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<ri:Resource created="2012-06-21T13:07:21Z" 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 abundances in red giants of M4</title><shortName>J/ApJ/716/L166</shortName><identifier>ivo://CDS.VizieR/J/ApJ/716/L166</identifier><altIdentifier>doi:10.26093/cds/vizier.17169166</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>D'Orazi V.</name></creator><creator><name>Marino A.F.</name></creator><date role="Updated">2017-11-29T11:48:38Z</date><date role="Created">2012-06-21T13:07:21Z</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>globular-star-clusters</subject><subject>chemical-abundances</subject><subject>giant-stars</subject><description>The determination of Li and proton-capture element abundances in globular cluster (GC) giants allows us to constrain several key questions on the multiple population scenarios in GCs, from formation and early evolution to pollution and dilution mechanisms. In this Letter, we present our results on Li abundances for a large sample of giants in the intermediate-metallicity GC NGC 6121 (M4), for which Na and O have been already determined by Marino et al. (2008, Cat. J/A+A/490/625). The stars analyzed are both below and above the red giant branch bump luminosity. We found that the first and second generation stars share the same Li content, suggesting that a Li production must have occurred. This provides strong observational evidence supporting the scenario in which asymptotic giant branch stars are GC polluters.</description><source format="bibcode">2010ApJ...716L.166D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/716/L166</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/539/A157">J/A+A/539/A157 : Lithium and sodium in M4 (Monaco+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/412/81">J/MNRAS/412/81 : Lithium abundance in M4 red giants (Mucciarelli+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/490/625">J/A+A/490/625 : Abundances of NGC 6121 red giants (Marino+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/689/1031">J/ApJ/689/1031 : Heavy element abundances in giant stars (Yong+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/2771">J/AJ/127/2771 : HST proper-motions of M4 main-sequence stars (Richer+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/1486">J/AJ/124/1486 : M4 UBV color-magnitude diagrams (Mochejska+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/120/265">J/ApJS/120/265 : HST photometry of M4 (Ibata+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/114/189">J/AJ/114/189 : M 4 CCD photometry (Alcaino+, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/22/847">J/PAZh/22/847 : Identification and coordinates in M4 (Shokin+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/443/124">J/ApJ/443/124 : Radial Velocities of Stars in M4 (Peterson+ 1995)</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/ApJ/716/L166</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/716/L166</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/716/L166</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/716/L166</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/716/L166</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/716/L166</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/ApJ/716/L166/table1 (Stellar parameters and abundances for our sample stars)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/716/L166/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/716/L166/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/716/L166/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>245.94994389</ra><dec>-26.54524111</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/42955</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/716/L166?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/716/L166/table1</name><description>Stellar parameters and abundances for our sample stars</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Star</name><description>[5359/45895] Stellar identification number (&lt;Cl* NGC 6121 MVP NNNNN&gt; in Simbad)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Teff</name><description>[3860/4950] Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>log(g)</name><description>[0.5/3.05] Log of the surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>xi</name><description>[1.1/1.88] Turbulent velocity</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Na/Fe]</name><description>[-0.05/0.53] Log Na/Fe number abundance ratio</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Na/Fe]</name><description>Error in [Na/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logn(Li)</name><description>[0/1.62] Log of Li number abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logn(Li)</name><description>Error in logn(Li)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Positions from Marino et al. 2008, Cat. 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