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<ri:Resource created="2006-12-21T11:16:35Z" 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>Lithium content of the Galactic Halo stars</title><shortName>J/A+A/442/961</shortName><identifier>ivo://CDS.VizieR/J/A+A/442/961</identifier><altIdentifier>doi:10.26093/cds/vizier.34420961</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Charbonnel C.</name></creator><creator><name>Primas F.</name></creator><date role="Updated">2017-10-13T15:42:09Z</date><date role="Created">2006-12-21T11:16:35Z</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>population-ii-stars</subject><subject>chemically-peculiar-stars</subject><description>Thanks to the accurate determination of the baryon density of the universe by the recent cosmic microwave background experiments, updated predictions of the standard model of Big Bang nucleosynthesis now yield the initial abundance of the primordial light elements with unprecedented precision. In the case of ^7^Li, the CMB+SBBN value is significantly higher than the generally reported abundances for Pop II stars along the so-called Spite plateau. In view of the crucial importance of this disagreement, which has cosmological, galactic and stellar implications, we decided to tackle the most critical issues of the problem by revisiting a large sample of literature Li data in halo stars that we assembled following some strict selection criteria on the quality of the original analyses. We dissect our sample in search of new constraints on Li depletion in halo stars. By means of the Hipparcos parallaxes, we derive the evolutionary status of each of our sample stars, and re-discuss our derived Li abundances.</description><source format="bibcode">2005A&amp;A...442..961C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/442/961</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/J/A+A/352/117">J/A+A/352/117 : Galactic lithium evolution revisited (Romano+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/105/2299">J/AJ/105/2299 : Li abundance of solar-type stars. II. (Soderblom+, 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/363/239">J/A+A/363/239 : Lithium abundances in single giant stars (De Medeiros+, 2000)</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+A/409/251">J/A+A/409/251 : Li abundances and velocities in F and G stars (Mallik+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/349/757">J/MNRAS/349/757 : Masses, ages and metallicities of F-G dwarfs (Lambert+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/57/45">J/PASJ/57/45 : Lithium abundances of F-K stars (Takeda+, 2005)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/442/961</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/442/961</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/442/961</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/442/961</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/442/961</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/442/961</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/A+A/442/961/table3 (The data sample and its main characteristics, as found in the literature)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/442/961/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/442/961/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/442/961/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>1.4416264</ra><dec>-19.6702467</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/146 154 373 488 798 2133 2997 3494 3712 3814 3970 4184 4376 4526 4905 5111 5195 5458 5589 6058 6159 6186 6256 6348 6792-6793 7117 7334 7456 8210 8779 8999 9004 9831 9992 9996 10359 10476 11999 12332 12451 12621 13020 13028 13075 13628 13829 14298 14385 14679 14743 14956 16115 16803 16808 16880 17099 17124 17136 17245 17509 17578 18887 19206 19347 19603 19766 20646 21269 21926 22205 23011 23070 23192 23607 23893 25051 25554 25595 25891 25948 26025 26030 26284 26289 26347 26534 27075 27091 27128 27330 27763 27915 27948 28154 28336 29490 29593 29596 29765 30179 30577 30939 31094 31748 32034 32302 32343 32468 32593 32743 33131 33273 33831 34684 35551 35913 35989 36135 36745 36888 40567 41460 41721 42331 43310 43445 43786 43962 44208 44281 44542 44575 44816 44880 46023 46506 46828 47147 47347 47596 48281 48736 48946 49105</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/442/961?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/442/961/table3</name><description>The data sample and its main characteristics, as found in the literature</description><column><name>HD</name><description>? 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Second value of surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]</name><description>Metallicity</description><unit>log(Sun)</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]2</name><description>? Second value of metallicity</description><unit>log(Sun)</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_EW</name><description>Limit flag on EW</description><ucd>meta.code.error;spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>EW</name><description>? 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