) De-epoxidation rate control Brown alga Macrocystis pyrifera Nonphotochemical quenching (NPQ quenching (qE), is not present in this alga. In contrast to higher plants, NPQ in this organism is much more

  3. Nonnative Lizards Nile Monitor 4 to 6 ft. Brown/yellow body bands; forked black/blue tongue; long sharp claws

    E-Print Network [OSTI]

    Mazzotti, Frank

    beneath the eye Reticulated Python 14 to 18 ft. Distinct reddish eyes; tan body with dark brown net dull with age. Males have larger spikes along back. Black and White Tegu 2 to 3 ft. Dark bands. Yellowish-tan to dark brown; red dewlap with yellow border Ianaré Sévi NATIVE Look-a-Likes David Barkasy

  4. Observation of Transverse Bose-Einstein Condensation via Hanbury BrownTwiss Correlations Wu RuGway, A. G. Manning, S. S. Hodgman, R. G. Dall, and A. G. Truscott

    E-Print Network [OSTI]

    Kheruntsyan, Karen

    Observation of Transverse Bose-Einstein Condensation via Hanbury Brown­Twiss Correlations Wu Ru a three-dimensional thermal gas to a gas undergoing transverse condensation by probing Hanbury Brown­Twiss

  5. Brigham Young University Geology Studies Volume 28, Part 2

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;Brigham Young University Geology Studies Volume 28, Part 2 Lower and Middle Ordovician at Section G, Ibex, Utah. #12;A publication of the Department of Geology Brigham Young University Provo, Utah o ~ l z gUfziversity Geology Studies is published by the Department of Geology. This publication

  6. Lifestyle, identity and young people's experiences of mountain biking

    E-Print Network [OSTI]

    Lifestyle, identity and young people's experiences of mountain biking It has been widely recognised emphasis on young people as a key target group. Mountain biking, as a popular youth sport that often occurs. The research employed ethnographic techniques to capture youth experiences and understandings of mountain

  7. The New York State Summer Young Writers Institute

    E-Print Network [OSTI]

    Alexandrova, Ivana

    #12;The New York State Summer Young Writers Institute W hat you hold in your hands are the poems and stories ­ true and imagined ­ that the stu- dents of the New York State Summer Young Writers Institute take advantage of the New York State Summer Writers Institute, directed by Robert Boyers, which

  8. The New York State Summer Young Writers Institute

    E-Print Network [OSTI]

    Alexandrova, Ivana

    #12;The New York State Summer Young Writers Institute The New York State Summer Young Writers Institute (NYSSYWI), sponsored jointly by the New York State Writers Institute at the University at Albany attend high schools in New York State. Now in its 9th year, NYSSYWI is held the first week in July

  9. GRADUATE STUDIES IN CHEMICAL ENGINEERING Brigham Young University

    E-Print Network [OSTI]

    Martinez, Tony R.

    GRADUATE STUDIES IN CHEMICAL ENGINEERING Brigham Young University Graduate Student Handbook The Department of Chemical Engineering 350 Clyde Building Brigham Young University Provo, Utah 84602 Phone: (801;2 To the New Graduate Student, On behalf of the faculty and staff of the Department of Chemical Engineering

  10. Spoken word recognition and lexical representation in very young children

    E-Print Network [OSTI]

    Makous, Walter

    Spoken word recognition and lexical representation in very young children Daniel Swingley*, Richard March 2000 Abstract Although children's knowledge of the sound patterns of words has been a focus of debate for many years, little is known about the lexical representations very young children use in word

  11. The New York State Summer Young Writers Institute

    E-Print Network [OSTI]

    Alexandrova, Ivana

    #12;The New York State Summer Young Writers Institute What you hold in your hands are the poems and stories ­ true and imagined ­ that the students of the New York State Summer Young Writers Institute that our students could take advantage of the New York State Summer Writers Institute, directed by Robert

  12. Brigham Young University Geology Studies Volume 26, Part 3

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;P I - #12;Brigham Young University Geology Studies Volume 26, Part 3 Conodont Biostratigraphy-meeting field trip held in conjunction with the Rocky Mountain section, Geological Society of America of the Department of Geology Brigham Young University Provo, Utah 84602 Editors W. Kenneth Hamblin Cynthia M

  13. Brigham Young University Geology Studies Volume 25, Part 3

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;Brigham Young University Geology Studies Volume 25, Part 3 CONTENTS Remains of Ornithopod ...........................................................................................................................................................ames M. Stolle Publications and Maps of the Geology Department Index to volumes 21-25 of Brigham Young University Geology Studies ........................................Carol T . Smith and Nathan M. Smith Cwec

  14. Brigham Young University Geology Studies Volume 26, Part 2

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;Brigham Young University Geology Studies Volume 26, Part 2 CONTENTS A New Large Theropod................................................................................................................................................................ Danny J. Wyatt Publications and Maps of the Geology Department Cover: Cretaceouscoals near Castle Gate, Utab. #12;A publication of the Department of Geology Brigham Young University Provo, Utah 84602 Editors

  15. Brigham Young University Geology Studies Volume 26, Part I

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;Brigham Young University Geology Studies Volume 26, Part I Papers presented at the 31st annual meeting, Rocky Mountain Section, Geological Society of America, April 28-29, 1978, at Brig- ham Young ............................................................................................................................Publications and Maps of the Geology Department 91 Cover The Great Basrn seen from a htgh

  16. DISTINCT PATTERNS OF NITRATE REDUCTASE ACTIVITY IN BROWN ALGAE: LIGHT AND AMMONIUM SENSITIVITY IN LAMINARIA DIGITATA IS ABSENT IN

    E-Print Network [OSTI]

    Berges, John A.

    DISTINCT PATTERNS OF NITRATE REDUCTASE ACTIVITY IN BROWN ALGAE: LIGHT AND AMMONIUM SENSITIVITY and lowest in summer. This is the first report of NR activity in any alga that is not strongly regulated the regulation of NR by light that has been observed in other algae and higher plants. Key index words: ammonium

  17. Arsenic Modulates Cell Proliferation Pathways in MCF-7 Breast Cancer Cells Krystle Brown, Somaly Neang, Dorrelyn Patacsil, and Deepak Kumar

    E-Print Network [OSTI]

    District of Columbia, University of the

    Arsenic Modulates Cell Proliferation Pathways in MCF-7 Breast Cancer Cells Krystle Brown, Somaly Viability Assay: The cell viability and proliferation of MCF-7 breast cancer cell lines were determined as indicated. The cells were fixed in methanol and stained with 4'-6-Diamidino-2-phenylindole (DAPI) nuclear

  18. A Field-Wise Wind Retrieval Algorithm for Satellite Scatterometers Charles G. Brown and David G . Long

    E-Print Network [OSTI]

    Long, David G.

    A Field-Wise Wind Retrieval Algorithm for Satellite Scatterometers Charles G. Brown and David G-378-6586 browncg@salt.ee.byii.edu Abstract-Traditional satellite scatterometer wind retrieval algorithms consist of point-wise wind estimation and point- wise ambiguity removal. Point-wise estimation yields mul- tiple

  19. Facies architecture of the upper Calvert Bluff Formation exposed in the highwall of Big Brown Mine, Fairfield, Texas 

    E-Print Network [OSTI]

    Sturdy, Michael Dale

    2006-10-30

    or liquefaction of adjacent sandy banks (Turner and Munro, 1987; Reading, 1996). Incised Valley Fill Description These brown to gray fine-grained cross stratified sands vary from zero to over 70 feet (21.3 m) thick. The lower bounding contact is an erosion surface...

  20. Influence of Drought Conditions on Brown Trout Biomass and Size Structure in the Black Hills, South Dakota

    E-Print Network [OSTI]

    of pool habitat can limit the carrying capacity for adult fish (Elliot 1987; Hakala and Hartman 2004). Elliot (2000) found that temperature increased and oxygen decreased as pool size decreased during drought pools during nondrought years (Elliot 2000). The survival of brown trout can be affected by drought

  1. Overview of the SSX-FRC experiment M. R. Brown, C. D. Cothran, M. Landreman, V. S. Lukin

    E-Print Network [OSTI]

    Washington at Seattle, University of

    be a big step towards an FRC fusion reactor. Design and construction: Plasma in SSX-FRC will stillOverview of the SSX-FRC experiment M. R. Brown, C. D. Cothran, M. Landreman, V. S. Lukin Swarthmore to produce a Field Reversed Configuration (FRC) by merging two counter-helicity spheromaks. A new, higher

  2. Hanbury-Brown-Twiss Interferometry with Identical Bosons in Relativistic Heavy Ion Collisions: Comparisons with Hadronic Scattering Models

    E-Print Network [OSTI]

    Thomas J. Humanic

    2005-10-17

    Identical boson Hanbury-Brown-Twiss interferometry as applied to relativistic heavy-ion collisions is reviewed. Emphasis is placed on the use of hadronic scattering models to interpret the physical significance of experimental results. Interferometric studies with center-of-mass energies from < 1 GeV/nucleon up to 5500 GeV/nucleon are considered.

  3. On Pipelining Dynamic Instruction Scheduling Logic Jared Stark y Mary D. Brown z Yale N. Patt z

    E-Print Network [OSTI]

    Patt, Yale

    On Pipelining Dynamic Instruction Scheduling Logic Jared Stark y Mary D. Brown z Yale N. Patt z operation. Either you sacrifice IPC by pipelin­ ing this logic, thereby eliminating its ability to execute de­ pendent instructions in consecutive cycles. Or you sacrifice clock frequency by not pipelining it

  4. New Joint Design for Three-dimensional Hyper Redundant Robots Elie Shammas Alon Wolf H. Ben Brown, Jr. Howie Choset

    E-Print Network [OSTI]

    Choset, Howie

    New Joint Design for Three-dimensional Hyper Redundant Robots Elie Shammas Alon Wolf H. Ben Brown makes it ideal for constructing spatial or three-dimensional hyper redundant robots. We also identify that are suitable for constructing spatial hyper redundant (SHR) robots, i.e., SHR robots with three- dimensional

  5. Abstract of "Revealing White Matter Fiber Structure with Diffusion Imaging" by Song Zhang, Ph.D., Brown University, August 2006.

    E-Print Network [OSTI]

    Laidlaw, David

    . Apart from qualitative exploration, I also present quantitative methods such as metrics on tractography. The work in this dissertation advances both qualitative visualization and quantitative analysis of the 3D. S., Nankai University, 1996 Sc. M, Brown University, 2000 Ph.D. Thesis Providence, Rhode Island

  6. The adhesive strength of the palettes of males of a boreal water beetle, Dytiscus alaskanus J. Balfour Browne (Coleoptera: Dytiscidae)

    E-Print Network [OSTI]

    Aiken, Ron

    The adhesive strength of the palettes of males of a boreal water beetle, Dytiscus alaskanus J., and KHAN,A. 1992. The adhesive strength of the palettes of males of a boreal water beetle, Dytiscus alaskanus J. Balfour Browne (Coleoptera: Dytiscidae). Can. J. Zool. 70: 1321- 1324. The adhesive strength

  7. SED modeling of Young Massive Stars

    E-Print Network [OSTI]

    Thomas P. Robitaille

    2007-11-27

    In this contribution, I review the applications and potential limitations of the spectral energy distribution fitting tool that I have developed, with a strong emphasis on the limits to which this tool can be used to improve our understanding of massive star formation. I discuss why our current grid of models cannot be used to distinguish between the several competing theories of massive star formation. I also discuss stellar mass determinations, artificial correlations between parameters in the grid of models, multiplicity, confusion, dust assumptions, and unique fits. I briefly review the improvements we intend to carry out for our next grid of models, which will eliminate many of these limitations. Finally, I show examples of applications of this tool to massive young stars.

  8. Isokinetic Peak Torque in Young Wrestlers

    E-Print Network [OSTI]

    Housh, Terry J.; Johnson, Glen O.; Housh, Dona J.; Stout, Jeffrey R.; Weir, Joseph P.; Weir, Loree L.; Eckerson, Joan M.

    1996-01-01

    previous studies (13, 21, 26) were within 1 stan- dard deviation of the means for the present sample of young wrestlers. These 146 — Housh, Johnson, Housh, etal. i i. E o 00 S 2 o o i en CN' —' ~ en — (N en" — — t A A A A A A A A A A A A A A A A A vo...»n'^mr^voiO':t"fnvow~i"^mvo'0"^m ooooooooaoooooooo en d +1 CN d +1 in d +1 en d +1 CN d +1 >n od +1 OS 14 5 9.7 +1 • VO t-; od +1 15 2.: GO 14 6.6 + 1 in VO +1 f^ CN vq +1 vq 13 3 +1 CN d +1 m 40 .: 1.1 +1 VO 52 . o d +1 45 .0 39 .4 ± 7, 1-: +1 OS od en OS +1 32 . p en +1...

  9. Are Low Surface Brightness Discs Young?

    E-Print Network [OSTI]

    Paolo Padoan; Raul Jimenez; Vincenzo Antonuccio-Delogu

    1996-09-12

    We reconsider the problem of the age of the stellar discs of late-type Low Surface Brightness (LSB) galaxies by making use of a new IMF recently derived from numerical fluid dynamical simulations (Padoan, Nordlund and Jones, 1997). While a Miller-Scalo IMF cannot adequately describe the photometric properties of LSBs, when we apply the new Padoan et al. (1997) IMF to a simple exponential disc model with parameters appropriate to LSBs, we get excellent fits of the colors and color gradients. We then conclude that: a) The star formation history of LSB disc galaxies can be described by an initial burst of a few times $10^7$ yr followed by a quiescent period with only sporadic star formation; b) LSBs' discs are not young. The age of the LSB disc galaxies for which colors have been measured are all larger than about 10 Gyr$.

  10. Peach Growing in Texas. 

    E-Print Network [OSTI]

    Kyle, E. J. (Edwin Jackson)

    1905-01-01

    ............................................................................................................ LaGrange ............................................ L. D. AMSLER .......... Hempstead ............................................................................. A. J. BROWN. Dallas STATION OFFICERS H. H. HARRINGTON, M. S., President... ....................................................................... G. S. FRAPS : . Acting Chemist . . R. L. BENNETT ................................................................................... Cotton Spec~al~st 0. M. BALL...

  11. Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 20945

    E-Print Network [OSTI]

    I. Baraffe; G. Chabrier; T. Barman; F. Allard; P. H. Hauschildt

    2003-02-14

    We present evolutionary models for cool brown dwarfs and extra-solar giant planets. The models reproduce the main trends of observed methane dwarfs in near-IR color-magnitude diagrams. We also present evolutionary models for irradiated planets, coupling for the first time irradiated atmosphere profiles and inner structures. We focus on HD 209458-like systems and show that irradiation effects can substantially affect the radius of sub-jovian mass giant planets. Irradiation effects, however, cannot alone explain the large observed radius of HD 209458b. Adopting assumptions which optimise irradiation effects and taking into account the extension of the outer atmospheric layers, we still find $\\sim$ 20% discrepancy between observed and theoretical radii. An extra source of energy seems to be required to explain the observed value of the first transit planet.

  12. On the Cool Side: Modeling the Atmospheres of Brown Dwarfs and Giant Planets

    E-Print Network [OSTI]

    Marley, Mark S

    2014-01-01

    The atmosphere of a brown dwarf or extrasolar giant planet controls the spectrum of radiation emitted by the object and regulates its cooling over time. While the study of these atmospheres has been informed by decades of experience modeling stellar and planetary atmospheres, the distinctive characteristics of these objects present unique challenges to forward modeling. In particular, complex chemistry arising from molecule-rich atmospheres, molecular opacity line lists (sometimes running to 10 billion absorption lines or more) multiple cloud-forming condensates, and disequilibrium chemical processes all combine to create a challenging task for any modeling effort. This review describes the process of incorporating these complexities into one-dimensional radiative-convective equilibrium models of sub-stellar objects. We discuss the underlying mathematics as well as the techniques used to model the physics, chemistry, radiative transfer, and other processes relevant to understanding these atmospheres. The revi...

  13. Hanbury Brown-Twiss effect and thermal light ghost imaging: A unified approach 

    E-Print Network [OSTI]

    Wang, Li-Gang; Qamar, Sajid; Zhu, Shi-Yao; Zubairy, M. Suhail

    2009-01-01

    /z=2x10 -4 #1;I/z=10 -3 #1;I/z=10 -2 #1;I/z=0.1 FIG. 2. #1;Color online#2; HBT effect for different ?I / z?=10?4 , 2#5;10?4 ,10?3 ,10?2, and 0.1 #1;from top to below#2;, with ?g=10 and z?=105. WANG et al. PHYSICAL REVIEW A 79, 033835 #1;2009...#2; ?I / z?1=0.2, with ?g=4, #1;d#2; ?I / z?1=0.2 and ?g=1, and #1;e#2; ?I / z?1=0.2 and ?g=0.1. HANBURY BROWN?TWISS EFFECT AND THERMAL LIGHT? PHYSICAL REVIEW A 79, 033835 #1;2009#2; 033835-3 and one-third. The more information in the object...

  14. X-ray Detection from Bona-fide and Candidate Brown Dwarfs in the Rho Ophiuchi Cloud with Chandra

    E-Print Network [OSTI]

    Kensuke Imanishi; Masahiro Tsujimoto; Katsuji Koyama

    2001-08-06

    We present results of an X-ray search from bona-fide and candidate brown dwarfs in the Rho Ophiuchi cloud cores with the Chandra X-ray Observatory. The selected areas are two fields near the cloud center and are observed with the ACIS-I array of a 17'x17' size and a ~100 ks exposure. Among 18 bona-fide and candidate brown dwarfs listed by the infrared spectroscopy, we find X-ray emission from 7 sources above 99.9% confidence level. Therefore ~40% of the infrared-selected brown dwarfs in this cloud emit X-rays. For the brightest 4 sources, the X-ray spectra are made and are fitted with a thin-thermal plasma model of a temperature 1-2.5 keV. The X-rays are also time variable with rapid flares from 2 of the brown dwarfs. Assuming 2 keV temperature and using the empirical relation of Av vs. NH, we estimate the X-ray luminosity or its upper limit of the other faint or non-X-ray sources. The X-ray luminosity (Lx) of the X-ray-detected sources is in the range of 0.3-90x10^28 ergs s^-1, while the luminosity ratio of X-ray to bolometric (Lx/Lbol) is 10^-3 - 10^-5, similar to those of low-mass pre-main-sequence and dMe stars. All these results suggest that the X-ray origin of brown dwarfs is the same as low-mass stars; strong magnetic activity at the stellar surface.

  15. Tunable Young's Modulus in Carbon MEMS using Graphene-based Stiffeners...

    Office of Scientific and Technical Information (OSTI)

    Tunable Young's Modulus in Carbon MEMS using Graphene-based Stiffeners. Citation Details In-Document Search Title: Tunable Young's Modulus in Carbon MEMS using Graphene-based...

  16. Black holes in young stellar clusters

    SciTech Connect (OSTI)

    Goswami, Sanghamitra; Kiel, Paul; Rasio, Frederic A. [Department of Physics and Astronomy, Northwestern University, Evanston, IL 60208 (United States)

    2014-02-01

    We present theoretical models for stellar black hole (BH) properties in young, massive star clusters. Using a Monte Carlo code for stellar dynamics, we model realistic star clusters with N ? 5 × 10{sup 5} stars and significant binary fractions (up to 50%) with self-consistent treatments of stellar dynamics and stellar evolution. We compute the formation rates and characteristic properties of single and binary BHs for various representative ages, cluster parameters, and metallicities. Because of dynamical interactions and supernova (SN) kicks, more single BHs end up retained in clusters compared to BHs in binaries. We also find that the ejection of BHs from a cluster is a strong function of initial density. In low-density clusters (where dynamical effects are negligible), it is mainly SN kicks that eject BHs from the cluster, whereas in high-density clusters (initial central density ? {sub c}(0) ? 10{sup 5} M {sub ?} pc{sup –3} in our models) the BH ejection rate is enhanced significantly by dynamics. Dynamical interactions of binary systems in dense clusters also modify the orbital period and eccentricity distributions while increasing the probability of a BH having a more massive companion.

  17. Young Stellar Objects in the Gould Belt

    E-Print Network [OSTI]

    Dunham, Michael M; Evans, Neal J; Broekhoven-Fiene, Hannah; Cieza, Lucas; Di Francesco, James; Gutermuth, Robert A; Harvey, Paul M; Hatchell, Jennifer; Heiderman, Amanda; Huard, Tracy; Johnstone, Doug; Kirk, Jason M; Matthews, Brenda C; Miller, Jennifer F; Peterson, Dawn E; Young, Kaisa E

    2015-01-01

    We present the full catalog of Young Stellar Objects (YSOs) identified in the 18 molecular clouds surveyed by the Spitzer Space Telescope "cores to disks" (c2d) and "Gould Belt" (GB) Legacy surveys. Using standard techniques developed by the c2d project, we identify 3239 candidate YSOs in the 18 clouds, 2966 of which survive visual inspection and form our final catalog of YSOs in the Gould Belt. We compile extinction corrected SEDs for all 2966 YSOs and calculate and tabulate the infrared spectral index, bolometric luminosity, and bolometric temperature for each object. We find that 326 (11%), 210 (7%), 1248 (42%), and 1182 (40%) are classified as Class 0+I, Flat-spectrum, Class II, and Class III, respectively, and show that the Class III sample suffers from an overall contamination rate by background AGB stars between 25% and 90%. Adopting standard assumptions, we derive durations of 0.40-0.78 Myr for Class 0+I YSOs and 0.26-0.50 Myr for Flat-spectrum YSOs, where the ranges encompass uncertainties in the ado...

  18. Who is Park Joo Young?, A Documentary Film

    E-Print Network [OSTI]

    Kopacz, Elizabeth Min-Sook

    2014-01-01

    Park Joo Young? , A Documentary Film A thesis submitted indocumentary narratives. I am drawn to firmly establishing the constructed nature of filmdocumentaries are visual by nature. Along a similar line, I was supposed to film

  19. Young fathers and their experiences of forming families 

    E-Print Network [OSTI]

    Ross, Nicola; Church, Stephanie; Hill, Malcolm; Seaman, Peter; Roberts, Tom

    The male partners of teenage mothers are often ignored or portrayed negatively. This briefing outlines a study that set out to see what could be learned about fathers’ roles by interviewing young couples who were committed ...

  20. BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 27, Part I

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 27, Part I Preble Formation, a Cambrian Outer ..........................................................................J. Roger Olsen Geology of the Sterling Quadrangle, Sanpete County, Utah ..............................................................................James Michael Taylor Publications and Maps of the Geology Department Cover: Aertalphorograph rhowing

  1. Brigham Young University Geology Studies Volume 28, Part 3

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;Brigham Young University Geology Studies Volume 28, Part 3 CONTENTS Three Creeks Caldera ................................................................................................................................... Scott Dean Geology of the Antelope Peak Area of the Southern .................................................................................................................. Craig D. Hall Geology of the Longlick and White Mountain Area, Southern San Francisco Mountains

  2. Cool with Change: Young People and Family Change 

    E-Print Network [OSTI]

    Highet, Gill; Jamieson, Lynn

    Cool with Change breaks new grounds by combining in-depth research of young people’s experience of family change in Scotland, reflection by service providers on the implications for their services and consultation with ...

  3. Field Testing of Activated Carbon Injection Options for Mercury Control at TXU's Big Brown Station

    SciTech Connect (OSTI)

    John Pavlish; Jeffrey Thompson; Christopher Martin; Mark Musich; Lucinda Hamre

    2009-01-07

    The primary objective of the project was to evaluate the long-term feasibility of using activated carbon injection (ACI) options to effectively reduce mercury emissions from Texas electric generation plants in which a blend of lignite and subbituminous coal is fired. Field testing of ACI options was performed on one-quarter of Unit 2 at TXU's Big Brown Steam Electric Station. Unit 2 has a design output of 600 MW and burns a blend of 70% Texas Gulf Coast lignite and 30% subbituminous Powder River Basin coal. Big Brown employs a COHPAC configuration, i.e., high air-to-cloth baghouses following cold-side electrostatic precipitators (ESPs), for particulate control. When sorbent injection is added between the ESP and the baghouse, the combined technology is referred to as TOXECON{trademark} and is patented by the Electric Power Research Institute in the United States. Key benefits of the TOXECON configuration include better mass transfer characteristics of a fabric filter compared to an ESP for mercury capture and contamination of only a small percentage of the fly ash with AC. The field testing consisted of a baseline sampling period, a parametric screening of three sorbent injection options, and a month long test with a single mercury control technology. During the baseline sampling, native mercury removal was observed to be less than 10%. Parametric testing was conducted for three sorbent injection options: injection of standard AC alone; injection of an EERC sorbent enhancement additive, SEA4, with ACI; and injection of an EERC enhanced AC. Injection rates were determined for all of the options to achieve the minimum target of 55% mercury removal as well as for higher removals approaching 90%. Some of the higher injection rates were not sustainable because of increased differential pressure across the test baghouse module. After completion of the parametric testing, a month long test was conducted using the enhanced AC at a nominal rate of 1.5 lb/Macf. During the time that enhanced AC was injected, the average mercury removal for the month long test was approximately 74% across the test baghouse module. ACI was interrupted frequently during the month long test because the test baghouse module was bypassed frequently to relieve differential pressure. The high air-to-cloth ratio of operations at this unit results in significant differential pressure, and thus there was little operating margin before encountering differential pressure limits, especially at high loads. This limited the use of sorbent injection as the added material contributes to the overall differential pressure. This finding limits sustainable injection of AC without appropriate modifications to the plant or its operations. Handling and storage issues were observed for the TOXECON ash-AC mixture. Malfunctioning equipment led to baghouse dust hopper plugging, and storage of the stagnant material at flue gas temperatures resulted in self-heating and ignition of the AC in the ash. In the hoppers that worked properly, no such problems were reported. Economics of mercury control at Big Brown were estimated for as-tested scenarios and scenarios incorporating changes to allow sustainable operation. This project was funded under the U.S. Department of Energy National Energy Technology Laboratory project entitled 'Large-Scale Mercury Control Technology Field Testing Program--Phase II'.

  4. SUPPLEMENTAL FIGURES Fig. S1 a-d: Cloud photographs taken on the Ron H. Brown on 29 October 2008 between 1 and

    E-Print Network [OSTI]

    Yuter, Sandra

    SUPPLEMENTAL FIGURES Fig. S1 a-d: Cloud photographs taken on the Ron H. Brown on 29 October 2008 `Wilbanksetal2015_supplemental_animation.mp4' Hourly GOES satellite IR image loop capturing the cloud field

  5. The Spatial Structure of Young Stellar Clusters. II. Total Young Stellar Populations

    E-Print Network [OSTI]

    Kuhn, Michael A; Feigelson, Eric D

    2015-01-01

    We investigate the intrinsic stellar populations (estimated total numbers of OB and pre-main-sequence stars down to 0.1 Mo) that are present in 17 massive star-forming regions (MSFRs) surveyed by the MYStIX project. The study is based on the catalog of >31,000 MYStIX Probable Complex Members with both disk-bearing and disk-free populations, compensating for extinction, nebulosity, and crowding effects. Correction for observational sensitivities is made using the X-ray Luminosity Function (XLF) and the near-infrared Initial Mass Function (IMF)--a correction that is often not made by infrared surveys of young stars. The resulting maps of the projected structure of the young stellar populations, in units of intrinsic stellar surface density, allow direct comparison between different regions. Several regions have multiple dense clumps, similar in size and density to the Orion Nebula Cluster. The highest projected density of ~34,000 stars/pc^2 is found in the core of the RCW38 cluster. Histograms of surface densit...

  6. Finite element simulations of compositionally graded InGaN solar cells G.F. Brown a,b,n

    E-Print Network [OSTI]

    Wu, Junqiao

    for cheap multi-junction solar cells [4]. Previous simulations have shown that double-junction InxGa1ÀxFinite element simulations of compositionally graded InGaN solar cells G.F. Brown a,b,n , J.W. Ager conversion efficiency of compositionally graded InxGa1ÀxN solar cells was simulated using a finite element

  7. M-dwarf binaries as tracers of star and brown dwarf formation

    E-Print Network [OSTI]

    Marks, Michael; Kroupa, Pavel; Leigh, Nathan; Thies, Ingo

    2015-01-01

    The separation distribution for M-dwarf binaries in the ASTRALUX survey is narrower and peaking at smaller separations than the distribution for solar-type binaries. This is often interpreted to mean that M-dwarfs constitute a continuous transition from brown dwarfs (BDs) to stars. Here a prediction for the M-dwarf separation distribution is presented, using a dynamical population synthesis (DPS) model in which "star-like" binaries with late-type primaries ($\\lesssim1.5 M_{\\rm sun}$) follow universal initial distribution functions and are dynamically processed in their birth embedded clusters. A separate "BD-like" population has both its own distribution functions for binaries and initial mass function (IMF), which overlaps in mass with the IMF for stars. Combining these two formation modes results in a peak on top of a wider separation distribution for late M-dwarfs consistent with the late ASTRALUX sample. The DPS separation distribution for early M-dwarfs shows no such peak and is in agreement with the M-d...

  8. Characterization of novel sorghum brown midrib mutants from an EMS-mutagenized population

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Sattler, Scott E.; Saballos, Ana; Xin, Zhanguo; Funnell-Harris, Deanna L.; Vermerris, Wilfred; Pedersen, Jeffrey F.

    2014-09-02

    Reducing lignin concentration in lignocellulosic biomass can increase forage digestibility for ruminant livestock and saccharification yields of biomass for bioenergy. In sorghum (Sorghum bicolor (L.) Moench) and several other C4 grasses, brown midrib (bmr) mutants have been shown to reduce lignin concentration. Putative bmr mutants isolated from an EMS-mutagenized population were characterized and classified based on their leaf midrib phenotype and allelism tests with the previously described sorghum bmr mutants bmr2, bmr6, and bmr12. These tests resulted in the identification of additional alleles of bmr2, bmr6,and bmr12, and, in addition, six bmr mutants were identified that were not allelic tomore »these previously described loci. Further allelism testing among these six bmr mutants showed that they represented four novel bmr loci. Based on this study, the number of bmr loci uncovered in sorghum has doubled. The impact of these lines on agronomic traits and lignocellulosic composition was assessed in a 2-yr field study. Most of the identified bmr lines showed reduced lignin concentration of their biomass relative to wild-type (WT). Effects of the six new bmr mutants on enzymatic saccharification of lignocellulosic materials were determined, but the amount of glucose released from the stover was similar to WT in all cases. Like bmr2, bmr6, and bmr12, these mutants may affect monolignol biosynthesis and may be useful for bioenergy and forage improvement when stacked together or in combination with the three previously described bmr alleles.« less

  9. Spitzer IRAC mid-infrared photometry of 500-750 brown dwarf

    SciTech Connect (OSTI)

    Saumon, Didier; Leggett, Sandy K; Albert, Loic; Artigau, Etienne; Burningham, Ben; Delfosse, Xavier; Delorme, Philippe; Forveille, Thierry; Lucas, Philip W; Marley, Mark S; Pinfield, David J; Reyle, Celine; Smart, Richard L; Warren, Stephen J

    2010-10-26

    Mid-infrared data, including Spitzer warm-IRAC [3.6] and [4.5] photometry, is critical for understanding the cold population of brown dwarfs now being found, objects which have more in common with planets than stars. As effective temperature (T{sub eff}) drops from 800K to 400K, the fraction of flux emitted beyond 3 {mu}m increases rapidly, from about 40% to > 75%. This rapid increase makes a color like H-[4.5] a very sensitive temperature indicator, and it can be combined with a gravity- and metallicity-sensitive color like H-K to constrain all three of these fundamental properties, which in turn gives us mass and age for these slowly cooling objects. Determination of mid-infrared color trends also allows better exploitation of the WISE mission by the community. We use new Spitzer Cycle 6 IRAC photometry, together with published data, to present trends of color with type for L0 to T10 dwarfs. We also use the atmospheric and evolutionary models of Saumon and Marley to investigate the masses and ages of 13 very late-type T dwarfs, which have H-[4.5] > 3.2 and T{sub eff} {approx} 500K to 750K.

  10. Probing the properties of event-by-event distributions in Hanbury-Brown--Twiss radii

    E-Print Network [OSTI]

    Plumberg, Christopher

    2015-01-01

    Hanbury-Brown--Twiss interferometry is a technique which yields effective widths (i.e., "HBT radii") of homogeneity regions in the fireballs produced in heavy ion collisions. Because the initial conditions of these collisions are stochastically fluctuating, the measured HBT radii also exhibit variation on an event-by-event basis. However, HBT measurements have, to date, been performed only on an ensemble-averaged basis, due to inherent limitations of finite particle statistics. In this paper, we show that experimental measurements to date are best characterized theoretically as weighted averages of the event-by-event HBT radii, and we propose a new method for extracting experimentally both the arithmetic mean and the variance of the event-by-event distribution of HBT radii. We demonstrate the extraction of the mean and variance of this distribution for a particular ensemble of numerically generated events, and offer some ideas to extend and generalize the method to enable measurement of higher moments of the ...

  11. Probing the properties of event-by-event distributions in Hanbury-Brown--Twiss radii

    E-Print Network [OSTI]

    Christopher Plumberg; Ulrich Heinz

    2015-07-17

    Hanbury-Brown--Twiss interferometry is a technique which yields effective widths (i.e., "HBT radii") of homogeneity regions in the fireballs produced in heavy ion collisions. Because the initial conditions of these collisions are stochastically fluctuating, the measured HBT radii also exhibit variation on an event-by-event basis. However, HBT measurements have, to date, been performed only on an ensemble-averaged basis, due to inherent limitations of finite particle statistics. In this paper, we show that experimental measurements to date are best characterized theoretically as weighted averages of the event-by-event HBT radii, and we propose a new method for extracting experimentally both the arithmetic mean and the variance of the event-by-event distribution of HBT radii. We demonstrate the extraction of the mean and variance of this distribution for a particular ensemble of numerically generated events, and offer some ideas to extend and generalize the method to enable measurement of higher moments of the HBT distribution as well.

  12. Effects of water hardness on the toxicity of manganese to developing brown trout (Salmo trutta)

    SciTech Connect (OSTI)

    Stubblefield, W.A.; Garrison, T.D.; Hockett, J.R.; Brinkman, S.F.; Davies, P.H.; McIntyre, M.W.

    1997-10-01

    Manganese is a common constituent of point and nonpoint discharges from mining and smelting activities. Available data indicate that Mn is acutely toxic at relatively high aqueous concentrations, when compared with trace metals, and its toxicity is affected by water hardness. Little information is available regarding the chronic toxicity of manganese. Early-life-stage (ELS) tests were conducted to determine the toxicity of manganese to brown trout (Salmo trutta) and to evaluate the extent to which water hardness (ranging from 30 to 450 mg/L as CaCO{sub 3}) affects the chronic toxicity of Mn. Water hardness of significantly affected Mn chronic toxicity, with toxicity decreasing with increasing hardness. Decreased survival was the predominant effect noted in the 30-mg/L hardness experiment, while significant effects on growth (as measured by changes in body weight) were observed in both the 150- and 450-mg/L hardness experiments. Twenty-five percent inhibition concentration (IC25) values, based on the combined endpoints (i.e., survival and body weight), were 4.67, 5.59, and 8.68 mg Mn/L (based on measured Mn concentration) at hardness levels of approximately 30, 150, and 450 mg/L as CaCO{sub 3}, respectively.

  13. A Brown Dwarf Microlens Candidate in the OGLE-II Database

    E-Print Network [OSTI]

    M. C. Smith; S. Mao; P. R. Wozniak

    2003-01-16

    We describe a unique mass determination for a microlensing event from the second phase of the Optical Gravitational Microlensing Experiment (OGLE-II). The event, sc26_2218, which is very bright (baseline magnitude I=15.10), appears to exhibit both parallax and finite source effects. The parallax effect allows us to determine the projected Einstein radius on the observer plane (approx. 3.8 AU), while the finite source effect allows us to determine the ratio of the angular source size and the angular Einstein radius. As the angular size of the star can be estimated using its color and magnitude, we can hence determine the angular Einstein radius (approx. 0.1 mas). By combining both the projected and angular Einstein radius we can determine the lens mass M = 0.050^{+0.016}_{-0.011} solar masses, independent of the source distance. The lens is therefore a brown dwarf candidate. However, the `parallax' signature is weak and so we cannot completely discount the possibility that these signatures originate from binary rotation of the source (which would prevent any estimate of the lens mass), rather than parallax. However, this can be tested by future spectroscopic observations. This event highlights the scientific returns for intense monitoring of bright microlensing events, since the parallax and finite source effects can be more easily identified due to their high signal-to-noise ratios.

  14. Pyrolysis product distribution of a Victorian brown coal under high pressures

    SciTech Connect (OSTI)

    Sathe, C.; Li, C.Z.

    1999-07-01

    A Loy Yang brown coal sample was pyrolyzed in a wire-mesh reactor at pressures ranging from 100 kPa to 1000 kPa. Tar yield was found to be very sensitive to changes in heating rate, peak temperature, holding time and pressure. Tar yield decreased with increases in pressure at high heating rate. At low heating rate tar yield was not sensitive to changes in pressure. Char yields were found to be much less sensitive to changes in pressure and/or heating rate. UV absorption spectroscopy of the tar samples indicated that the yields of larger aromatic ring systems decreased with increasing pressure and/or decreasing heating rate. The effects of pressure are mainly due to the changes in the transportation of volatile precursors with pressure. Increases in pressure might have slowed down the bulk diffusion within meso- and macro-pores in char, which in turn have slowed down the Knudsen diffusion in the micro-pores due to the reduced concentration gradients for the Knudsen diffusion. During the extended stay within the char particle, volatile precursors were thermally cracked, leading to the retention of some larger aromatic ring systems as char and the release of other components as tar and gas.

  15. CANDIDATES FOR THE YOUNG STELLAR OUTFLOWS: WATER AND METHANOL MASERS FROM YOUNG STELLAR OBJECTS

    SciTech Connect (OSTI)

    Lim, Wanggi; Lyo, A-Ran; Kim, Kee-Tae; Byun, Do-Young [Korea Astronomy and Space Science Institute, Daedeok Street 776, Yuseong-Gu, 305-348 Daejeon (Korea, Republic of)

    2012-11-01

    We conducted simultaneous 22 GHz water maser and 44 GHz class I methanol maser surveys of newly identified 282 H{sub 2} emission features from the 2.122 {mu}m H{sub 2} narrowband image survey in the Galactic plane (UWISH2 project) using Korean VLBI Network 21 m radio telescopes. We detected 16 and 13 new water and methanol maser sources, respectively. This result indicates that at least {approx}5% of the H{sub 2} emission features originate from young stellar objects (YSOs) that are in the right physical condition to produce the water and methanol masers. The masers are closely related to the current outflow activities in the Galactic plane. The power sources of these 23 diffused/collimated H{sub 2} emission features (six sources are detected for both masers) are likely to be intermediate- to high-mass YSOs, based on a comparison with the maser luminosities of other well-studied YSOs. Both maser velocities are mostly close to their own systemic velocities within {approx}<5 km s{sup -1}, even though water masers generally show larger variabilities in the intensity, velocity, and shape than methanol masers. We also discovered three new water maser sources with high-velocity components: {approx}25 km s{sup -1} redshifted CMHO 019, {approx}50 km s{sup -1} blueshifted CMHO 132, and {approx}120 km s{sup -1} blueshifted CMHO 182. In particular, we propose that the dominant blueshifted water maser of CHMO 182 can be a unique laboratory for the study of the high-mass young stellar jet and its acceleration.

  16. Formation of NH{sub 3} during the pyrolysis of a brown coal

    SciTech Connect (OSTI)

    Li, C.Z.; Pang, Y.; Li, X.G. [Monash Univ., Clayton, Victoria (Australia). Dept. of Chemical Engineering

    1998-12-31

    Emissions of oxides of nitrogen (NO, NO{sub 2} and N{sub 2}O) from power generation using coal are an important environmental problem, contributing to the formation of photochemical smog and acid rain or to the enhancement of greenhouse effects and to the enhanced depletion of stratospheric ozone. During pyrolysis, the nitrogen in coal, as a part of coal organic matter, is converted into NOx precursors (eg. NH{sub 3}, HCN, HNCO and the nitrogen in tar and char). These NOx precursors may then be converted into either NOx or N{sub 2} during subsequent combustion or gasification/combustion. The conversion efficiency of these NOx precursors into NOx depends strongly upon the type of NOx precursor. Knowledge of the formation of these NOx precursors during pyrolysis is therefore essential for the accurate predictions of NOx emissions from large scale power plants, and therefore for the development of optimum strategies for NOx reduction. Formation of NH{sub 3} during the pyrolysis of a Victorian brown coal (Loy Yang) has been studied in a novel reactor. The experimental results obtained suggest that a considerable amount of the nitrogen in the nascent char could be converted into NH{sub 3} if the char is held at high temperatures for a long period of time. The formation of NH{sub 3} from the thermal cracking of char was seen to last for more than an hour even at temperatures as high as 700--900 C. The experimental results seem to suggest that the differences in reactor geometries would account at least partially for some of the discrepancies in the literature regarding the formation of NH{sub 3} during the pyrolysis of coals. It is thought that NH{sub 3} may be formed from the hydrogenation of the N sites in the char by the active hydrogen generated from the thermal cracking of the char.

  17. Properties of Young Massive Cluster Derived from Photometry

    E-Print Network [OSTI]

    U. Fritze-v. Alvensleben

    2004-08-25

    I will show that photometry -- if extending over a reasonable choice of passbands -- can give fairly precise information about young star clusters and their evolutionary state. Optical colors alone are known to leave severe ambiguities due to degeneracies between age, metallicity and extinction. High quality photometry including $U, B, V$ or $I$, and a NIR band, however, in combination with an extensive grid of evolutionary synthesis models for star clusters and a dedicated tool to analyse spectral energy distributions allows to assess and largely disentangle star cluster ages, metallicities, extinction values and, hence, to derive their masses. Gaseous emission contributions sensibly affect broad band colors during the youngest stages, depending on metallicity. Mass functions of young star cluster systems may considerably differ in shape from luminosity functions. An ESO ASTROVIRTEL project provides multi-color photometry for a large number of young, intermediate age and old star cluster systems. As a first example I show results obtained for NGC 1569.

  18. Acceleration of wound healing in young and aged rats 

    E-Print Network [OSTI]

    Maxwell, Bryan Douglas

    1996-01-01

    1. The effect of ACM on wound healing in young rats. . Page 15 2. The effect of ACM on wound healing in old, ad-lib rats . . . . . . . 17 3. The effect of ACM on wound healing in old, caloric-restricted rats . . . 4. The effect of old and young... group (AL) had been fed a laboratory diet ad libitum during their lifetime. The other group (CR) had been maintained on a calorie-restricted diet at a level of 60% of the food intake of the ad libitum-fed group. This decrease in caloric intake resulted...

  19. Severe Accident Sequence Analysis Program: Anticipated transient without scram simulations for Browns Ferry Nuclear Plant Unit 1

    SciTech Connect (OSTI)

    Dallman, R J; Gottula, R C; Holcomb, E E; Jouse, W C; Wagoner, S R; Wheatley, P D

    1987-05-01

    An analysis of five anticipated transients without scram (ATWS) was conducted at the Idaho National Engineering Laboratory (INEL). The five detailed deterministic simulations of postulated ATWS sequences were initiated from a main steamline isolation valve (MSIV) closure. The subject of the analysis was the Browns Ferry Nuclear Plant Unit 1, a boiling water reactor (BWR) of the BWR/4 product line with a Mark I containment. The simulations yielded insights to the possible consequences resulting from a MSIV closure ATWS. An evaluation of the effects of plant safety systems and operator actions on accident progression and mitigation is presented.

  20. A Systematic Study of X-Ray Flares from Low-Mass Young Stellar Objects in the Rho Ophiuchi Star-Forming Region with Chandra

    E-Print Network [OSTI]

    K. Imanishi; H. Nakajima; M. Tsujimoto; K. Koyama; Y. Tsuboi

    2003-05-10

    We report on the results of a systematic study of X-ray flares from low-mass young stellar objects, using Chandra observations of the main region of the Rho Oph. From 195 X-ray sources, including class I-III sources and some young brown dwarfs, we detected a total of 71 X-ray flares. Most of the flares have the typical profile of solar and stellar flares, fast rise and slow decay. We derived the time-averaged temperature (kT), luminosity (L_X), rise and decay timescales (tau_r and tau_d) of the flares, finding that (1) class I-II sources tend to have a high kT, (2) the distribution of L_X during flares is nearly the same for all classes, and (3) positive and negative log-linear correlations are found between tau_r and tau_d, and kT and tau_r. In order to explain these relations, we used the framework of magnetic reconnection model to formulate the observational parameters as a function of the half-length of the reconnected magnetic loop (L) and magnetic field strength (B). The estimated L is comparable to the typical stellar radius of these objects (10^{10-11} cm), which indicates that the observed flares are triggered by solar-type loops, rather than larger ones (10^{12} cm) connecting the star with its inner accretion disk. The higher kT observed for class I sources may be explained by a higher magnetic field strength (about 500 G) than for class II-III sources (200-300 G).

  1. NONPARAMETRIC REGRESSION ESTIMATION OF HOUSEHOLD VMT Young-Jun Kweon

    E-Print Network [OSTI]

    Kockelman, Kara M.

    NONPARAMETRIC REGRESSION ESTIMATION OF HOUSEHOLD VMT Young-Jun Kweon (Corresponding Author Transportation Survey. The results are density functions and regression surfaces for VMT, in relation regressions perform better than their ordinary-least squares counterparts in many ways: they permit full

  2. KnowledgeAssetManagementMentzasApostolou AbeckerYoung

    E-Print Network [OSTI]

    Chen-Burger, Yun-Heh (Jessica)

    123 KnowledgeAssetManagementMentzas·Apostolou Abecker·Young Gregoris Mentzas Dimitris Apostolou Knowledge Asset Management There are two main approaches to knowledge management (KM): · the process Asset Management presents a knowledge asset-centric approach, which fuses the previous two approaches

  3. Activity Identification Utilizing Data Mining Techniques Jae Young Lee

    E-Print Network [OSTI]

    Hoff, William A.

    Activity Identification Utilizing Data Mining Techniques Jae Young Lee Dept. of Math. and Computer belong to. The proposed method utilizes various data mining techniques, including clustering Sciences Colorado School of Mines Golden, Colorado, USA jaelee@mines.edu William Hoff Engineering Division

  4. Sex differences in indirect aggression Psychological evidence from young adults

    E-Print Network [OSTI]

    Sex differences in indirect aggression Psychological evidence from young adults Nicole H. Hessa theories of sex differences in indirect aggression propose selection pressures that would have acted on older teenagers and adults. Evidence for sex differences in indirect aggression in adults, however

  5. The New York State Summer Young Writers Institute

    E-Print Network [OSTI]

    Alexandrova, Ivana

    #12;The New York State Summer Young Writers Institute This anthology contains poems, stories, and creative nonfiction pieces produced by the talented high school writers of the 2009 New York State Summer held in July on the campus of Skidmore College in Saratoga Springs, New York, to coincide with one week

  6. Brigham Young University Geology Studies Volume 29, Part 2

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;Brigham Young University Geology Studies Volume 29, Part 2 CONTENTS Stratigraphy ...................................................................................................... Terry C. Gosney 27 Geology of the Champlin Peak Quadrangle,Juab and Millard Counties, Utah ..................................................................................................................................... David R. Keller 103 Publications and Maps of the Department of Geology 117 Cover: Rafted orjoreign

  7. VOLUMF -31, PART 1 BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES

    E-Print Network [OSTI]

    Seamons, Kent E.

    Y O U N G VOLUMF -31, PART 1 #12;BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES VOLUME 31.PART 1 CONTENTS .................................................................. Ralph E.Lambert Geology of the Mount Ellen Quadrangle. Henry Mountains. Garfield County. Utah near White Horse Pass. Elko County. Nevada ............Stephen M Smith Geology of the Steele Butte

  8. BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 27, Part 3

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 27, Part 3 CONTENTS Studies for Students #lo, Geologic Guide to Provo Canyon and Weber Canyon, Central Wasatch Mountains, Utah ............................................................................................................................. Randy L. Chamberlain The Geology of the Drum Mountains, Millard and Juab Counties, Utah

  9. Brigham Young University Geology Studies Volume 27, Part 2

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;Brigham Young University Geology Studies Volume 27, Part 2 CONTENTS The Kinnikinic Quartzite ........................................................Robert Q. Oaks,Jr., and W . Calvin James Geology of the Sage Valley 7 W'Quadrangle, Caribou County, Idaho, and Lincoln County, Wyoming ....................J ohn L. Conner Geology of the Elk Valley Quadrangle, Bear

  10. Brigham Young University Geology Studies Volume 30, Part 1

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;Brigham Young University Geology Studies Volume 30, Part 1 CONTENTS Diagenetic Aspects ................................................................................................... Steven G. Driese Geology of the Dog Valley-Red Ridge Area, Southern Pavant Mountains, Millard County .................................................................................................. Lynn C Meibos Geology of the Southwestern Quarter of the Scipio North (15-Minute) Quadrangle, Millard

  11. BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 25,Part 1

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 25,Part 1 Papers reviewing geology of field trip areas, 31st annual meeting, Rocky Mountain Section, Geological Society of America, April 28 ....................................................................................................................................................... Geology of Volcanic Rocks and Mineral Deposits in the Southern Thomas Range, Utah: A Brief Summary

  12. Brigham Young University Geology Studies Volume 24, Part 2

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;Brigham Young University Geology Studies Volume 24, Part 2 CONTENTS Studies for Students ............................................................................................................................... Robert C. Ahlborn Publications and Maps of the Geology Department Cover: Sahara dune sand, X130. Photo, Univer~ityof Cincinnati, Cincinnati, Ohio 45221. #12;A publication of the Department of Geology Brigham

  13. How Europe fails its young Sep 8th 2005

    E-Print Network [OSTI]

    Marrucci, Lorenzo

    How Europe fails its young Sep 8th 2005 From The Economist print edition The state of Europe sense of a sort: Europe's only chance of preserving its living standards lies in working smarter than its competitors rather than harder or cheaper. But Europe's failing higher-education system poses

  14. The Young Planet-mass Ob ject 2M1207b: A cool, cloudy, and methane...

    Office of Scientific and Technical Information (OSTI)

    Young Planet-mass Ob ject 2M1207b: A cool, cloudy, and methane-poor atmosphere Citation Details In-Document Search Title: The Young Planet-mass Ob ject 2M1207b: A cool, cloudy, and...

  15. BrighamYoungUniversitySummerInternships DEPARTMENT OF CHEMISTRY AND BIOCHEMISTRY

    E-Print Network [OSTI]

    Seamons, Kent E.

    BrighamYoungUniversitySummerInternships DEPARTMENT OF CHEMISTRY AND BIOCHEMISTRY BRIGHAM YOUNG UNIVERSITY EIGHT WEEK SUMMER UNDERGRADUATE RESEARCH INTERNSHIPS The Department of Chemistry and Biochemistry programs. Summer Term 2013: June 24 through August 12 Requirements: Registered chemistry or biochemistry

  16. BrighamYoungUniversitySummerInternships DEPARTMENT OF CHEMISTRY AND BIOCHEMISTRY

    E-Print Network [OSTI]

    Seamons, Kent E.

    BrighamYoungUniversitySummerInternships DEPARTMENT OF CHEMISTRY AND BIOCHEMISTRY BRIGHAM YOUNG UNIVERSITY EIGHT WEEK SUMMER UNDERGRADUATE RESEARCH INTERNSHIPS The Department of Chemistry and Biochemistry programs. Summer Term 2012: June 18 through August 10 Requirements: Registered chemistry or biochemistry

  17. How was it for you? The quality of young people's sexual relationships 

    E-Print Network [OSTI]

    Wright, Daniel; Forrest, Simon

    Few studies have investigated young people’s own evaluations of their heterosexual experiences or relationships, other than by measuring negative sexual encounters. An evaluation of young peoples’ views is important, to ...

  18. Doing ok? Children and young people's views on what affects their mental health 

    E-Print Network [OSTI]

    Elsley, Susan; McMellon, Christina

    This briefing highlights the findings from a consultation which was undertaken with specific groups of children and young people in order to inform the NHS Health Scotland draft framework for children and young people’s ...

  19. EVIDENCE FOR A WEAK WIND FROM THE YOUNG SUN

    SciTech Connect (OSTI)

    Wood, Brian E.; Müller, Hans-Reinhard; Redfield, Seth; Edelman, Eric

    2014-02-01

    The early history of the solar wind has remained largely a mystery due to the difficulty of detecting winds around young stars that can serve as analogs for the young Sun. Here we report on the detection of a wind from the 500 Myr old solar analog ?{sup 1} UMa (G1.5 V), using spectroscopic observations from the Hubble Space Telescope. We detect H I Ly? absorption from the interaction region between the stellar wind and interstellar medium, i.e., the stellar astrosphere. With the assistance of hydrodynamic models of the ?{sup 1} UMa astrosphere, we infer a wind only half as strong as the solar wind for this star. This suggests that the Sun and solar-like stars do not have particularly strong coronal winds in their youth.

  20. What could infant and young child nutrition learn from sweatshops?

    E-Print Network [OSTI]

    Singer, Peter A; Ansett, Sean; Sagoe-Moses, Isabella

    2011-05-05

    Vitamin A, iron, zinc), essential fats, and energy. Therefore, ade- quate Infant and Young Child Nutrition (IYCN) demands high rates of breastfeeding and good access to nutrient rich complementary foods, requiring public sec- tor action to promote... feeding are diminished with reliable access to Singer et al. BMC Public Health 2011, 11:276 http://www.biomedcentral.com/1471-2458/11/276 Page 2 of 5 clean water. Moreover, the companies claim the Code has shortcomings: it is open to interpretation...

  1. Gravitational wave emission and spin-down of young pulsars

    SciTech Connect (OSTI)

    Alford, Mark G.; Schwenzer, Kai [Department of Physics, Washington University, St. Louis, MO 63130 (United States)

    2014-01-20

    The rotation frequencies of young pulsars are systematically below their theoretical Kepler limit. r-modes have been suggested as a possible explanation for this observation. With the help of semi-analytic expressions that make it possible to assess the uncertainties of the r-mode scenario due to the impact of uncertainties in underlying microphysics, we perform a quantitative analysis of the spin-down and the emitted gravitational waves of young pulsars. We find that the frequency to which r-modes spin-down a young neutron star (NS) is surprisingly insensitive to both the microscopic details and the saturation amplitude. Comparing our result to astrophysical data, we show that for a range of sufficiently large saturation amplitudes r-modes provide a viable spin-down scenario and that all observed young pulsars are very likely already outside the r-mode instability region. Therefore, the most promising sources for gravitational wave detection are unobserved NSs associated with recent supernovae, and we find that advanced LIGO should be able to see several of them. Our analysis shows that despite the coupling of the spin-down and thermal evolution, a power-law spin-down with an effective braking index n {sub rm} ? 7 is realized. Because of this, the gravitational wave strain amplitude is completely independent of both the r-mode saturation amplitude and the microphysics and depends on the saturation mechanism only within some tens of percent. However, the gravitational wave frequency depends on the amplitude, and we provide the required expected timing parameter ranges to look for promising sources in future searches.

  2. Production of high-energy ?neutrinos from young neutron stars

    E-Print Network [OSTI]

    G. F. Burgio; B. Link

    2006-09-20

    Young, rapidly rotating neutron stars could accelerate protons to energies of $\\sim 1$ PeV close to the stellar surface, which scatter with x-rays from the stellar surface through the $\\Delta$ resonance and produce pions. The pions subsequently decay to produce muon neutrinos. We find that the energy spectrum of muon neutrinos consists of a sharp rise at $\\sim 50$ TeV, corresponding to the onset of the resonance, above which the flux drops as $\\epsilon_\

  3. Lean color characteristics of beef from steers and young bulls 

    E-Print Network [OSTI]

    Purser, David Elbert

    1982-01-01

    bulls are more muscular with less fat than those from steers; it would seem logical that beef from young bulls could be utilized at the retail level to provide consumers with retail cuts with less fat. One of the problems associated with marketing... panel evaluations of steaks from retail display, microbial sampling, colorimetric measures of muscle surface light reflectance, pH, and total pigment concentration were analyzed to determine causes, if any, for the differences in muscle color between...

  4. Young Texas Saves Program Leader Instructions Thank you for committing to be a Young Texas Saves Leader. You will make a difference in your 4-H club. Below, we

    E-Print Network [OSTI]

    Young Texas Saves Program Leader Instructions Thank you for committing to be a Young Texas Saves the Saves program. Young Texas Saves is a youth-led movement in the Texas 4-H Program. 4-H members across 3000 4-H members across the state take part in the Young Texas Saves Program. Begin the program

  5. Ensemble Asteroseismology of the Young Open Cluster NGC 2244

    E-Print Network [OSTI]

    Aerts, Conny; Marcos-Arenal, Pablo; Moravveji, Ehsan; Degroote, Pieter; Papics, Peter; Tkachenko, Andrew; De Ridder, Joris; Briquet, Maryline; Thoul, Anne; Saesen, Sophie; Mowlavi, Nami; Barblan, Fabio; Neiner, Coralie; Pavlovski, Kresimir; Guzik, Joyce

    2013-01-01

    Our goal is to perform in-depth ensemble asteroseismology of the young open cluster NGC2244 with the 2-wheel Kepler mission. While the nominal Kepler mission already implied a revolution in stellar physics for solar-type stars and red giants, it was not possible to perform asteroseismic studies of massive OB stars because such targets were carefully avoided in the FoV in order not to disturb the exoplanet hunting. Now is an excellent time to fill this hole in mission capacity and to focus on the metal factories of the Universe, for which stellar evolution theory is least adequate. Our white paper aims to remedy major shortcomings in the theory of stellar structure and evolution of the most massive stars by focusing on a large ensemble of stars in a carefully selected young open cluster. Cluster asteroseismology of very young stars such as those of NGC2244 has the major advantage that all cluster stars have similar age, distance and initial chemical composition, implying drastic restrictions for the stellar mo...

  6. A photometric investigation of the young open cluster Trumpler 15

    E-Print Network [OSTI]

    Carraro, G

    2002-01-01

    In this paper we present and analyze new CCD $UBVRI$ photometry down to $V\\approx$21 in the region of the young open cluster Trumpler~15, located in the Carina spiral feature. The cluster is rather compact and has a core radius of about 2$^{\\prime}$, which translates in about 1 pc at the distance of the cluster. We provide the first CCD investigation and update its fundamental parameters. We identify 90 candidate photometric members on the base of the position in the color-color and color-magnitude diagrams. This sample allows us to obtain a distance of 2.4$\\pm$0.3 kpc from the Sun and a reddening E$(B-V)$=0.52$\\pm0.07$. We confirm that the cluster is young, and fix a upper limit of 6 million yrs to its age . In addition, we draw the attention on the lower part of the Main Sequence (MS) suggesting that some stars can be in contracting phase and on a gap in the MS, that we show to be a real feature, the $B1-B5$ gap found in other young open clusters. We finally study in details the extinction toward Trumpler~1...

  7. NEW CANDIDATE ERUPTIVE YOUNG STARS IN LYNDS 1340

    SciTech Connect (OSTI)

    Kun, M.; Moór, A.; Szegedi-Elek, E. [Konkoly Observatory, H-1121 Budapest, Konkoly Thege út 15-17 (Hungary); Apai, D. [Department of Astronomy and Department of Planetary Sciences, The University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); O'Linger-Luscusk, J. [California Institute of Technology, 1200 East California Avenue, Pasadena, CA 91125 (United States); Stecklum, B. [Thüringer Landessternwarte Tautenburg, Sternwarte 5, D-07778 Tautenburg (Germany); Wolf-Chase, G., E-mail: kun@konkoly.hu [Astronomy Department, Adler Planetarium, 1300 South Lake Shore Drive, Chicago, IL 60605 (United States)

    2014-11-10

    We report on the discovery of three candidate eruptive young stars, found during our comprehensive multi-wavelength study of the young stellar population of the dark cloud L1340. These stars are as follows. (1) IRAS 02224+7227 (2MASS 02270555+7241167, HH 487S) exhibited FUor-like spectrum in our low-resolution optical spectra. The available photometric data restrict its luminosity to 23 L {sub ?} < L {sub bol} < 59 L {sub ?}. (2) 2MASS 02263797+7304575, identified as a classical T Tauri star during our H? survey, exhibited an EXor-type brightening in 2005 November at the time of the Sloan Digital Sky Survey observations of the region. (3) 2MASS 02325605+7246055, a low-mass embedded young star, associated with a fan-shaped infrared nebula, underwent an outburst between the DSS 1 and DSS 2 surveys, leading to the appearance of a faint optical nebula. Our [S II] and H? images, as well as the Spitzer Infrared Array Camera 4.5 ?m images, revealed Herbig-Haro objects associated with this star. Our results suggest that amplitudes and timescales of outbursts do not necessarily correlate with the evolutionary stage of the stars.

  8. The tropical brown alga Lobophora variegata as a bioindicator of mining1 contamination in the New Caledonia lagoon: a field transplantation study2

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    1 The tropical brown alga Lobophora variegata as a bioindicator of mining1 contamination in the New field and laboratory studies have identified the alga Lobophora variegata as a good21 candidate key contaminants, i.e. Ag, As, Cd, Co, Cr,25 Cu, Mn, Ni and Zn. Algae from clean and contaminated

  9. Hydraulic Drivetrain and Regenerative Braking Team 13: Andrew Brown, Karan Desai, Andrew McGrath, Hurst Nuckols, Grant Wilson Adviser: Dr. Andrew Jackson

    E-Print Network [OSTI]

    Carpick, Robert W.

    Hydraulic Drivetrain and Regenerative Braking Team 13: Andrew Brown, Karan Desai, Andrew Mc Pressure Reservior Filter Variable Vane Pump Motor/Pump Hydraulic Accumulators Solenoid Valve Relief Valve Suction Line Since their development in 2006, hydraulic drivetrain systems have gained considerable

  10. ADVANCES IN NOVEL FRC PLASMAS M.J. Schaffer, M.R. Brown, J.A. Leuer, P.B. Parks, C.D. Cothran

    E-Print Network [OSTI]

    Washington at Seattle, University of

    ADVANCES IN NOVEL FRC PLASMAS M.J. Schaffer, M.R. Brown, J.A. Leuer, P.B. Parks, C.D. Cothran fields are stabilizing, an experiment, SSX­FRC, is being prepared to test this and other ideas. The FRCs. Analytical work shows that FRC rotation may initiate self-generation of the antisymmetric toroidal B

  11. 510 Plant Disease / Vol. 97 No. 4 Etiology of Moldy Core, Core Browning, and Core Rot of Fuji Apple in China

    E-Print Network [OSTI]

    Biggs, Alan R.

    510 Plant Disease / Vol. 97 No. 4 Etiology of Moldy Core, Core Browning, and Core Rot of Fuji Apple, and core rot of Fuji apple in China. Plant Dis. 97:510-516. `Fuji' apple fruit were collected in Shaanxi to species. Pathogenicity was determined by cutting apple fruit into halves and daubing spore suspensions

  12. Resource Utilization and Coexistence of Seed-Eating Desert Rodents in Sand Dune Habitats Author(s): James H. Brown and Gerald A. Lieberman

    E-Print Network [OSTI]

    Brown, James H.

    Resource Utilization and Coexistence of Seed-Eating Desert Rodents in Sand Dune Habitats Author UTILIZATION AND COEXISTENCE OF SEED-EATING DESERT RODENTS IN SAND DUNE HABITATS' JAMES H. BROWN Department how these differences affect the utilization of seeds. Our estimates of total overlap in resource

  13. Fracture Testing of a Self-Healing Polymer Composite by E.N. Brown, N.R. Sottos and S.R. White

    E-Print Network [OSTI]

    Sottos, Nancy R.

    Fracture Testing of a Self-Healing Polymer Composite by E.N. Brown, N.R. Sottos and S.R. White with an embedded catalyst. The effects of size and concentration of the catalyst and mi- crocapsules on fracture as much as 90 percent of its virgin fracture toughness. KEY WORDS--Self-healing, autonomic healing

  14. The SOPHIE search for northern extrasolar planets VIII. Follow-up of ELODIE candidates: long-period brown-dwarf companions

    E-Print Network [OSTI]

    Bouchy, F; Díaz, R F; Forveille, T; Boisse, I; Arnold, L; Astudillo-Defru, N; Beuzit, J -L; Bonfils, X; Borgniet, S; Bourrier, V; Courcol, B; Delfosse, X; Demangeon, O; Delorme, P; Ehrenreich, D; Hébrard, G; Lagrange, A -M; Mayor, M; Montagnier, G; Moutou, C; Naef, D; Pepe, F; Perrier, C; Queloz, D; Rey, J; Sahlmann, J; Santerne, A; Santos, N C; Sivan, J -P; Udry, S; Wilson, P A

    2015-01-01

    Long-period brown dwarf companions detected in radial velocity surveys are important targets for direct imaging and astrometry to calibrate the mass-luminosity relation of substellar objects. Through a 20-year radial velocity monitoring of solar-type stars that began with ELODIE and was extended with SOPHIE spectrographs, giant exoplanets and brown dwarfs with orbital periods longer than ten years are discovered. We report the detection of five new potential brown dwarfs with minimum masses between 32 and 83 Jupiter mass orbiting solar-type stars with periods longer than ten years. An upper mass limit of these companions is provided using astrometric Hipparcos data, high-angular resolution imaging made with PUEO, and a deep analysis of the cross-correlation function of the main stellar spectra to search for blend effects or faint secondary components. These objects double the number of known brown dwarf companions with orbital periods longer than ten years and reinforce the conclusion that the occurrence of s...

  15. Atmospheric Chemistry in Giant Planets, Brown Dwarfs, and Low-Mass Dwarf Stars II. Sulfur and Phosphorus

    E-Print Network [OSTI]

    Channon Visscher; Katharina Lodders; Bruce Fegley Jr

    2006-06-06

    Thermochemical equilibrium and kinetic calculations are used to model sulfur and phosphorus chemistry in giant planets, brown dwarfs, and extrasolar giant planets (EGPs). The chemical behavior of individual S- and P-bearing gases and condensates is determined as a function of pressure, temperature, and metallicity. The results are independent of particular model atmospheres and, in principle, the equilibrium composition along the pressure-temperature profile of any object can be determined. Hydrogen sulfide (H2S) is the dominant S-bearing gas throughout substellar atmospheres and approximately represents the atmospheric sulfur inventory. Silicon sulfide (SiS) is a potential tracer of weather in substellar atmospheres. Disequilibrium abundances of phosphine (PH3) approximately representative of the total atmospheric phosphorus inventory are expected to be mixed upward into the observable atmospheres of giant planets and T dwarfs. In hotter objects, several P-bearing gases (e.g., P2, PH3, PH2, PH, HCP) become increasingly important at high temperatures.

  16. Applications of the RELAP5 code to the station blackout transients at the Browns Ferry Unit One Plant

    SciTech Connect (OSTI)

    Schultz, R.R.; Wagoner, S.R.

    1983-01-01

    As a part of the charter of the Severe Accident Sequence Analysis (SASA) Program, station blackout transients have been analyzed using a RELAP5 model of the Browns Ferry Unit 1 Plant. The task was conducted as a partial fulfillment of the needs of the US Nuclear Regulatory Commission in examining the Unresolved Safety Issue A-44: Station Blackout (1) the station blackout transients were examined (a) to define the equipment needed to maintain a well cooled core, (b) to determine when core uncovery would occur given equipment failure, and (c) to characterize the behavior of the vessel thermal-hydraulics during the station blackout transients (in part as the plant operator would see it). These items are discussed in the paper. Conclusions and observations specific to the station blackout are presented.

  17. Young County, Texas: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page| Open Energy Information Serbia-EnhancingEtGeorgia:Illinois:WizardYates County, NewYorktown Heights, New York:Young

  18. Young Women's Conference in Science, Technology, Engineering & Mathematics

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home RoomPreservationBio-Inspired SolarAboutXu Named| Princeton Plasma Physics Lab Programs Young

  19. Sandia Energy - Sandian Selected for Outstanding Young Engineer Award

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power AdministrationRobust, High-Throughput AnalysisSinkhole OfficialsWork onand NaturalAppliedRecognized asYoung

  20. Generic relation between the electron work function and Young's modulus of metals

    SciTech Connect (OSTI)

    Hua Guomin; Li Dongyang [Department of Chemical and Materials Engineering, University of Alberta, Edmonton, Alberta T6G 2V4 (Canada)

    2011-07-25

    In this study, efforts were made to establish a generic relation between the Young's modulus and the electron work function of polycrystalline metals, in which Young's Modulus was defined as the second order derivative of interaction potential with respect to the equilibrium distance. The obtained Young's modulus shows a sextic relation with the work function. Data of Young's modulus and work function of polycrystalline metals, including Alkali earth metals, transition metals, and rare earth metals, can be fitted reasonably well by this derived generic relationship.

  1. iScreening Young Children for Lead Poisoning Foreword..........................................................................................v

    E-Print Network [OSTI]

    iScreening Young Children for Lead Poisoning Contents Foreword Advisory Committee on Childhood Lead Poisoning Prevention 1. Childhood Lead Poisoning in the United States

  2. Review of Research on Vulnerable Young people and Their Transitions to Independent Living 

    E-Print Network [OSTI]

    Elsley, Susan; Backett-Milburn, Kathryn; Jamieson, Lynn

    A research review focusing on young people who have been looked after at home and those who have been looked after and accommodated by Local Authorities.

  3. Review of Research on Vulnerable Young People and Their Transitions to Independent Living 

    E-Print Network [OSTI]

    Elsley, Susan; Backett-Milburn, Kathryn; Jamieson, Lynn

    A research review focusing on young people who have been looked after at home and those who have been looked after and accommodated by Local Authorities.

  4. Risky Business: Sex-work and Young Southeast Asian American Women in Oakland

    E-Print Network [OSTI]

    U, Nicol

    2008-01-01

    Press. ——— (b). 2001. Sex Crimes, Predators, Perpetrators,treat and “protect” young sex-workers as “victims”, how isfalling into the business of sex-work. References Bromberg,

  5. THE GEMINI/NICI PLANET-FINDING CAMPAIGN: THE FREQUENCY OF PLANETS AROUND YOUNG MOVING GROUP STARS

    SciTech Connect (OSTI)

    Biller, Beth A.; Ftaclas, Christ; Liu, Michael C.; Wahhaj, Zahed; Nielsen, Eric L.; Hayward, Thomas L.; Hartung, Markus; Chun, Mark; Clarke, Fraser; Thatte, Niranjan; Shkolnik, Evgenya L.; Reid, I. Neill; Boss, Alan; Lin, Douglas; Alencar, Silvia H. P.; De Gouveia Dal Pino, Elisabete; Gregorio-Hetem, Jane [Universidade de Sao Paulo, IAG and others

    2013-11-10

    We report results of a direct imaging survey for giant planets around 80 members of the ? Pic, TW Hya, Tucana-Horologium, AB Dor, and Hercules-Lyra moving groups, observed as part of the Gemini/NICI Planet-Finding Campaign. For this sample, we obtained median contrasts of ?H = 13.9 mag at 1'' in combined CH{sub 4} narrowband ADI+SDI mode and median contrasts of ?H = 15.1 mag at 2'' in H-band ADI mode. We found numerous (>70) candidate companions in our survey images. Some of these candidates were rejected as common-proper motion companions using archival data; we reobserved with Near-Infrared Coronagraphic Imager (NICI) all other candidates that lay within 400 AU of the star and were not in dense stellar fields. The vast majority of candidate companions were confirmed as background objects from archival observations and/or dedicated NICI Campaign followup. Four co-moving companions of brown dwarf or stellar mass were discovered in this moving group sample: PZ Tel B (36 ± 6 M{sub Jup}, 16.4 ± 1.0 AU), CD–35 2722B (31 ± 8 M{sub Jup}, 67 ± 4 AU), HD 12894B (0.46 ± 0.08 M{sub ?}, 15.7 ± 1.0 AU), and BD+07 1919C (0.20 ± 0.03 M{sub ?}, 12.5 ± 1.4 AU). From a Bayesian analysis of the achieved H band ADI and ASDI contrasts, using power-law models of planet distributions and hot-start evolutionary models, we restrict the frequency of 1-20 M{sub Jup} companions at semi-major axes from 10-150 AU to <18% at a 95.4% confidence level using DUSTY models and to <6% at a 95.4% using COND models. Our results strongly constrain the frequency of planets within semi-major axes of 50 AU as well. We restrict the frequency of 1-20 M{sub Jup} companions at semi-major axes from 10-50 AU to <21% at a 95.4% confidence level using DUSTY models and to <7% at a 95.4% using COND models. This survey is the deepest search to date for giant planets around young moving group stars.

  6. UV Radiation Fields Produced by Young Embedded Star Clusters

    E-Print Network [OSTI]

    M. Fatuzzo; F. C. Adams

    2007-12-20

    A large fraction of stars form within young embedded clusters, and these environments produce a substantial ultraviolet (UV) background radiation field, which can provide feedback on the star formation process. To assess the possible effects of young stellar clusters on the formation of their constituent stars and planets, this paper constructs the expected radiation fields produced by these clusters. We include both the observed distribution of cluster sizes $N$ in the solar neighborhood and an extended distribution that includes clusters with larger $N$. The paper presents distributions of the FUV and EUV luminosities for clusters with given stellar membership $N$, distributions of FUV and EUV luminosity convolved over the expected distribution of cluster sizes $N$, and the corresponding distributions of FUV and EUV fluxes. These flux distributions are calculated both with and without the effects of extinction. Finally, we consider the effects of variations in the stellar initial mass function on these radiation fields. Taken together, these results specify the distributions of radiation environments that forming solar systems are expected to experience.

  7. NEW YOUNG STAR CANDIDATES IN BRC 27 AND BRC 34

    SciTech Connect (OSTI)

    Rebull, L. M.; Laher, R.; Legassie, M.; Gibbs, J. C.; Aryal, S.; Canakapalli, T. S.; Linahan, M.; Ezyk, N.; Fagan, J.; Sartore, D.; Badura, K. S.; Armstrong, J. D.; Allen, L. E.; McGehee, P.; and others

    2013-01-01

    We used archival Spitzer Space Telescope mid-infrared data to search for young stellar objects (YSOs) in the immediate vicinity of two bright-rimmed clouds, BRC 27 (part of CMa R1) and BRC 34 (part of the IC 1396 complex). These regions both appear to be actively forming young stars, perhaps triggered by the proximate OB stars. In BRC 27, we find clear infrared excesses around 22 of the 26 YSOs or YSO candidates identified in the literature, and identify 16 new YSO candidates that appear to have IR excesses. In BRC 34, the one literature-identified YSO has an IR excess, and we suggest 13 new YSO candidates in this region, including a new Class I object. Considering the entire ensemble, both BRCs are likely of comparable ages, within the uncertainties of small number statistics and without spectroscopy to confirm or refute the YSO candidates. Similarly, no clear conclusions can yet be drawn about any possible age gradients that may be present across the BRCs.

  8. The young active star SAO 51891 (V383 Lac)

    E-Print Network [OSTI]

    Biazzo, Katia; Marilli, Ettore; Covino, Elvira; Alcala', Juan M; Cakirli, Omur; Klutsch, Alexis; Meyer, Michael R

    2009-01-01

    Our aim is investigating surface inhomogeneities of the young late-type star SAO51891, from photosphere to upper chromosphere, analyzing contemporaneous high-resolution spectra and broad-band photometry. The FOCES@CAHA spectral range is used to determine spectral classification and derive vsini and Vrad. The Li abundance is measured to estimate the age. The BVRIJHKs bands are used to construct the SED. The variations of our BV fluxes and Teff are used to infer the presence of photospheric spots and observe their behavior over time. The chromospheric activity is studied applying the spectral subtraction technique to Halpha, CaII H&K, Heps, and CaII IRT lines. We find SAO51891 to be a young K0-1V star with Li abundance close to the Pleiades upper envelope, confirming its youth (~100 Myr), also inferred from its kinematical membership to the Local Association. We detect no IR excess from SED analysis, and rotational modulation of luminosity, Teff, CaII, and Heps total fluxes. A spot model with two active reg...

  9. Ultracool Subdwarfs: Metal-poor Stars and Brown Dwarfs Extending into the Late-type M, L and T Dwarf Regimes

    E-Print Network [OSTI]

    Adam J. Burgasser; J. Davy Kirkpatrick; Sebastien Lepine

    2004-09-10

    Recent discoveries from red optical proper motion and wide-field near-infrared surveys have uncovered a new population of ultracool subdwarfs -- metal-poor stars and brown dwarfs extending into the late-type M, L and possibly T spectral classes. These objects are among the first low-mass stars and brown dwarfs formed in the Galaxy, and are valuable tracers of metallicity effects in low-temperature atmospheres. Here we review the spectral, photometric, and kinematic properties of recent discoveries. We also examine L subdwarf classification, and discuss how a large, complete sample of substellar halo subdwarfs could probe the star formation history of the Galaxy's Population II. We conclude by outlining a roadmap for future work to more thoroughly explore this old and very low-mass population.

  10. A review of "The Sale of the Century: Artistic Relations between Spain and Great Britain, 1604-1655." by Jonathan Brown and John Elliott, eds. 

    E-Print Network [OSTI]

    Elizabeth R. Wright

    2003-01-01

    Elliott, eds. The Sale of the Century: Ar- tistic Relations between Spain and Great Britain, 1604?1655. Madrid: Yale University Press and Museo Nacional del Prado, 2002. 315 pp. $65 hardback. Review by ELIZABETH R. WRIGHT, UNIVERSITY OF GEORGIA. Art... historian Jonathan Brown and historian John Elliott have joined forces to provide an indispensable guide to the political and artistic relationship between Spain and England in the first half of the seventeenth century. Though specifically focused...

  11. How this year's contest classes were placed BROWN SWISS A--First C--Second D--Third B--Fourth

    E-Print Network [OSTI]

    Hamza, Iqbal

    How this year's contest classes were placed BROWN SWISS A--First C--Second D--Third B--Fourth HOLSTEIN A--First B--Second D--Third C--Fourth D--First A--Second B--Third C--Fourth AYRSHIRE B--First D--Second C--Third A--Fourth JERSEY C--First A--Second B--Third D--Fourth OFFICIAL SCORING KEY FOR 2005 COW

  12. How this year's contest classes were placed BROWN SWISS A--First C--Second D--Third B--Fourth

    E-Print Network [OSTI]

    Hamza, Iqbal

    How this year's contest classes were placed BROWN SWISS A--First C--Second D--Third B--Fourth HOLSTEIN B--First A--Second D--Third C--Fourth B--First A--Second C--Third D--Fourth AYRSHIRE C--First B--Second A--Third D--Fourth JERSEY C--First D--Second B--Third A--Fourth OFFICIAL SCORING KEY FOR 2004 COW

  13. How this year's contest classes were placed BROWN SWISS D--First A--Second C--Third B--Fourth

    E-Print Network [OSTI]

    Hamza, Iqbal

    How this year's contest classes were placed BROWN SWISS D--First A--Second C--Third B--Fourth HOLSTEIN D--First C--Second A--Third B--Fourth D--First A--Second B--Third C--Fourth AYRSHIRE D--First C--Second B--Third A--Fourth JERSEY C--First A--Second D--Third B--Fourth OFFICIAL SCORING KEY FOR 2006 COW

  14. How this year's contest classes were placed BROWN SWISS C--First B--Second D--Third A--Fourth

    E-Print Network [OSTI]

    Hamza, Iqbal

    How this year's contest classes were placed BROWN SWISS C--First B--Second D--Third A--Fourth HOLSTEIN C--First D--Second A--Third B--Fourth B--First A--Second C--Third D--Fourth AYRSHIRE D--First B--Second C--Third A--Fourth JERSEY B--First D--Second A--Third C--Fourth OFFICIAL SCORING KEY FOR 2008 COW

  15. How this year's contest classes were placed BROWN SWISS B--First A--Second D--Third C--Fourth

    E-Print Network [OSTI]

    Hamza, Iqbal

    How this year's contest classes were placed BROWN SWISS B--First A--Second D--Third C--Fourth HOLSTEIN C--First A--Second B--Third D--Fourth D--First C--Second B--Third A--Fourth AYRSHIRE A--First C--Second B--Third D--Fourth JERSEY D--First C--Second B--Third A--Fourth OFFICIAL SCORING KEY FOR 2009 COW

  16. How this year's contest classes were placed BROWN SWISS D--First A--Second B--Third C--Fourth

    E-Print Network [OSTI]

    Hamza, Iqbal

    How this year's contest classes were placed BROWN SWISS D--First A--Second B--Third C--Fourth HOLSTEIN C--First A--Second D--Third B--Fourth A--First B--Second C--Third D--Fourth SHORTHORN B--First C--Second A--Third D--Fourth JERSEY D--First B--Second C--Third A--Fourth OFFICIAL SCORING KEY FOR 2007 COW

  17. Description of three ecology studies on brown shrimp Penaeus aztecus and white shrimp P. setiferus conducted by the National Marine Fisheries Service, Galveston, Texas 

    E-Print Network [OSTI]

    Diego, Maria Eugenia de

    1984-01-01

    Description of three ecology studies on brown shrimp Penaeus aztecus and white shrimp'P; setiferus conducted by the Mational Marine Fisheries Service, Galveston, Texas. A professional paper by Maria Eugenia de Diego Submitted to the College... shrimp Penaeus aztecus and white shrimp P, set1ferus conducted by the Nat1onal Marine F1sheries Ser- v1ce, Galveston, Texas. (December, 19843 Maria Eugenia de Diego, B. S. , Universidad de Panama Chairman of Adv1sory Committee: Dr. Addison L...

  18. PAUL SHORT --MENS BROWN file:///Users/bkatten/Desktop/R092812AF.html[9/28/12 4:04:11 PM

    E-Print Network [OSTI]

    Devoto, Stephen H.

    PAUL SHORT -- MENS BROWN file:///Users/bkatten/Desktop/R092812AF.html[9/28/12 4:04:11 PM] PAUL 163 183 191 27:03 1:28 22 Lafayette College 532 11 107 115 147 152 225 27:01 2:11 23 South Florida 564 file:///Users/bkatten/Desktop/R092812AF.html[9/28/12 4:04:11 PM] West Chester Universi 14 wins Vassar

  19. Introduction to low-momentum effective interactions with Brown-Rho scaling and three-nucleon forces

    E-Print Network [OSTI]

    Kuo, T T S; Osnes, E

    2015-01-01

    Model-space effective interactions $V_{eff}$ derived from free-space nucleon-nucleon interactions $V_{NN}$ are reviewed. We employ a double decimation approach: first we extract a low-momentum interaction $V_{low-k}$ from $V_{NN}$ using a $T$-matrix equivalence decimation method. Then $V_{eff}$ is obtained from $V_{low-k}$ by way of a folded-diagram effective interaction method. For decimation momentum $\\Lambda \\simeq 2 fm^{-1}$, the $V_{low-k}$ interactions derived from different realistic $V_{NN}$ models are nearly model independent, and so are the resulting shell-model effective interactions. For nucleons in a low-density nuclear medium like valence nucleons near the nuclear surface, such effective interactions derived from free-space $V_{NN}$ are satisfactory in reproducing experimental nuclear properties. But it is not so for nucleons in a nuclear medium with density near or beyond nuclear matter saturation density. In this case it may be necessary to include the effects from Brown-Rho (BR) scaling of ha...

  20. PII S0016-7037(98)00211-7 The young age of Earth

    E-Print Network [OSTI]

    Zhang, Youxue

    PII S0016-7037(98)00211-7 The young age of Earth YOUXUE ZHANG* Department of Geological Sciences form June 8, 1998) Abstract--Patterson (1956) established that the age of Earth is close, disagreement is abundant, and the young age of Earth has not been widely accepted. In this work, I examine all

  1. Course Profile: Programming and Services for Children and Young Adults Course Number: LIS 7250

    E-Print Network [OSTI]

    Berdichevsky, Victor

    Course Profile: Programming and Services for Children and Young Adults Course Number: LIS 7250 with children and young adults in public libraries there is a need for skill in the development of programming adults. Course Objectives: To provide an understanding of age-specific services, program planning

  2. SYNTHETIC SPECTRA AND COLORS OF YOUNG GIANT PLANET ATMOSPHERES: EFFECTS OF INITIAL CONDITIONS AND ATMOSPHERIC METALLICITY

    E-Print Network [OSTI]

    , as giant planets should be warmest, largest, and brightest when they are young, but will cool, contractSYNTHETIC SPECTRA AND COLORS OF YOUNG GIANT PLANET ATMOSPHERES: EFFECTS OF INITIAL CONDITIONS 2008 March 17; accepted 2008 May 7 ABSTRACT We examine the spectra and infrared colors of the cool

  3. Skin Cancer: A Young Person's Disease By Lauren Duffy (B.S. Communication, Journalism '14)

    E-Print Network [OSTI]

    Massachusetts at Amherst, University of

    Skin Cancer: A Young Person's Disease By Lauren Duffy (B.S. Communication, Journalism '14 is that this behavior is extremely unhealthy and risky for their bodies, specifically their skin. Skin cancer is the most common form of cancer found in young adults and second most common cancer found in adolescents

  4. Brigham Young University Geology Studies Volume 23, Part 3-October 1976

    E-Print Network [OSTI]

    Seamons, Kent E.

    #12;Brigham Young University Geology Studies Volume 23, Part 3-October 1976 Contents A Well ........................................................ E. Blair Maxfield 67 Publications and Maps of the Geology Department ............................ 163 #12;A publication of the Department of Geology Brigham Young University Provo, Utah 84602 Edltor W

  5. Town of Dallas, North Carolina (Utility Company) | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page| Open Energy Information Serbia-EnhancingEt Al., 2013)OpenEnergy Facilities Biomass FacilityTown ofTown ofNorth

  6. KaushikRajashekara TheUniversityofTexasatDallas

    E-Print Network [OSTI]

    California at Davis, University of

    of a EV Power-train 13 14 #12;15 Vehicle range per battery charge under various driving conditions Fuel/DOETargets Batteries ElectricMachines PowerElectronics Futurepowertrains Conclusions 2 #12;GeneralMotorsEV1 * Engine: 1.3 liter, 4 cylinder * Battery: 100.8V DC (NiMH battery), 5.75 Ah * Motor/Generator: 13 KW @1500

  7. Continuous Commissioning® of the Dallas/Fort Worth International Airport 

    E-Print Network [OSTI]

    Yazdani, B.; Schroeder, F.; Kramer, L.; Baltazar, J. C.; Turner, W. D.; Wei, G.; Deng, S.; Henson, R.; Dennis, J. R.; T., R.

    2008-01-01

    savings from the CC work. The savings are approximately $60,000 (?40,000) for nine months. Projected 12-month savings are $80,000 (?53,000), representing a savings of approximately $1 per square foot per year (?6.2/m 2 per year). There are still... load causes this building to ?peak? at night. The savings from the CC process are in excess of 18% of the total building energy consumption, including lighting. The dollar savings amounted to about $0.80 per ft2 or ?5.50 per m2). DFW...

  8. Timothy E John Dallas Department of Electrical and Computer Engineering

    E-Print Network [OSTI]

    Gelfond, Michael

    . of Microelectromechanical Systems 19, pp. 632-639 (2010). 9. "Design and Analysis of a Dual-Mode MEMS Micromirror," X. Xiong (Accepted, Journal of Electrostatics, 7/2012). 2. "The 18mm 2 Laboratory: Teaching MEMS Development-micromachined MEMS," Ashwin P. Vijayasai, Ganapathy Sivakumar, Matthew Mulsow, Shelby Lacouture, Alex Holness

  9. Official Approved Minutes UT DALLAS STAFF COUNCIL MEETING MINUTES

    E-Print Network [OSTI]

    O'Toole, Alice J.

    (resigned,) Linda Heard, Lin Maute, Tracey Tatum, Rikk Terhune, Rhonda Walls GUESTS: Chief Larry Zacharias

  10. Official Approved Minutes UT DALLAS STAFF COUNCIL MEETING MINUTES

    E-Print Network [OSTI]

    O'Toole, Alice J.

    Holt, Lin Maute, Jayar Howard Medlock, Mike Mogg, Wendy Newton, Rochelle Peña, Sheila Rollerson, Deann

  11. HASE'07 Panel 4a Dallas, TX Achieving High Assurance

    E-Print Network [OSTI]

    Tian, Jeff

    . Ishikawa's fishbone diagrams. FTA: Fault tree analysis. ETA: Event tree analysis. FMEA: Failure mode

  12. SMU, Dept of Electrical Engineering Dallas, Texas 75275

    E-Print Network [OSTI]

    Chen, Thomas M.

    on surfing habits Hijacks Web searches and IE settings Tricks user by claiming to delete porn Bundled

  13. 01 Gennaio 2010 Agile scopre emissione gamma dalla nebulosa

    E-Print Network [OSTI]

    partecipazione dell'Istituto Nazionale di Astrofisica (INAF) e dell'Istituto Nazionale di Fisica Nucleare (INFN ad altissima energia. Questa scoperta ci consentirà di modellare i processi che presiedono, in questa

  14. Alternative Fuels Data Center: Dallas Airport Operates With Alternative

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 OutreachProductswsicloudwsiclouddenDVA N C E D B L O O D S TA I NLoans TheCountyCitiesDriving FutureFuels

  15. Alternative Fuels Data Center: Dallas Police Department Reduces Vehicle

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 OutreachProductswsicloudwsiclouddenDVA N C E D B L O O D S TA I NLoans TheCountyCitiesDriving

  16. Dallas County, Alabama: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTIONRobertsdale, Alabama (UtilityInstruments Inc Jump to:67-2006-12DabbrookAssociationDalianAlabama:

  17. Dallas County, Arkansas: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTIONRobertsdale, Alabama (UtilityInstruments Inc Jump

  18. Dallas County, Iowa: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTIONRobertsdale, Alabama (UtilityInstruments Inc JumpIowa: Energy Resources Jump to: navigation, search

  19. Dallas County, Missouri: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTIONRobertsdale, Alabama (UtilityInstruments Inc JumpIowa: Energy Resources Jump to: navigation,

  20. Dallas: Building a Greener City | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of Natural GasAdjustmentsShirleyEnergy A plug-in electricLaboratory | version of the1996of EnergyIdahoS . DandThanks to the

  1. Lake Dallas, Texas: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsource History ViewInformation Actions(RedirectedLouisiana: Energy ResourcesIDallas,

  2. Dallas County, Texas: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX ECoopButtePower VenturesInformation9) WindGrid Project) | OpenCoop IncTexas: Energy

  3. City of Dallas - Green Building Policy for Municipal Buildings | Department

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of Natural GasAdjustmentsShirleyEnergyTher i n c i p a lCaribElectricSouthApplying2-2002Joshua<Department<<of

  4. City of Dallas - Residential and Commercial Green Building Requirements |

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of Natural GasAdjustmentsShirleyEnergyTher i n c i p a

  5. The young stellar population in M17 revealed by Chandra

    E-Print Network [OSTI]

    Patrick S. Broos; Eric D. Feigelson; Leisa K. Townsley; Konstantin V. Getman; Junfeng Wang; Gordon P. Garmire; Zhibo Jiang; Yohko Tsuboi

    2006-12-20

    We report here results from a Chandra ACIS observation of the stellar populations in and around the Messier 17 H II region. The field reveals 886 sources, 771 of which have stellar counterparts in infrared images. In addition to comprehensive tables of X-ray source properties, several results are presented: * The X-ray Luminosity Function is calibrated to that of the Orion Nebula Cluster population to infer a total population of roughly 8000--10,000 stars * About 40% of the ACIS sources are heavily obscured with A_V > 10 mag. Some are concentrated around well-studied star-forming regions but most are distributed across the field. X-ray emission is detected from 64 of the hundreds of Class I protostar candidates that can be identified by near- and mid-infrared colors. These constitute the most likely protostar candidates known in M17. * The spatial distribution of X-ray stars is complex: we find a new embedded cluster, a 2 pc-long arc of young stars along the southwest edge of the M17 H II region, and 0.1 pc substructure within various populations. These structures may indicate that the populations are dynamically young. * All (14/14) of the known O stars but only about half (19/34) of the known B0--B3 stars in the M17 field are detected. Six of these stars exhibit very hard thermal plasma components (kT>4 keV) that may be due to colliding wind binaries. More than 100 candidate new OB stars are found, including 28 X-ray detected intermediate- and high-mass protostar candidates with infrared excesses. * Only a small fraction (perhaps 10%) of X-ray selected high- and intermediate- mass stars exhibit K-band emitting protoplanetary disks, providing further evidence that inner disks evolve very rapidly around more massive stars.

  6. International Workshop of Young Doctors in Geomechanics -W(H)YDOC 08 Pereira, De Gennaro & Delage (eds) 2008, Ecole des Ponts ParisTech, Champs-sur-Marne

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    3 rd International Workshop of Young Doctors in Geomechanics - W(H)YDOC 08 Pereira, De Gennaro of young doctors in geomechanics,

  7. International Workshop of Young Doctors in Geomechanics -W(H)YDOC 08 Pereira, De Gennaro & Delage (eds) 2008, Ecole des Ponts ParisTech, Champs-sur-Marne

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    3 rd International Workshop of Young Doctors in Geomechanics - W(H)YDOC 08 Pereira, De Gennaro of young doctors in geomechanics

  8. Presented by the UT Dallas Career Center UT Dallas Fall Career Expo Days STEM Day | Friday, Sept. 26, 2014

    E-Print Network [OSTI]

    O'Toole, Alice J.

    , SAP, & Cyber Security Computer Engineering, Computer Science, Software Engineering, Systems, Software Engineering, Systems Engineering and Management, MIS, ITM Bachelors, Masters Full-time, Interns Bachelors Full-time Unable to consider Availity Developer, Product Owner, Scrum Master, Project Manager All

  9. Young's modulus of electroplated Ni thin film for MEMS applications J.K. Luoa,*, A.J. Flewitta

    E-Print Network [OSTI]

    Fleck, Norman A.

    to a less dense coating. D 2004 Elsevier B.V. All rights reserved. Keywords: Young's modulus; ElectroplatedYoung's modulus of electroplated Ni thin film for MEMS applications J.K. Luoa,*, A.J. Flewitta , S online 28 April 2004 Abstract The Young's modulus of an electroplated nickel (Ni) thin film suitable

  10. Effect of Solar Radiation on the Optical Properties and Molecular Composition of Laboratory Proxies of Atmospheric Brown Carbon

    SciTech Connect (OSTI)

    Lee, Hyun Ji; Aiona, Paige K.; Laskin, Alexander; Laskin, Julia; Nizkorodov, Sergey

    2014-09-02

    Sources, optical properties, and chemical composition of atmospheric brown carbon (BrC) aerosol are uncertain, making it challenging to estimate its contribution to radiative forcing. Furthermore, optical properties of BrC may change significantly during its atmospheric aging. We examined the effect of solar photolysis on the molecular composition, mass absorption coefficient, and fluorescence of secondary organic aerosol prepared by high-NOx photooxidation of naphthalene (NAP SOA). The aqueous solutions of NAP SOA was observed to photobleach with an effective half-time of ?15 hours (with sun in its zenith) for the loss of the near-UV (300 -400 nm) absorbance. The molecular composition of NAP SOA was significantly modified by photolysis, with the average SOA formula changing from C14.1H14.5O5.1N0.08 to C11.8H14.9O4.5N0.02 after 4 hours of irradiation. The average O/C ratio did not change significantly, however, suggesting that it is not a good metric for assessing the extent of photolysis-driven aging in NAP SOA (and in BrC in general). In contrast to NAP SOA, the photolysis of BrC material produced by aqueous reaction of limonene+O3 SOA (LIM/O3 SOA) with ammonium sulfate was much faster, but it did not result in a significant change in the molecular level composition. The characteristic absorbance of the aged LIM/O3 SOA in the 450-600 nm range decayed with an effective half-time of <0.5 hour. This result emphasizes the highly variable and dynamic nature of different types of atmospheric BrC.

  11. Characterization of novel sorghum brown midrib mutants from an EMS-mutagenized population

    SciTech Connect (OSTI)

    Sattler, Scott E.; Saballos, Ana; Xin, Zhanguo; Funnell-Harris, Deanna L.; Vermerris, Wilfred; Pedersen, Jeffrey F.

    2014-09-02

    Reducing lignin concentration in lignocellulosic biomass can increase forage digestibility for ruminant livestock and saccharification yields of biomass for bioenergy. In sorghum (Sorghum bicolor (L.) Moench) and several other C4 grasses, brown midrib (bmr) mutants have been shown to reduce lignin concentration. Putative bmr mutants isolated from an EMS-mutagenized population were characterized and classified based on their leaf midrib phenotype and allelism tests with the previously described sorghum bmr mutants bmr2, bmr6, and bmr12. These tests resulted in the identification of additional alleles of bmr2, bmr6,and bmr12, and, in addition, six bmr mutants were identified that were not allelic to these previously described loci. Further allelism testing among these six bmr mutants showed that they represented four novel bmr loci. Based on this study, the number of bmr loci uncovered in sorghum has doubled. The impact of these lines on agronomic traits and lignocellulosic composition was assessed in a 2-yr field study. Most of the identified bmr lines showed reduced lignin concentration of their biomass relative to wild-type (WT). Effects of the six new bmr mutants on enzymatic saccharification of lignocellulosic materials were determined, but the amount of glucose released from the stover was similar to WT in all cases. Like bmr2, bmr6, and bmr12, these mutants may affect monolignol biosynthesis and may be useful for bioenergy and forage improvement when stacked together or in combination with the three previously described bmr alleles.

  12. Possible contribution of low shear modulus C?? to the low Young’s modulus of Ti-36Nb-5Zr alloy

    SciTech Connect (OSTI)

    Meng, Qingkun; Guo, Shun; Ren, Xiaobing; Xu, Huibin; Zhao, Xinqing

    2014-09-29

    Despite the importance of single-crystal elastic constants of ?-phase titanium alloys in understanding their low Young's modulus—a property crucial for many applications, such data are often difficult to obtain when the alloy composition is close to the instability limit of the ? phase, where the presence of ?" martensite precludes the fabrication of ?-phase single crystal. In the present study, we extracted the single-crystal elastic constants of such a ?-phase titanium alloy with low Young's modulus, Ti-36Nb-5Zr (wt. %), from polycrystalline specimens by using an in-situ synchrotron X-ray diffraction technique. It is indicated that the low Young's modulus of the alloy originates from the anomalously low shear modulus C?? as well as the low shear modulus C', which is different from a common viewpoint that the Young's modulus of ?-phase titanium alloys is dominantly controlled by the C'. This suggests that low C?? is an important contributor to low Young's modulus for instable ?-phase titanium alloys.

  13. Three new cool brown dwarfs discovered with the wide-field infrared survey explorer (WISE) and an improved spectrum of the Y0 dwarf wise J041022.71+150248.4

    SciTech Connect (OSTI)

    Cushing, Michael C.; Kirkpatrick, J. Davy; Gelino, Christopher R.; Mace, Gregory N.; Skrutskie, Michael F.; Gould, Andrew

    2014-05-01

    As part of a larger search of Wide-field Infrared Survey Explorer (WISE) data for cool brown dwarfs with effective temperatures less than 1000 K, we present the discovery of three new cool brown dwarfs with spectral types later than T7. Using low-resolution, near-infrared spectra obtained with the NASA Infrared Telescope Facility and the Hubble Space Telescope, we derive spectral types of T9.5 for WISE J094305.98+360723.5, T8 for WISE J200050.19+362950.1, and Y0: for WISE J220905.73+271143.9. The identification of WISE J220905.73+271143.9 as a Y dwarf brings the total number of spectroscopically confirmed Y dwarfs to 17. In addition, we present an improved spectrum (i.e., higher signal-to-noise ratio) of the Y0 dwarf WISE J041022.71+150248.4 that confirms the Cushing et al. classification of Y0. Spectrophotometric distance estimates place all three new brown dwarfs at distances less than 12 pc, with WISE J200050.19+362950.1 lying at a distance of only 3.9-8.0 pc. Finally, we note that brown dwarfs like WISE J200050.19+362950.1 that lie in or near the Galactic plane offer an exciting opportunity to directly measure the mass of a brown dwarf via astrometric microlensing.

  14. Enhanced hydrolysis and methane yield by applying microaeration pretreatment to the anaerobic co-digestion of brown water and food waste

    SciTech Connect (OSTI)

    Lim, Jun Wei; Wang, Jing-Yuan

    2013-04-15

    Highlights: ? Microaeration pretreatment was effective for brown water and food waste mixture. ? The added oxygen was consumed fully by facultative microorganisms. ? Enhanced solubilization, acidification and breakdown of SCFAs to acetate. ? Microaeration pretreatment improved methane yield by 10–21%. ? Nature of inoculum influenced the effects of microaeration. - Abstract: Microaeration has been used conventionally for the desulphurization of biogas, and recently it was shown to be an alternative pretreatment to enhance hydrolysis of the anaerobic digestion (AD) process. Previous studies on microaeration pretreatment were limited to the study of substrates with complex organic matter, while little has been reported on its effect on substrates with higher biodegradability such as brown water and food waste. Due to the lack of consistent microaeration intensities, previous studies were not comparable and thus inconclusive in proving the effectiveness of microaeration to the overall AD process. In this study, the role of microaeration pretreatment in the anaerobic co-digestion of brown water and food waste was evaluated in batch-tests. After a 4-day pretreatment with 37.5 mL-O{sub 2}/L{sub R}-d added to the liquid phase of the reactor, the methane production of substrates were monitored in anaerobic conditions over the next 40 days. The added oxygen was consumed fully by facultative microorganisms and a reducing environment for organic matter degradation was maintained. Other than higher COD solubilization, microaeration pretreatment led to greater VFA accumulation and the conversion of other short chain fatty acids to acetate. This could be due to enhanced activities of hydrolytic and acidogenic bacteria and the degradation of slowly biodegradable compounds under microaerobic conditions. This study also found that the nature of inoculum influenced the effects of microaeration as a 21% and 10% increase in methane yield was observed when pretreatment was applied to inoculated substrates, and substrates without inoculum, respectively.

  15. Searches for continuous gravitational waves from nine young supernova remnants

    E-Print Network [OSTI]

    Aasi, J; Abbott, R; Abbott, T; Abernathy, M R; Acernese, F; Ackley, K; Adams, C; Adams, T; Addesso, P; Adhikari, R X; Adya, V; Affeldt, C; Agathos, M; Agatsuma, K; Aggarwal, N; Aguiar, O D; Ain, A; Ajith, P; Alemic, A; Allen, B; Allocca, A; Amariutei, D; Anderson, S B; Anderson, W G; Arai, K; Araya, M C; Arceneaux, C; Areeda, J S; Ast, S; Aston, S M; Astone, P; Aufmuth, P; Aulbert, C; Aylott, B E; Babak, S; Baker, P T; Baldaccini, F; Ballardin, G; Ballmer, S W; Barayoga, J C; Barbet, M; Barclay, S; Barish, B C; Barker, D; Barone, F; Barr, B; Barsotti, L; Barsuglia, M; Bartlett, J; Barton, M A; Bartos, I; Bassiri, R; Basti, A; Batch, J C; Bauer, Th S; Baune, C; Bavigadda, V; Behnke, B; Bejger, M; Belczynski, C; Bell, A S; Bell, C; Benacquista, M; Bergman, J; Bergmann, G; Berry, C P L; Bersanetti, D; Bertolini, A; Betzwieser, J; Bhagwat, S; Bhandare, R; Bilenko, I A; Billingsley, G; Birch, J; Biscans, S; Bitossi, M; Biwer, C; Bizouard, M A; Blackburn, J K; Blackburn, L; Blair, C D; Blair, D; Bloemen, S; Bock, O; Bodiya, T P; Boer, M; Bogaert, G; Bojtos, P; Bond, C; Bondu, F; Bonelli, L; Bonnand, R; Bork, R; Born, M; Boschi, V; Bose, Sukanta; Bradaschia, C; Brady, P R; Braginsky, V B; Branchesi, M; Brau, J E; Briant, T; Bridges, D O; Brillet, A; Brinkmann, M; Brisson, V; Brooks, A F; Brown, D A; Brown, D D; Brown, N M; Buchman, S; Buikema, A; Bulik, T; Bulten, H J; Buonanno, A; Buskulic, D; Buy, C; Cadonati, L; Cagnoli, G; Bustillo, J Calderón; Calloni, E; Camp, J B; Cannon, K C; Cao, J; Capano, C D; Carbognani, F; Caride, S; Caudill, S; Cavaglià, M; Cavalier, F; Cavalieri, R; Cella, G; Cepeda, C; Cesarini, E; Chakraborty, R; Chalermsongsak, T; Chamberlin, S J; Chao, S; Charlton, P; Chassande-Mottin, E; Chen, Y; Chincarini, A; Chiummo, A; Cho, H S; Cho, M; Chow, J H; Christensen, N; Chu, Q; Chua, S; Chung, S; Ciani, G; Clara, F; Clark, J A; Cleva, F; Coccia, E; Cohadon, P -F; Colla, A; Collette, C; Colombini, M; Cominsky, L; Constancio,, M; Conte, A; Cook, D; Corbitt, T R; Cornish, N; Corsi, A; Costa, C A; Coughlin, M W; Coulon, J -P; Countryman, S; Couvares, P; Coward, D M; Cowart, M J; Coyne, D C; Coyne, R; Craig, K; Creighton, J D E; Creighton, T D; Cripe, J; Crowder, S G; Cumming, A; Cunningham, L; Cuoco, E; Cutler, C; Dahl, K; Canton, T Dal; Damjanic, M; Danilishin, S L; D'Antonio, S; Danzmann, K; Dartez, L; Dattilo, V; Dave, I; Daveloza, H; Davier, M; Davies, G S; Daw, E J; Day, R; DeBra, D; Debreczeni, G; Degallaix, J; De Laurentis, M; Deléglise, S; Del Pozzo, W; Denker, T; Dent, T; Dereli, H; Dergachev, V; De Rosa, R; DeRosa, R T; DeSalvo, R; Dhurandhar, S; Díaz, M; Di Fiore, L; Di Lieto, A; Di Palma, I; Di Virgilio, A; Dojcinoski, G; Dolique, V; Dominguez, E; Donovan, F; Dooley, K L; Doravari, S; Douglas, R; Downes, T P; Drago, M; Driggers, J C; Du, Z; Ducrot, M; Dwyer, S; Eberle, T; Edo, T; Edwards, M; Effler, A; Eggenstein, H -B; Ehrens, P; Eichholz, J; Eikenberry, S S; Essick, R; Etzel, T; Evans, M; Evans, T; Factourovich, M; Fafone, V; Fairhurst, S; Fan, X; Fang, Q; Farinon, S; Farr, B; Farr, W M; Favata, M; Fays, M; Fehrmann, H; Fejer, M M; Feldbaum, D; Ferrante, I; Ferreira, E C; Ferrini, F; Fidecaro, F; Fiori, I; Fisher, R P; Flaminio, R; Fournier, J -D; Franco, S; Frasca, S; Frasconi, F; Frei, Z; Freise, A; Frey, R; Fricke, T T; Fritschel, P; Frolov, V V; Fuentes-Tapia, S; Fulda, P; Fyffe, M; Gair, J R; Gammaitoni, L; Gaonkar, S; Garufi, F; Gatto, A; Gehrels, N; Gemme, G; Gendre, B; Genin, E; Gennai, A; Gergely, L Á; Ghosh, S; Giaime, J A; Giardina, K D; Giazotto, A; Gleason, J; Goetz, E; Goetz, R; Gondan, L; González, G; Gordon, N; Gorodetsky, M L; Gossan, S; Goßler, S; Gouaty, R; Gräf, C; Graff, P B; Granata, M; Grant, A; Gras, S; Gray, C; Greenhalgh, R J S; Gretarsson, A M; Groot, P; Grote, H; Grunewald, S; Guidi, G M; Guido, C J; Guo, X; Gushwa, K; Gustafson, E K; Gustafson, R; Hacker, J; Hall, E D; Hammond, G; Hanke, M; Hanks, J; Hanna, C; Hannam, M D; Hanson, J; Hardwick, T; Harms, J; Harry, G M; Harry, I W; Hart, M; Hartman, M T; Haster, C -J; Haughian, K; Hee, S; Heidmann, A; Heintze, M; Heinzel, G; Heitmann, H; Hello, P; Hemming, G; Hendry, M; Heng, I S; Heptonstall, A W; Heurs, M; Hewitson, M; Hild, S; Hoak, D; Hodge, K A; Hofman, D; Hollitt, S E; Holt, K; Hopkins, P; Hosken, D J; Hough, J; Houston, E; Howell, E J; Hu, Y M; Huerta, E; Hughey, B; Husa, S; Huttner, S H; Huynh, M; Huynh-Dinh, T; Idrisy, A; Indik, N; Ingram, D R; Inta, R; Islas, G; Isler, J C; Isogai, T; Iyer, B R; Izumi, K; Jacobson, M; Jang, H; Jaranowski, P; Jawahar, S; Ji, Y; Jiménez-Forteza, F; Johnson, W W; Jones, D I; Jones, R; Jonker, R J G; Ju, L; K, Haris; Kalogera, V; Kandhasamy, S; Kang, G; Kanner, J B; Kasprzack, M; Katsavounidis, E; Katzman, W; Kaufer, H; Kaufer, S; Kaur, T; Kawabe, K; Kawazoe, F; Kéfélian, F; Keiser, G M; Keitel, D; Kelley, D B; Kells, W; Keppel, D G; Key, J S; Khalaidovski, A

    2014-01-01

    We describe directed searches for continuous gravitational waves in data from the sixth LIGO science data run. The targets were nine young supernova remnants not associated with pulsars; eight of the remnants are associated with non-pulsing suspected neutron stars. One target's parameters are uncertain enough to warrant two searches, for a total of ten. Each search covered a broad band of frequencies and first and second frequency derivatives for a fixed sky direction. The searches coherently integrated data from the two LIGO interferometers over time spans from 5.3-25.3 days using the matched-filtering F-statistic. We found no credible gravitational-wave signals. We set 95% confidence upper limits as strong (low) as $4\\times10^{-25}$ on intrinsic strain, $2\\times10^{-7}$ on fiducial ellipticity, and $4\\times10^{-5}$ on r-mode amplitude. These beat the indirect limits from energy conservation and are within the range of theoretical predictions for neutron-star ellipticities and r-mode amplitudes.

  16. Photon Bubbles in the Circumstellar Envelopes of Young Massive Stars

    E-Print Network [OSTI]

    N. J. Turner; E. Quataert; H. W. Yorke

    2007-01-28

    We show that the optically-thick dusty envelopes surrounding young high-mass stars are subject to the photon bubble instability. The infrared radiation passing through the envelope amplifies magnetosonic disturbances, with growth rates in our local numerical radiation MHD calculations that are consistent with a linear analysis. Modes with wavelengths comparable to the gas pressure scale height grow by more than two orders of magnitude in a thousand years, reaching non-linear amplitudes within the envelope lifetime. If the magnetic pressure in the envelope exceeds the gas pressure, the instability develops into trains of propagating shocks. Radiation escapes readily through the low-density material between the shocks, enabling accretion to continue despite the Eddington limit imposed by the dust opacity. The supersonic motions arising from the photon bubble instability can help explain the large velocity dispersions of hot molecular cores, while conditions in the shocked gas are suitable for maser emission. We conclude that the photon bubble instability may play a key role in the formation of massive stars.

  17. Do you know the extinction in your young massive cluster?

    E-Print Network [OSTI]

    De Marchi, Guido; Sabbi, Elena

    2015-01-01

    Up to ages of ~100 Myr, massive clusters are still swamped in large amounts of gas and dust, with considerable and uneven levels of extinction. At the same time, large grains (ices?) produced by type II supernovae profoundly alter the interstellar medium (ISM), thus resulting in extinction properties very different from those of the diffuse ISM. To obtain physically meaningful parameters of stars, from basic luminosities and effective temperatures to masses and ages, we must understand and measure the local extinction law. This problem affects all the massive young clusters discussed in his volume. We have developed a powerful method to unambiguously determine the extinction law in an uniform way across a cluster field, using multi-band photometry of red giant stars belonging to the red clump (RC). In the Large Magellanic Cloud, with about 20 RC stars per arcmin^2, we can easily derive a solid and self-consistent absolute extinction curve over the entire wavelength range of the photometry. Here, we present th...

  18. Lyman-break galaxies are they young spheroids?

    E-Print Network [OSTI]

    Matteucci, F

    2002-01-01

    We have compared the results from a model for the chemical evolution of an elliptical galaxy with initial luminous mass of 2x10^10 M_sun and effective radius of 2 kpc with the recent abundance determinations for the Lyman-break galaxy MS 1512-cB58 at a redshift z=2.7276. After correcting the iron abundance determination for the presence of dust we concluded that the observed [Si/Fe], [Mg/Fe], [N/Fe] are consistent with our model when a galactic age between 20 and 35 Myr is assumed. Moreover, the [N/O] ratio also suggests the same age. This age is in very good agreement with other independent studies based on the analysis of the spectral energy distribution suggesting that this object is younger than 35 Myr. Therefore, we suggest that MS 1512-cB58 is a truly young normal elliptical galaxy experiencing its main episode of star formation and galactic wind.

  19. Searches for continuous gravitational waves from nine young supernova remnants

    E-Print Network [OSTI]

    J. Aasi; B. P. Abbott; R. Abbott; T. Abbott; M. R. Abernathy; F. Acernese; K. Ackley; C. Adams; T. Adams; T. Adams; P. Addesso; R. X. Adhikari; V. Adya; C. Affeldt; M. Agathos; K. Agatsuma; N. Aggarwal; O. D. Aguiar; A. Ain; P. Ajith; A. Alemic; B. Allen; A. Allocca; D. Amariutei; S. B. Anderson; W. G. Anderson; K. Arai; M. C. Araya; C. Arceneaux; J. S. Areeda; S. Ast; S. M. Aston; P. Astone; P. Aufmuth; C. Aulbert; B. E. Aylott; S. Babak; P. T. Baker; F. Baldaccini; G. Ballardin; S. W. Ballmer; J. C. Barayoga; M. Barbet; S. Barclay; B. C. Barish; D. Barker; F. Barone; B. Barr; L. Barsotti; M. Barsuglia; J. Bartlett; M. A. Barton; I. Bartos; R. Bassiri; A. Basti; J. C. Batch; Th. S. Bauer; C. Baune; V. Bavigadda; B. Behnke; M. Bejger; C. Belczynski; A. S. Bell; C. Bell; M. Benacquista; J. Bergman; G. Bergmann; C. P. L. Berry; D. Bersanetti; A. Bertolini; J. Betzwieser; S. Bhagwat; R. Bhandare; I. A. Bilenko; G. Billingsley; J. Birch; S. Biscans; M. Bitossi; C. Biwer; M. A. Bizouard; J. K. Blackburn; L. Blackburn; C. D. Blair; D. Blair; S. Bloemen; O. Bock; T. P. Bodiya; M. Boer; G. Bogaert; P. Bojtos; C. Bond; F. Bondu; L. Bonelli; R. Bonnand; R. Bork; M. Born; V. Boschi; Sukanta Bose; C. Bradaschia; P. R. Brady; V. B. Braginsky; M. Branchesi; J. E. Brau; T. Briant; D. O. Bridges; A. Brillet; M. Brinkmann; V. Brisson; A. F. Brooks; D. A. Brown; D. D. Brown; N. M. Brown; S. Buchman; A. Buikema; T. Bulik; H. J. Bulten; A. Buonanno; D. Buskulic; C. Buy; L. Cadonati; G. Cagnoli; J. Calderón Bustillo; E. Calloni; J. B. Camp; K. C. Cannon; J. Cao; C. D. Capano; F. Carbognani; S. Caride; S. Caudill; M. Cavaglià; F. Cavalier; R. Cavalieri; G. Cella; C. Cepeda; E. Cesarini; R. Chakraborty; T. Chalermsongsak; S. J. Chamberlin; S. Chao; P. Charlton; E. Chassande-Mottin; Y. Chen; A. Chincarini; A. Chiummo; H. S. Cho; M. Cho; J. H. Chow; N. Christensen; Q. Chu; S. Chua; S. Chung; G. Ciani; F. Clara; J. A. Clark; F. Cleva; E. Coccia; P. -F. Cohadon; A. Colla; C. Collette; M. Colombini; L. Cominsky; M. Constancio, Jr.; A. Conte; D. Cook; T. R. Corbitt; N. Cornish; A. Corsi; C. A. Costa; M. W. Coughlin; J. -P. Coulon; S. Countryman; P. Couvares; D. M. Coward; M. J. Cowart; D. C. Coyne; R. Coyne; K. Craig; J. D. E. Creighton; T. D. Creighton; J. Cripe; S. G. Crowder; A. Cumming; L. Cunningham; E. Cuoco; C. Cutler; K. Dahl; T. Dal Canton; M. Damjanic; S. L. Danilishin; S. D'Antonio; K. Danzmann; L. Dartez; V. Dattilo; I. Dave; H. Daveloza; M. Davier; G. S. Davies; E. J. Daw; R. Day; D. DeBra; G. Debreczeni; J. Degallaix; M. De Laurentis; S. Deléglise; W. Del Pozzo; T. Denker; T. Dent; H. Dereli; V. Dergachev; R. De Rosa; R. T. DeRosa; R. DeSalvo; S. Dhurandhar; M. Díaz; L. Di Fiore; A. Di Lieto; I. Di Palma; A. Di Virgilio; G. Dojcinoski; V. Dolique; E. Dominguez; F. Donovan; K. L. Dooley; S. Doravari; R. Douglas; T. P. Downes; M. Drago; J. C. Driggers; Z. Du; M. Ducrot; S. Dwyer; T. Eberle; T. Edo; M. Edwards; M. Edwards; A. Effler; H. -B. Eggenstein; P. Ehrens; J. Eichholz; S. S. Eikenberry; R. Essick; T. Etzel; M. Evans; T. Evans; M. Factourovich; V. Fafone; S. Fairhurst; X. Fan; Q. Fang; S. Farinon; B. Farr; W. M. Farr; M. Favata; M. Fays; H. Fehrmann; M. M. Fejer; D. Feldbaum; I. Ferrante; E. C. Ferreira; F. Ferrini; F. Fidecaro; I. Fiori; R. P. Fisher; R. Flaminio; J. -D. Fournier; S. Franco; S. Frasca; F. Frasconi; Z. Frei; A. Freise; R. Frey; T. T. Fricke; P. Fritschel; V. V. Frolov; S. Fuentes-Tapia; P. Fulda; M. Fyffe; J. R. Gair; L. Gammaitoni; S. Gaonkar; F. Garufi; A. Gatto; N. Gehrels; G. Gemme; B. Gendre; E. Genin; A. Gennai; L. Á. Gergely; S. Ghosh; J. A. Giaime; K. D. Giardina; A. Giazotto; J. Gleason; E. Goetz; R. Goetz; L. Gondan; G. González; N. Gordon; M. L. Gorodetsky; S. Gossan; S. Goßler; R. Gouaty; C. Gräf; P. B. Graff; M. Granata; A. Grant; S. Gras; C. Gray; R. J. S. Greenhalgh; A. M. Gretarsson; P. Groot; H. Grote; S. Grunewald; G. M. Guidi; C. J. Guido; X. Guo; K. Gushwa; E. K. Gustafson; R. Gustafson; J. Hacker; E. D. Hall; G. Hammond; M. Hanke; J. Hanks; C. Hanna; M. D. Hannam; J. Hanson; T. Hardwick; J. Harms; G. M. Harry; I. W. Harry; M. Hart; M. T. Hartman; C. -J. Haster; K. Haughian; S. Hee; A. Heidmann; M. Heintze; G. Heinzel; H. Heitmann; P. Hello; G. Hemming; M. Hendry; I. S. Heng; A. W. Heptonstall; M. Heurs; M. Hewitson; S. Hild; D. Hoak; K. A. Hodge; D. Hofman; S. E. Hollitt; K. Holt; P. Hopkins; D. J. Hosken; J. Hough; E. Houston; E. J. Howell; Y. M. Hu; E. Huerta; B. Hughey; S. Husa; S. H. Huttner; M. Huynh; T. Huynh-Dinh; A. Idrisy; N. Indik; D. R. Ingram; R. Inta; G. Islas; J. C. Isler; T. Isogai; B. R. Iyer; K. Izumi; M. Jacobson; H. Jang; P. Jaranowski; S. Jawahar; Y. Ji; F. Jiménez-Forteza; W. W. Johnson; D. I. Jones; R. Jones; R. J. G. Jonker; L. Ju; Haris K; V. Kalogera; S. Kandhasamy; G. Kang; J. B. Kanner; M. Kasprzack; E. Katsavounidis; W. Katzman

    2014-12-18

    We describe directed searches for continuous gravitational waves in data from the sixth LIGO science data run. The targets were nine young supernova remnants not associated with pulsars; eight of the remnants are associated with non-pulsing suspected neutron stars. One target's parameters are uncertain enough to warrant two searches, for a total of ten. Each search covered a broad band of frequencies and first and second frequency derivatives for a fixed sky direction. The searches coherently integrated data from the two LIGO interferometers over time spans from 5.3-25.3 days using the matched-filtering F-statistic. We found no credible gravitational-wave signals. We set 95% confidence upper limits as strong (low) as $4\\times10^{-25}$ on intrinsic strain, $2\\times10^{-7}$ on fiducial ellipticity, and $4\\times10^{-5}$ on r-mode amplitude. These beat the indirect limits from energy conservation and are within the range of theoretical predictions for neutron-star ellipticities and r-mode amplitudes.

  20. Mass Segregation in Young LMC Clusters I. NGC 2157

    E-Print Network [OSTI]

    Philippe Fischer; Carlton Pryor; Stephen Murray; Mario Mateo; Tom Richtler

    1997-10-31

    We have carried out WFPC2 V- and I-band imaging of the young LMC cluster NGC 2157. Construction of a color-magnitude diagram and isochrone fitting yields an age of tau = 100 000 000 yrs, a reddening E(B-V) = 0.1 and a distance modulus of 18.4 mag. Our data covers the mass range 0.75 < m < 5.1 solar masses. We find that the cluster mass function changes significantly from the inner regions to the outer regions, becoming steeper (larger number of low mass stars relative to high mass stars) at larger radii. The age of NGC 2157 is comparable to its two-body relaxation timescale only in the cluster core. The observed steepening of the mass function at larger radii is therefore most likely an initial condition of the cluster stars. Such initial conditions are predicted in models of cluster star formation in which dissipative processes act more strongly upon more massive stars.

  1. The Properties of Young Clusters in M82

    E-Print Network [OSTI]

    L. J. Smith; J. S. Gallagher

    2000-01-31

    We present a detailed study of two luminous super star clusters in the starburst galaxy M82. Spectra, covering 3250-8790 A at a resolution of 1.6 A, were obtained at the 4.2 m William Herschel Telescope (WHT) for cluster F and the highly reddened cluster L. We compare the strengths of the observed Balmer absorption lines and the Balmer jump in the blue spectrum of F with theoretical model cluster spectra using the PEGASE spectral synthesis code to derive an age of 60+/-20 Myr. For cluster L, we find that the similarities in the strength of the Ca II triplet and overall spectral appearance with cluster F suggest a similar age. The brightness and compactness of cluster F make it an ideal candidate for determining its dynamical mass by measuring the velocity dispersion. We present the results of such an investigation based on echelle spectra at a resolution of 8 km/s obtained at the WHT from 5760-9140 A. By cross-correlating various wavelength regions in the spectrum of cluster F with cool giant and supergiant template stars, we derive a velocity dispersion and, by application of the virial theorem, determine a dynamical mass of 2 million solar masses. We compare our derived mass with those determined for other young super star clusters and discuss whether our derived parameters are consistent with cluster F being able to survive to become a globular cluster.

  2. Interaction of Infall and Winds in Young Stellar Objects

    E-Print Network [OSTI]

    G. Delamarter; A. Frank; L. Hartmann

    1999-10-14

    The interaction of a stellar or disk wind with a collapsing environment holds promise for explaining a variety of outflow phenomena observed around young stars. In this paper we present the first simulations of these interactions. The focus here is on exploring how ram pressure balance between wind and ambient gas and post-shock cooling affects the shape of the resulting outflows. In our models we explore the role of ram pressure and cooling by holding the wind speed constant and adjusting the ratio of the inflow mass flux to the wind mass flux (Mdot_a/Mdot_w) Assuming non-spherical cloud collapse, we find that relatively strong winds can carve out wide, conical outflow cavities and that relatively weak winds can be strongly collimated into jet-like structures. If the winds become weak enough, they can be cut off entirely by the infalling environment. We identify discrepancies between results from standard snowplow models and those presented here that have important implications for molecular outflows. We also present mass vs. velocity curves for comparison with observations.

  3. SIMP J2154–1055: A NEW LOW-GRAVITY L4? BROWN DWARF CANDIDATE MEMBER OF THE ARGUS ASSOCIATION

    SciTech Connect (OSTI)

    Gagné, Jonathan; Lafrenière, David; Doyon, René; Artigau, Étienne; Malo, Lison; Robert, Jasmin; Nadeau, Daniel

    2014-09-01

    We present SIMP J21543454–1055308, a new L4? brown dwarf identified in the SIMP survey that displays signs of low gravity in its near-infrared spectrum. Using BANYAN II, we show that it is a candidate member of the Argus association, albeit with a 21% probability that it is a contaminant from the field. Measurements of radial velocity and parallax will be needed to verify its membership. If it is a member of Argus (age 30-50 Myr), then this object would have a planetary mass of 10 ± 0.5 M {sub Jup}.

  4. Comparison of MELCOR and SCDAP/RELAP5 results for a low-pressure, short-term station blackout at Browns Ferry

    SciTech Connect (OSTI)

    Carbajo, J.J. [Oak Ridge National Lab., TN (United States)

    1995-12-31

    This study compares results obtained with two U.S. Nuclear Regulatory Commission (NRC)-sponsored codes, MELCOR version 1.8.3 (1.8PQ) and SCDAP/RELAP5 Mod3.1 release C, for the same transient - a low-pressure, short-term station blackout accident at the Browns Ferry nuclear plant. This work is part of MELCOR assessment activities to compare core damage progression calculations of MELCOR against SCDAP/RELAP5 since the two codes model core damage progression very differently.

  5. Parenting style and older children's and young adolescents' dietary intake and nutritional status 

    E-Print Network [OSTI]

    Kim, Mi Jeong

    2007-09-17

    neglected. The present study examined whether perceived parenting style and its dimensions are associated with older children�s/young adolescents� health outcomes, including self-concept, eating behaviors, physical activity behaviors, energy...

  6. Tracking Reading: Dual Task Costs of Oral Reading for Young Versus Older Adults

    E-Print Network [OSTI]

    Kemper, Susan; Bontempo, Daniel; Schmalzried, RaLynn Cheri; McKedy, Whitney; Tagliaferri, Bruno; Kieweg, Doug

    2014-02-01

    A digital pursuit rotor was used to monitor oral reading costs by time-locking tracking performance to the auditory wave form produced as young and older adults were reading out short paragraphs. Multilevel modeling was ...

  7. Queering young adult literature: examining sexual minorities in contemporary realistic fiction 

    E-Print Network [OSTI]

    Wickens, Corrine Marie

    2009-05-15

    Fiction that incorporates gay, lesbian, bisexual, transgender, or questioning of heterosexuality itself (GLBTQ) themes and characters has been noted among the most widely censored novels for young adults (ALA, 2007; Finnessy, ...

  8. Young Professionals in Nuclear Industry Group Forms at Savannah River Site

    Broader source: Energy.gov [DOE]

    AIKEN, S.C. – Supporting the development of young nuclear professionals in the Central Savannah River Area (CSRA) is the purpose behind a new group forming at the Savannah River Site (SRS).

  9. Professional environment of post-school transitions of young people with additional support needs 

    E-Print Network [OSTI]

    Brown, Joan

    2012-11-29

    The focus of this qualitative study is the professional environment where post-school transitions take place. It seeks to identify some possible means for improving outcomes for young people with low educational achievement, ...

  10. RADIO DETECTION OF GREEN PEAS: IMPLICATIONS FOR MAGNETIC FIELDS IN YOUNG GALAXIES

    E-Print Network [OSTI]

    Chakraborti, Sayan

    Green Peas are a new class of young, emission line galaxies that were discovered by citizen volunteers in the Galaxy Zoo project. Their low stellar mass, low metallicity, and very high star formation rates make Green Peas ...

  11. Optical Third-Harmonic Generation in Graphene Hong, Sung-Young...

    Office of Scientific and Technical Information (OSTI)

    Third-Harmonic Generation in Graphene Hong, Sung-Young; Dadap, Jerry I.; Petrone, Nicholas; Yeh, Po-Chun; Hone, James; Osgood, Richard M. American Physical Society None USDOE...

  12. The shared experience of adolescent and young adult cancer patients and their caregivers

    E-Print Network [OSTI]

    Juth, V; Silver, RC; Sender, L

    2015-01-01

    young adult survivors of childhood cancer. Oncology Nursingadults with cancer. Journal of Pediatric Oncology Nursing,adults with cancer: Comparing the findings from two qualitative studies. European Journal of Oncology Nursing,

  13. Survey of Brain Variations of Young Adult and Aged B2 (-/-) Knockout Mice 

    E-Print Network [OSTI]

    Kuban, J Katherine

    2008-07-16

    loss and therefore decreased brain area and that this effect would be pronounced in older ?2 (-/-) knockout mice compared to younger mice. Currently, young adult mice (2-3 month old), have been evaluated, and no significant statistical difference...

  14. Engineering and Science Experts Needed to Assist Young People 14 January 2014

    E-Print Network [OSTI]

    Hansen, James E.

    reconstruction of a pipeline that caused a major oil spill. They want to use the necessity defense, their actions for why unconventional fossil fuels should not be developed and likely will harm the future of young

  15. Stay on marked paths to avoid poison ivy. Watch young children carefully around river and creeks.

    E-Print Network [OSTI]

    Shyy, Wei

    Caution · Stay on marked paths to avoid poison ivy. · Watch young children carefully around river or outdoor cooking are not permitted. Poison Ivy Hours · Trails and gardens open 8 am to dusk. · Conservatory

  16. PHYTOREMEDIATION OF CHLORPYRIFOS BY POPULUS AND Keum Young Lee, Stuart E. Strand, and Sharon L. Doty

    E-Print Network [OSTI]

    Doty, Sharon Lafferty

    PHYTOREMEDIATION OF CHLORPYRIFOS BY POPULUS AND SALIX Keum Young Lee, Stuart E. Strand, and Sharon of chlorpyrifos, several plant species of poplar (Populus sp.) and willow (Salix sp.) were investigated

  17. The voice-bar after closure of coda consonants in the speech of young children

    E-Print Network [OSTI]

    Cho, Won Ron

    2008-01-01

    The purpose of this study is to gain some insight into the speech acquisition process and articulator development of young children whose mother-tongue is American English. The presence of voice-bars after the closure of ...

  18. A Feminist Dialogue on Theatre for Young Audiences through Suzan Zeder's Plays.

    E-Print Network [OSTI]

    Klein, Jeanne; Austin, Gayle; Zeder, Suzan; Still, James; Smith, Iris

    1997-01-01

    Klein and Austin share perceptions of Theatre for Young Audiences and discuss three plays by Suzan Zeder using feminist dramatic criticism. Zeder responded from her playwright's perspective. Subsequently, playwright James ...

  19. Enhancing Interventions for Pediatric Obesity Among Young Latino Children: A Mixed Methods Study

    E-Print Network [OSTI]

    Sampilo, Marilyn L.

    2014-12-31

    Recent national data indicate that nearly 1/3 of US youth are overweight (BMI % 85th). Of these children, a disproportionate number are Latino. This racial and ethnic disparity has been observed in young childhood and ...

  20. Different effects of dual task demands on the speech of young and older adults

    E-Print Network [OSTI]

    Kemper, Susan; Herman, Ruth; Nartowicz, Jennifer

    2005-12-01

    Young and older adults provided language samples in response to elicitation questions while concurrently performing 3 different tasks. The language samples were scored on three dimensions: fluency, grammatical complexity, and content. Previous...

  1. arXiv:astro-ph/0310394v115Oct2003 Palomar Testbed Interferometer Observations of Young

    E-Print Network [OSTI]

    arXiv:astro-ph/0310394v115Oct2003 Palomar Testbed Interferometer Observations of Young Stellar Cygni. Our K-band (2.2 µm) observations from the Palomar Testbed Interferometer (PTI) used baselines

  2. Eating Attitudes and Behaviours in Young People With or Without a Diabetic Sibling 

    E-Print Network [OSTI]

    Smith, Rachel K

    2007-01-01

    Objectives: Body image concerns and problematic eating attitudes and behaviours are recognised as an important concern for young people and clinicians. Identification of groups that might be at risk of developing such ...

  3. Priming the interpretation of ambiguous noun-noun compounds in young children 

    E-Print Network [OSTI]

    Fialka, Justine K B

    2010-06-30

    Abstract: Investigation into adult language users’ interpretation of ambiguous noun-noun compounds has been considerably explored and documented. However, investigation into the same phenomenon in a population such as young ...

  4. Quality of Life Concerns in Young Adult Survivors of Childhood Cancer: A Qualitative Research Investigation 

    E-Print Network [OSTI]

    Puckett, Stevie

    2013-06-13

    , while balancing the dual roles of young adult and survivor. Survivors revealed difficulties in essentially every area of their lives (school, work, friendships, family, romance, self-esteem, outlook and attitudes, etc.), and though many could identify...

  5. I Am the Monster: Self and the Monstrous Feminine in Contemporary Young Adult Literature 

    E-Print Network [OSTI]

    Talafuse, Elizabeth

    2014-05-15

    My dissertation surveys British, American, Australian, and New Zealand young adult texts of the late twentieth and early twenty-first centuries featuring female protagonists who are fantastic monsters. Addressing such texts ...

  6. A Model for Conducting Research with Learning Disabled Adolescents and Young Adults

    E-Print Network [OSTI]

    Meyen, Edward L.; Schiefelbusch, Richard L.; Deshler, Donald D.; Alley, Gordon R.; Schumaker, Jean B.; Clark, Frances L.

    1980-01-01

    Issues from the field of learning disabilities and the field of education in general which impact the learning disabled individual are discussed as they relate to research with learning disabled adolescents and young adults ...

  7. A Research Strategy for Studying Learning Disabled Adolescents and Young Adults

    E-Print Network [OSTI]

    Schumaker, Jean B.; Alley, Gordon R.; Warner, Michael M.; Deshler, Donald D.

    1980-01-01

    Unique problems related to adolescents and young adults which researchers must consider in designing interventions are discussed. These unique factors associate with the condition of learning disabilities in adolescents ...

  8. Assessing the Health Care Needs of Kansas' Young Adults with Disabilities

    E-Print Network [OSTI]

    Hall, Jean P.; Starrett, B.

    2007-08-01

    Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Assessing the Health Care Needs of Kansas' Young Adults with Disabilities Jean Hall; Barbara Starrett Kansas Nurse; Aug 2007; 82, 7; Pro...Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. Assessing the Health Care Needs of Kansas' Young Adults with Disabilities Jean Hall; Barbara Starrett Kansas Nurse; Aug 2007; 82, 7; Pro...

  9. Water destruction by X-rays in young stellar objects

    E-Print Network [OSTI]

    P. Stauber; J. K. Jorgensen; E. F. van Dishoeck; S. D. Doty; A. O. Benz

    2006-02-06

    We study the H2O chemistry in star-forming environments under the influence of a central X-ray source and a central far ultraviolet (FUV) radiation field. The gas-phase water chemistry is modeled as a function of time, hydrogen density and X-ray flux. To cover a wide range of physical environments, densities between n_H = 10^4-10^9 cm^-3 and temperatures between T = 10-1000 K are studied. Three different regimes are found: For T water abundance is of order 10^-7-10^-6 and can be somewhat enhanced or reduced due to X-rays, depending on time and density. For 100 K 10^-3 ergs s-1 cm^-2 (t = 10^4 yrs) and for F_X > 10^-4 ergs s^-1 cm^-2 (t = 10^5 yrs). At higher temperatures (T > 250 K) and hydrogen densities, water can persist with x(H2O) ~ 10^-4 even for high X-ray fluxes. The X-ray and FUV models are applied to envelopes around low-mass Class 0 and I young stellar objects (YSOs). Water is destroyed in both Class 0 and I envelopes on relatively short timescales (t ~ 5000 yrs) for realistic X-ray fluxes, although the effect is less prominent in Class 0 envelopes due to the higher X-ray absorbing densities there. FUV photons from the central source are not effective in destroying water. The average water abundance in Class I sources for L_X > 10^27 ergs s^-1 is predicted to be x(H2O) < 10^-6.

  10. Uranium and thorium decay series disequilibria in young volcanic rocks

    SciTech Connect (OSTI)

    Williams, R.W.

    1988-01-01

    Two of the central questions in igneous geochemistry that study of radioactive disequilibria can help to answer are: what are the rates of magma genesis; and what are the timescales of magma separation and transport. In addition to the temporal information that may be extracted from disequilibria data, the {sup 230}Th/{sup 232}Th of a young rock may be used as a tracer of the Th/U ratio of its source region. Measurements were made by isotope dilution alpha-spectrometry of {sup 238}U, {sup 234}U, {sup 230}Th, and {sup 232}Th in 20 subduction related, 3 oceanic intraplate, and 10 continental intraplate volcanics. {sup 210}Pb was measured in all, {sup 226}Ra was measured in about half, and {sup 228}Th was measured in 10 of the most recent samples. Disequilibrium between {sup 228}Th and {sup 232}Th was found only in the Nacarbonatite samples from Oldoinyo Lengai volcano in Tanzania, which is attributable to {sup 228}Ra/{sup 232}Th {approximately} 27 at the time of eruption. These rocks also have {sup 226}Ra/{sup 230}Th > 60. Three Ra-enrichment models are developed which constrain carbonatite magma formation at less than 20 years before eruption. The effects of different partial melting processes on the {sup 238}U decay series are investigated. If mid-ocean ridge basalts are formed by a dynamic melting process, the {sup 230}Th/{sup 232}Th of the basalts provides a minimum estimate of the Th/U ratio of the source region. The {sup 238}U enrichment in arc volcanics is probably the results of metasomatism of the source by fluids derived from the subducting slab, and the {sup 230}Th enrichment observed for other volcanics is probably due to the partial melting process in the absence of U-bearing fluids.

  11. THE ENIGMATIC YOUNG, LOW-MASS VARIABLE TWA 30

    SciTech Connect (OSTI)

    Looper, Dagny L.; Rayner, John; Pitts, Mark A.; Mohanty, Subhanjoy; Bochanski, John J.; Burgasser, Adam J.; Mamajek, Eric E.; Herczeg, Gregory J.; West, Andrew A.; Faherty, Jacqueline K.; Kirkpatrick, J. Davy

    2010-05-01

    TWA 30 is a remarkable young (7 {+-} 3 Myr), low-mass (0.12 {+-} 0.04 M{sub sun}), late-type star (M5 {+-} 1) residing 42 {+-} 2 pc away from the Sun in the TW Hydrae Association (TWA). It shows strong outflow spectral signatures such as [S II], [O I], [O II], [O III], and Mg I], while exhibiting weak H{alpha} emission (-6.8 {+-} 1.2 A). Emission lines of [S II] and [O I] are common to T Tauri stars still residing in their natal molecular clouds, while [O III] and Mg I] emission lines are incredibly rare in this same population; in the case of TWA 30, these latter lines may arise from new outflow material colliding into older outflow fronts. The weak H{alpha} emission and small radial velocity shifts of line emission relative to the stellar frame of rest (generally {approx_lt}10 km s{sup -1}) suggest that the disk is viewed close to edge-on and that the stellar axis may be inclined to the disk, similar to the AA Tau system, based on its temporal changes in emission/absorption line strengths/profiles and variable reddening (A{sub V} = 1.5-9.0). The strong Li absorption (0.61 {+-} 0.13 A) and common kinematics with members of the TWA confirm its age and membership to the association. Given the properties of this system such as its proximity, low mass, remarkable outflow signatures, variability, and edge-on configuration, this system is a unique case study at a critical time in disk evolution and planet-building processes.

  12. Brown blob (algae?) (Native) 

    E-Print Network [OSTI]

    James R. Manhart

    2011-08-10

    | pg. 20 cientists at three Texas universities investigating golden algae, its explosive growth, and its deadly toxins have dis- covered an apparent competition between golden algae and blue green algae in certain Texas lakes. Understanding... this competition could lead them closer to controlling this harmful algae, the researchers said. ?Our biggest finding so far,? said Dr. Daniel Roelke of Texas AgriLife Research and one of the investigators, ?is that there appears to be a chemical warfare...

  13. Brown Chapter 1

    E-Print Network [OSTI]

    Insuring a nuclear reactor against ... concealment of some fact or knowledge, is able to bring a risk to .... 1.5 Assume the management of a firm has utility function.

  14. Brown-Peterson

    E-Print Network [OSTI]

    This partial failure of the Morava structure theorem is compensated for by the lack ...... In the latter case, Theorem 3.7 would not give us the precise control we need ...... This induction is trivial to ground; just use K(n)*(BP__2) = K(n)*(K(Z(p); ...

  15. Brown Bag Teaching Seminar

    E-Print Network [OSTI]

    When the department chooses a new Head (roughly, every five years), ... c) Certification and licensure examinations d) External accreditation reports e) ...

  16. Brown Chapter 2

    E-Print Network [OSTI]

    coverages include boiler and machinery insurance, contract surety insurance, business interruption insurance, and many others. Each coverage has its own ...

  17. Brown University Mathematics Department

    E-Print Network [OSTI]

    Schwartz, Richard Evan

    Introduction 1 Math 42 Introduction to Number Theory 2 Math 52 Linear Algebra 4 Math 54 Honors Linear Algebra 6 Math 141 Combinatorial Topology 23 Math 153 Abstract Algebra 25 Math 154 Topics in Abstract Algebra 27 Statistics 34 Math 201 Diferential Geometry 35 Math 205-206 Algebraic Geometry 38 Math 211 Introduction

  18. brown-98.pdf

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power AdministrationRobust,Field-effectWorkingLos Alamos verifiesValidationENCOAL®April 8, 2014 In replyHigh

  19. brown-99.PDF

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power AdministrationRobust,Field-effectWorkingLos Alamos verifiesValidationENCOAL®April 8, 2014 In replyHighNCAR/ARM

  20. Changes in char structure during the gasification of a Victorian brown coal in steam and oxygen at 800{degree}C

    SciTech Connect (OSTI)

    Xin Guo; Hui Ling Tay; Shu Zhang; Chun-Zhu Li [Monash University, Vic. (Australia). Department of Chemical Engineering

    2008-11-15

    Char structure is an important factor influencing its reactivity during gasification. This study aims to investigate the changes in char structure during the gasification of brown coal. A Victorian brown coal was gasified in a fluidized-bed/fixed-bed reactor at 800{degree}C in atmospheres containing 15% H{sub 2}O, 2000 ppm O{sub 2}, or 15% H{sub 2}O and 2000 ppm O{sub 2}, respectively. Although the char gasification in 2000 ppm O{sub 2} was mainly rate-limited by the external diffusion of O{sub 2}, the char-H{sub 2}O reaction was mainly rate-limited by the chemical reactions. The structural features of char at different levels of char gasification conversion were examined with FT-Raman spectroscopy. Our results show that the chars from the gasification in the mixture of 2000 ppm O{sub 2} and 15% H{sub 2}O had almost the same features as the chars from the gasification in 15% H{sub 2}O alone when the same levels of char conversion were achieved. Both the thermal decomposition of char and the char gasification reactions could result in changes in char structure during gasification. 29 refs., 5 figs., 1 tab.

  1. They are often eclipsed by more attractive topics, like black holes or exoplanets. Even the name itself is less than sensational: brown dwarfs. But Viki Joergens and her

    E-Print Network [OSTI]

    Joergens, Viki

    this threshold possess. The fundamental characteris- tic of stars consists in the multi-step fusion of hydrogen in the cloud center becomes more and more compressed until hydrogen fusion begins. The young star Institute for Astronomy in Heidelberg have gained fascinating insights in this research field. Neither Star

  2. A Model for Parent-Teacher Collaboration to Promote Self-Determination in Young Children With Disabilities

    E-Print Network [OSTI]

    Lee, Suk-Hyang; Palmer, Susan B.; Turnbull, Ann P.; Wehmeyer, Michael L.

    2006-01-01

    Curriculum Modifications and Accommodations t s a A Model for Parent-Teacher Collaboration to Promote SeK-Determination in Young Children With Disabilities Suk-Hyang Lee Susan B. Palmer Ann P. TXirnbull Michael L. Wehmeyer Young's mother says she...Curriculum Modifications and Accommodations t s a A Model for Parent-Teacher Collaboration to Promote SeK-Determination in Young Children With Disabilities Suk-Hyang Lee Susan B. Palmer Ann P. TXirnbull Michael L. Wehmeyer Young's mother says she...

  3. Corona driven air propulsion for cooling of electronics F. Yang, N.E. Jewell-Larsen, D.L. Brown, K. Pendergrass, D.A. Parker, I.A. Krichtafovitch*, A.V. Mamishev

    E-Print Network [OSTI]

    Mamishev, Alexander

    Corona driven air propulsion for cooling of electronics F. Yang, N.E. Jewell-Larsen, D.L. Brown, K of Washington, Seattle, WA 98105, USA *Chief Scientific Officer, Kronos Air Technologies, Redmond, WA 98052, USA Abstract: The possibility of building a high voltage electrostatic air pump for cooling of microelectronics

  4. Cloud Structure of the Nearest Brown Dwarfs II: High-amplitude variability for Luhman 16 A and B in and out of the 0.99 micron FeH feature

    E-Print Network [OSTI]

    Buenzli, Esther; Apai, Dániel; Saumon, Didier; Biller, Beth A; Crossfield, Ian J M; Radigan, Jacqueline

    2015-01-01

    The re-emergence of the 0.99 $\\mu$m FeH feature in brown dwarfs of early- to mid-T spectral type has been suggested as evidence for cloud disruption where flux from deep, hot regions below the Fe cloud deck can emerge. The same mechanism could account for color changes at the L/T transition and photometric variability. We present the first observations of spectroscopic variability of brown dwarfs covering the 0.99 $\\mu$m FeH feature. We observed the spatially resolved very nearby brown dwarf binary WISE J104915.57-531906.1 (Luhman 16AB), a late-L and early-T dwarf, with HST/WFC3 in the G102 grism at 0.8-1.15 $\\mu$m. We find significant variability at all wavelengths for both brown dwarfs, with peak-to-valley amplitudes of 9.3% for Luhman 16B and 4.5% for Luhman 16A. This represents the first unambiguous detection of variability in Luhman 16A. We estimate a rotational period between 4.5 and 5.5 h, very similar to Luhman 16B. Variability in both components complicates the interpretation of spatially unresolved ...

  5. Young Pulsars and the Galactic Center GeV Gamma-ray Excess

    E-Print Network [OSTI]

    Ryan M. O'Leary; Matthew D. Kistler; Matthew Kerr; Jason Dexter

    2015-04-09

    Studies of Fermi data indicate an excess of GeV gamma rays around the Galactic center (GC), possibly due to dark matter. We show that young gamma-ray pulsars can yield a similar signal. First, a high concentration of GC supernovae naturally leads to a population of kicked pulsars symmetric about the GC. Second, while very-young pulsars with soft spectra reside near the Galactic plane, pulsars with spectra that have hardened with age accumulate at larger angles. This combination, including unresolved foreground pulsars, traces the morphology and spectrum of the Excess.

  6. Young Pulsars and the Galactic Center GeV Gamma-ray Excess

    E-Print Network [OSTI]

    O'Leary, Ryan M; Kerr, Matthew; Dexter, Jason

    2015-01-01

    Studies of Fermi data indicate an excess of GeV gamma rays around the Galactic center (GC), possibly due to dark matter. We show that young gamma-ray pulsars can yield a similar signal. First, a high concentration of GC supernovae naturally leads to a population of kicked pulsars symmetric about the GC. Second, while very-young pulsars with soft spectra reside near the Galactic plane, pulsars with spectra that have hardened with age accumulate at larger angles. This combination, including unresolved foreground pulsars, traces the morphology and spectrum of the Excess.

  7. Assessing "Dangerous Climate Change": Required Reduction of Carbon Emissions to Protect Young People, Future Generations and Nature

    E-Print Network [OSTI]

    Hansen, James E.

    Assessing "Dangerous Climate Change": Required Reduction of Carbon Emissions to Protect Young high and would subject young people, future generations and nature to irreparable harm. Carbon dioxide. Of course carbon dioxide from deforestation also causes warming and policies must address that carbon source

  8. Deformation zone `jumps' in a young convergent setting; the Lengguru fold-and-thrust belt, New Guinea Island

    E-Print Network [OSTI]

    Nicolas, Chamot-Rooke

    Deformation zone `jumps' in a young convergent setting; the Lengguru fold-and-thrust belt, New The Lengguru fold-and-thrust belt in West Papua (Indonesia) has all the characteristics of a young orogen buttress. The construction of these two wedges is younger than 11 Myr. The structures of the Lengguru belt

  9. Caffeine and stress alter salivary a-amylase activity in young men Laura C. Klein1*, Jeanette M. Bennett1

    E-Print Network [OSTI]

    Ritter, Frank

    Caffeine and stress alter salivary a-amylase activity in young men Laura C. Klein1*, Jeanette M and a psychological stressor on salivary a-amylase (sAA) in healthy young males (age 18­ 30 years) who consumed. Copyright # 2010 John Wiley & Sons, Ltd. key words -- blood pressure; caffeine; heart rate; salivary alpha-amylase

  10. Water movement and its resistance in young trees of Cryptomeria japonica

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    Water movement and its resistance in young trees of Cryptomeria japonica H. Yahata Laboratory Information about water flow resistance is essential to understanding and simulating water movement in trees japonica and no data are available on the gradient of water potential in intact stem. This study

  11. ORIGINAL ARTICLE -H2AX foci are increased in lymphocytes in vivo in young

    E-Print Network [OSTI]

    Brenner, David Jonathan

    very low ionizing radiation exposure doses from CT exams can induce -H2AX formation in vivo in young children. Objective To test whether very low ionizing radiation doses from CT exams can induce lymphocytic low-dose X-irradiation: a pilot study Brunhild M. Halm & Adrian A. Franke & Jennifer F. Lai & Helen C

  12. Anorexia nervosa during adolescence and young adulthood: Towards a developmental and integrative approach sensitive to

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    1 Anorexia nervosa during adolescence and young adulthood: Towards a developmental and integrative of print" DOI : 10.1016/j.jphysparis.2013.03.010 #12;2 Abstract Anorexia nervosa is situated of the underlying mental disorder. Taken together, these observations support an approach to anorexia nervosa

  13. Murder Mystery Day Day event for young people in care in school years 10-13

    E-Print Network [OSTI]

    Jackson, Sophie

    Murder Mystery Day Day event for young people in care in school years 10-13 Develop your scientific investigative skills while investigating a fiendish crime! Take part in solving a murder mystery activity, plus: Saturday 11 July 2015 www.cam.ac.uk/care-events #12;Murder Mystery Day www

  14. Carbon fluxes in a young, naturally regenerating jack pine ecosystem Eugenie S. Euskirchen

    E-Print Network [OSTI]

    Chen, Jiquan

    , are measurements within young, recently disturbed ecosystems. [3] Generally, net ecosystem productivity (NEP, or equiv- alently, net ecosystem exchange of carbon, NEE = ­NEP; where a positive value of NEP indicates a C uptake, or equivalently, a C sink, and a negative value of NEP indicates a C loss, or equivalently

  15. Instructor: Brad de Young Physics and Physical Oceanography bdeyoung@physics.mun.ca

    E-Print Network [OSTI]

    deYoung, Brad

    Instructor: Brad de Young Physics and Physical Oceanography bdeyoung@physics.mun.ca Room C-3000 737-8738 This course will cover data analysis techniques in oceanography. We will cover some basic time-series analysis for this paper: (i) Maximum Entropy Analysis, (ii) Neural networks, (iii) Oceanography 6316 ­ Winter 2007 Physics

  16. An adult pine weevil feeding on the bark of the main stem of a young tree.

    E-Print Network [OSTI]

    Figure 1 An adult pine weevil feeding on the bark of the main stem of a young tree. 1 P R A C T I C forest sites after clearfelling. Typically, adult weevils feed on bark of the main stem (Figure 1 of attack, the main management alternatives are to delay planting, to restock with pre- treated trees or

  17. Atmosphere-crust coupling and carbon sequestration on the young Mars Professor Martin R. Lee1

    E-Print Network [OSTI]

    Guo, Zaoyang

    Atmosphere-crust coupling and carbon sequestration on the young Mars Professor Martin R. Lee1 *, Dr the idea that CO2 was `scrubbed' by precipitation of carbonate minerals within the planet's crust - a reaction termed `carbonation'. This project will seek evidence for carbonation by analysis of martian

  18. The Astrophysical Journal, in press A Determination of the Coronal Emission Measure Distribution in the Young

    E-Print Network [OSTI]

    Guedel, Manuel

    to this temperature regime. We argue that the DEM distribution seen in EK Dra is induced by the propertiesThe Astrophysical Journal, in press A Determination of the Coronal Emission Measure Distribution of a coronal differential emission measure (DEM) analysis of the nearby analog of the young Sun, EK Draconis

  19. Top-Down Influence in Young Children's Linguistic Ambiguity Resolution Hugh Rabagliati

    E-Print Network [OSTI]

    Pylkkänen, Liina

    Top-Down Influence in Young Children's Linguistic Ambiguity Resolution Hugh Rabagliati New York adults resolve syntactic ambiguities by integrating a variety of cues, children are less sensitive to top-down evidence. We test whether this top-down insensitivity is specific to syntax or a general feature

  20. Session: Poster Session + Poster Award + Scientific Award + Excellent young wind doctor award (PO.56) Track: Technical

    E-Print Network [OSTI]

    Session: Poster Session + Poster Award + Scientific Award + Excellent young wind doctor award (PO.56) Track: Technical CONNECTING THE OFFSHORE WIND AND WAVE RESOURCE CALCULATIONS (abstract-ID: 462) Gregor Giebel (Risø DTU, Wind Energy Department, Denmark) Teresa Pontes, Portugal (1) Rebecca Barthelmie

  1. Session: Poster Session + Poster Award + Scientific Award + Excellent young wind doctor award (PO.206) Track: Technical

    E-Print Network [OSTI]

    Session: Poster Session + Poster Award + Scientific Award + Excellent young wind doctor award (PO.206) Track: Technical INVESTIGATION OF THE MEASUREMENT OF THE WIND SPEED STANDARD DEVIATION USING) Siemens wind power The LiDAR seems to be an effective alternative to met masts measurements of wind

  2. Session: Poster Session + Poster Award + Scientific Award + Excellent young wind doctor award (PO.201) Track: Technical

    E-Print Network [OSTI]

    Session: Poster Session + Poster Award + Scientific Award + Excellent young wind doctor award (PO.201) Track: Technical OPERATIONAL EXPERIENCE AND ANALYSIS OF A SPINNER ANEMOMETER ON A MW SIZE WIND TURBINE (abstract-ID: 356) Troels Friis Pedersen (Risø DTU, Wind Energy Department, Denmark) Uwe Schmidt

  3. Session: Poster Session + Poster Award + Scientific Award + Excellent young wind doctor award (PO.139) Track: Technical

    E-Print Network [OSTI]

    Session: Poster Session + Poster Award + Scientific Award + Excellent young wind doctor award (PO.139) Track: Technical VARIABLE SPEED WIND TURBINES ­ FAULT RIDE-THROUGH AND GRID SUPPORT CAPABILITIES is on the fault ride through and grid support capability of variable speed wind turbines. The paper focuses

  4. Session: Poster Session + Poster Award + Scientific Award + Excellent young wind doctor award (PO.141) Track: Technical

    E-Print Network [OSTI]

    Session: Poster Session + Poster Award + Scientific Award + Excellent young wind doctor award (PO.141) Track: Technical MODELLING AND FAULT RIDE-THROUGH CAPABILITY OF A FULL CONVERTER WIND TURBINE WITH MULTI-POLE PMSG (abstract-ID: 114) Anca Hansen (Risø DTU, Wind Energy Department, Denmark) Gabriele

  5. Earth's Glow on the Young Moon: A Conjecture on the Lunar Farside Asymmetry

    E-Print Network [OSTI]

    Rhoads, James

    Earth's Glow on the Young Moon: A Conjecture on the Lunar Farside Asymmetry Arpita Roy & Jason of the Moon with the Earth" by Stigmatella aurantiaca Licensed under CC BY-SA 3.0 via Wikimedia Commons File:Tidal_locking_of_the_Moon_with_the_Earth Hypothesis: Moon formed from impact of Mars sized protoplanet, "Theia", with proto-earth Moon formed from

  6. Chinese-English Code-switching in Blogs by Macao Young People 

    E-Print Network [OSTI]

    San, Hong Ka

    2009-11-26

    This paper attempts to investigate Chinese-English code-switching behaviour present in blogs (a kind of computer-mediated communication) belonging to young people in Macao. The first goal of this study is to describe the patterns of Chinese...

  7. Study of Latina Mothers' Coping Processes While Their Young Adult Sons Are Incarcerated

    E-Print Network [OSTI]

    Hayes-Bautista, Teodocia Maria

    2013-01-01

    Mexican American adults. Oncology Nursing Forum 36, 413-420Adult Sons Are Incarcerated by Teodocia Maria Hayes-Bautista Doctor of Philosophy in NursingNursing Research so that I can understand how Latina mothers cope while their young adult

  8. An experience of young software engineers' employability in the Moroccan offshore industry

    E-Print Network [OSTI]

    Brest, Université de

    An experience of young software engineers' employability in the Moroccan offshore industry Philippe the emergence of an offshore software development industry in Morocco. A network of eight Moroccan universities and the University of Brest has set up a mobility scheme for Moroccan Master students. The OTI programme "Offshoring

  9. Implicit Learning of Predictive Relationships in Three-Element Visual Sequences by Young and Old Adults

    E-Print Network [OSTI]

    Dennis, Nancy

    sequence task and illustrate its utility for investi- gating procedural learning in healthy old adultsImplicit Learning of Predictive Relationships in Three-Element Visual Sequences by Young and Old Adults James H. Howard Jr. The Catholic University of America and Georgetown University Darlene V. Howard

  10. Climate signal age effects--Evidence from young and old trees in the Swiss Engadin

    E-Print Network [OSTI]

    Esper, Jan

    Climate signal age effects--Evidence from young and old trees in the Swiss Engadin Jan Esper a of these long-term records are composed of >1000- year old living trees, such as the reconstructions from different climatic information than ``adult'' rings that are typically defined as being older than 50

  11. Enhanced Teleoperation for D&D Young S. Park, Hyosig Kang, Thomas F. Ewing

    E-Print Network [OSTI]

    Amaral, Luis A.N.

    Enhanced Teleoperation for D&D Young S. Park, Hyosig Kang, Thomas F. Ewing Nuclear Engineering-based control architecture and cobot control technology. Keywords ­ teleoperation, teleautonomy Platform (DAWP) system for dismantling the CP-5 reactor internals at Argonne National Laboratory. Despite

  12. Ph.D in Economics at the Andrew Young School, Georgia State University

    E-Print Network [OSTI]

    Frantz, Kyle J.

    Ph.D in Economics at the Andrew Young School, Georgia State University WHY Georgia State University's Department of Economics? We are part of one of America's best public affairs graduate schools: the Andrew in scholarly journals including Econometrica, American Economic Review, Journal of Political Economy, Quarterly

  13. iD Tech needs your help to inspire more young women to enter the

    E-Print Network [OSTI]

    Oviedo, Néstor J.

    -18 as well as a new all-girls option (Alexa Café for ages 10-15). At Alexa Café, we also emphasize techiD Tech needs your help to inspire more young women to enter the tech industry and make their voices and ideas heard. iD Tech is determined to help reshape the face of the tech industry by providing

  14. Loyalty Fund + for deceased donors | ^ for young alumni 2014 Loyalty Fund Honor Roll | page 2

    E-Print Network [OSTI]

    Holliday, Mark A.

    Roll | page 2 2013­2014 Donors The 2014 Loyalty Fund Honor Roll includes alumni, friends and parents Steed Gold Scholars: $1,000-$4,999 Katherine Abbott-Beam '67 and David Beam Cynthia H. '71 and Robert H `77 Alan T. '69 and Cynthia Yount #12;+ for deceased donors | ^ for young alumni 2014 Loyalty Fund

  15. Basin-Wavelength Equatorial Deep Jet Signals Across Three Oceans1 Madeleine K. Youngs2

    E-Print Network [OSTI]

    Johnson, Gregory C.

    of intermediate and deep water masses in the Atlantic. Brandt et al. (2011, 2012) argue38 that as wellBasin-Wavelength Equatorial Deep Jet Signals Across Three Oceans1 Madeleine K. Youngs2 NOAA/Pacific Marine Environmental Laboratory, Seattle WA and Environmental Science and Engineering, California

  16. Virus Calculated as Culprit Killing Sea Stars By Ben Young Landis

    E-Print Network [OSTI]

    Virus Calculated as Culprit Killing Sea Stars By Ben Young Landis [Reprinted from USGS Science Features: Top Story, November 17, 2014, virus://soundwaves.usgs.gov/ (Virus Killing Sea Stars continued on page 2) Sound Waves Volume FY 2015, Issue No. 156156 January

  17. In today's world, financial education is crucial; however, many young people are leaving high school lacking

    E-Print Network [OSTI]

    Relevance In today's world, financial education is crucial; however, many young people are leaving say students are prepared to deal with the financial challenges awaiting them in the adult world. More The Welcome to the Real World! (WTTRW) program consists of two parts: financial education and real-world

  18. http://valhalla.chem.udel.edu/YSA.pdf Philadelphia Multi-Stake -Young Single Adult

    E-Print Network [OSTI]

    Firestone, Jeremy

    http://valhalla.chem.udel.edu/YSA.pdf Philadelphia Multi-Stake - Young Single Adult Comprising the Stakes in Cherry Hill NJ, Philadelphia PA, Reading PA, Valley Forge PA and Wilmington DE Please send at 3913 Chestnut Street, Philadelphia, at 5:00. Be prompt, as the activity will move on from there. Bring

  19. YOUNG MEASURES AND ORDER-DISORDER TRANSITION IN STATIONARY FLOW OF LIQUID CRYSTALS

    E-Print Network [OSTI]

    Panchenko, Alexander

    YOUNG MEASURES AND ORDER-DISORDER TRANSITION IN STATIONARY FLOW OF LIQUID CRYSTALS M. CARME measures generated by sequences of weak solutions of the governing equations. It is experimentally well [-1, 1] with R2 Ã? (-1, 1), representing the domain of the flow. The governing system is highly

  20. YOUNG MEASURES AND ORDER-DISORDER TRANSITION IN STATIONARY FLOW OF LIQUID CRYSTALS

    E-Print Network [OSTI]

    YOUNG MEASURES AND ORDER-DISORDER TRANSITION IN STATIONARY FLOW OF LIQUID CRYSTALS By M. Carme AND ORDER-DISORDER TRANSITION IN STATIONARY FLOW OF LIQUID CRYSTALS M. CARME CALDERER AND ALEXANDER of the governing equations. It is experimentally well known that liquid crystal flows with large Ericksen number