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<ri:Resource created="2015-08-06T13:52:30Z" 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>Iron EWs for 21 giant star members of NGC3201</title><shortName>J/ApJ/801/69</shortName><identifier>ivo://CDS.VizieR/J/ApJ/801/69</identifier><altIdentifier>doi:10.26093/cds/vizier.18010069</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mucciarelli A.</name></creator><creator><name>Lapenna E.</name></creator><creator><name>Massari D.</name></creator><creator><name>Ferraro F.R.</name></creator><creator><name>Lanzoni B.</name></creator><date role="Updated">2022-05-02T14:43:43Z</date><date role="Created">2015-08-06T13:52:30Z</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>line-intensities</subject><subject>metallicity</subject><subject>radial-velocity</subject><subject>giant-stars</subject><subject>globular-star-clusters</subject><description>NGC 3201 is a globular cluster suspected to have an intrinsic spread in the iron content. We re-analyzed a sample of 21 cluster stars observed with UVES-FLAMES at the Very Large Telescope and for which Simmerer et al. (2013ApJ...764L...7S) found a 0.4dex wide [Fe/H] distribution with a metal-poor tail. We confirmed that when spectroscopic gravities are adopted, the derived [Fe/H] distribution spans ~0.4dex. On the other hand, when photometric gravities are used, the metallicity distribution from Fe I lines remains large, while that derived from Fe II lines is narrow and compatible with no iron spread. We demonstrate that the metal-poor component claimed by Simmerer et al. (2013ApJ...764L...7S) is composed by asymptotic giant branch stars that could be affected by non-local thermodynamical equilibrium effects driven by iron overionization. This leads to a decrease of the Fe I abundance, while leaving the Fe II abundance unaltered. A similar finding has been already found in asymptotic giant branch stars of the globular clusters M5 and 47 Tucanae. We conclude that NGC 3201 is a normal cluster, with no evidence of intrinsic iron spread.</description><source format="bibcode">2015ApJ...801...69M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/801/69</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/B/eso">B/eso : ESO Science Archive Catalog (ESO, 1991-2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/780/94">J/ApJ/780/94 : Abundances of red giants in 47 Tuc (Cordero+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A18">J/A+A/527/A18 : EW of 6 subgiants of {omega} Cen (Pancino+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/726/L20">J/ApJ/726/L20 : Spectroscopy of Terzan 5 (Origlia+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/722/1373">J/ApJ/722/1373 : {omega} Centauri giants abundances (Johnson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/517/A81">J/A+A/517/A81 : 2nd &amp; 3d param. of HB of globular clusters (Gratton+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/139">J/A+A/505/139 : Abundances of red giants in 17 GCs (Carretta+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/383/183">J/MNRAS/383/183 : CaII triplet of RGB from VLT/FLAMES obs. (Battaglia+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/1298">J/AJ/134/1298 : CaII EWs in 29 Galactic clusters (Carrera+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/161/304">J/ApJS/161/304 : Star clusters in the MW and satellites (McLaughlin+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/2140">J/AJ/130/2140 : Abundances &amp; velocities in globular clusters (Pritzl+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/416/1117">J/A+A/416/1117 : Abundances in the early Galaxy (Cayrel+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/22/269">J/PAZh/22/269 : Giant branch and variable stars in NGC 3201 (Samus+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/90/83">J/ApJS/90/83 : Binaries in NGC 3201 (Cote+, 1994)</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/801/69</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/801/69</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/801/69</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/801/69</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/801/69</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/801/69</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/801/69/table1 (Main information of the target stars)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/801/69/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/801/69/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/801/69/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>154.308468</ra><dec>-46.412579</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/38465</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/801/69?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJ/801/69/table1</name><description>Main information of the target stars</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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