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<ri:Resource created="2012-06-25T20:10:16Z" 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>Li and Na in globular cluster M4</title><shortName>J/A+A/539/A157</shortName><identifier>ivo://CDS.VizieR/J/A+A/539/A157</identifier><altIdentifier>doi:10.26093/cds/vizier.35390157</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Monaco L.</name></creator><creator><name>Villanova S.</name></creator><creator><name>Bonifacio P.</name></creator><creator><name>Caffau E.</name></creator><creator><name>Geisler D.</name></creator><creator><name>Marconi G.,Momany Y.</name></creator><creator><name>Ludwig H.-G.</name></creator><date role="Updated">2012-07-14T19:55:05Z</date><date role="Created">2012-06-25T20:10:16Z</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>dwarf-stars</subject><subject>chemical-abundances</subject><description>The abundance inhomogeneities of light elements observed in globular clusters (GCs), and notably the ubiquitous Na-O anti-correlation, are generally interpreted as evidence that GCs comprise several generations of stars. There is an on-going debate as to the nature of the stars, which produce the inhomogeneous elements, and investigating the behavior of several elements is a way to shed new light on this problem. We aim at investigating the Li and Na content of the GC M4, that is known to have a well defined Na-O anti-correlation. We obtained moderate resolution (R=17000-18700) spectra for 91 main sequence (MS)/sub-giant branch stars of M4 with the Giraffe spectrograph at the FLAMES/VLT ESO facility. Using model atmospheres analysis we measured lithium and sodium abundances.</description><source format="bibcode">2012A&amp;A...539A.157M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/539/A157</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/ApJ/443/124">J/ApJ/443/124 : Radial Velocities of Stars in M4 (Peterson+ 1995)</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/AJ/114/189">J/AJ/114/189 : M4 CCD photometry (Alcaino+, 1997)</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/124/1486">J/AJ/124/1486 : M4 UBV color-magnitude diagrams (Mochejska+, 2002)</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/ApJ/689/1031">J/ApJ/689/1031 : Heavy element abundances in giant stars (Yong+, 2008)</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/MNRAS/412/81">J/MNRAS/412/81 : Lithium abundance in M4 red giants (Mucciarelli+, 2011)</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/539/A157</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/539/A157</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/539/A157</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/539/A157</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/539/A157</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/539/A157</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/539/A157/tablea1 (Basic data for MS/SGB stars studied in this paper)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/539/A157/tablea1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/539/A157/tablea1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/539/A157/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>246.0545833</ra><dec>-26.3929722</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/A+A/539/A157?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/539/A157/tablea1</name><description>Basic data for MS/SGB stars studied in this paper</description><column><name>Seq</name><description>Sequential number</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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