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<ri:Resource created="2013-06-18T10:16:22Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Abundances (Be,{alpha}) in metal-poor stars</title><shortName>J/ApJ/743/140</shortName><identifier>ivo://CDS.VizieR/J/ApJ/743/140</identifier><altIdentifier>doi:10.26093/cds/vizier.17430140</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Boesgaard A.M.</name></creator><creator><name>Rich J.A.</name></creator><creator><name>Levesque E.M.</name></creator><creator><name>Bowler B.P.</name></creator><date role="Updated">2017-06-30T05:49:10Z</date><date role="Created">2013-06-18T10:16:22Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>chemical-abundances</subject><subject>line-intensities</subject><subject>chemically-peculiar-stars</subject><subject>radial-velocity</subject><description>The light elements, Li, Be, and B, provide tracers for many aspects of astronomy including stellar structure, Galactic evolution, and cosmology. We have made observations of Be in 117 metal-poor stars ranging in metallicity from [Fe/H]=-0.5 to -3.5 with Keck I/HIRES. Our spectra are high resolution (~42000) and high signal to noise (the median is 106 per pixel). We have determined the stellar parameters spectroscopically from lines of FeI, FeII, TiI, and TiII. The abundances of Be and O were derived by spectrum synthesis techniques, while abundances of Fe, Ti, and Mg were found from many spectral line measurements. We have kinematic information on 114 stars in our sample and they divide equally into dissipative and accretive stars.</description><source format="bibcode">2011ApJ...743..140B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/743/140</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/V/130">V/130 : Geneva-Copenhagen Survey of Solar neighbourhood III (Holmberg+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/124/164">J/PASP/124/164 : Lithium measurements in metal-poor stars (Schaeuble+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/522/A26">J/A+A/522/A26 : Fe Abundances in metal-poor stars (Sbordone+ 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/445/939">J/A+A/445/939 : Metal-poor stars uvby-beta photometry. XI. (Schuster+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/367/1329">J/MNRAS/367/1329 : Elemental abundances for 176 stars (Reddy+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/438/139">J/A+A/438/139 : Abundances in Milky Way's disk (Soubiran+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/442/961">J/A+A/442/961 : Lithium content of the Galactic Halo stars (Charbonnel+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/82/453">J/AZh/82/453 : Cat. of spectroscopic abundances in stars (Borkova+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/30/173">J/PAZh/30/173 : Space velocities of solar neighborhood stars (Borkova+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/418/551">J/A+A/418/551 : Galactic disk stars abundances &amp; velocities (Mishenina+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1177">J/AJ/128/1177 : Galactic stellar abundances (Venn+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/371/943">J/A+A/371/943 : Lithium abundances for 185 main-sequence stars (Chen+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/141/491">J/A+AS/141/491 : Chemical composition of halo and disk stars (Nissen+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/319/593">J/A+A/319/593 : [Be] abundances in low-metallicity stars (Molaro+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/107/2240">J/AJ/107/2240 : Proper motion stars survey. 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