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<ri:Resource created="2014-01-29T08:10:00Z" 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 of red giants in NGC 6752</title><shortName>J/ApJ/750/L14</shortName><identifier>ivo://CDS.VizieR/J/ApJ/750/L14</identifier><altIdentifier>doi:10.26093/cds/vizier.17509014</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Carretta E.</name></creator><creator><name>Bragaglia A.</name></creator><creator><name>Gratton R.G.</name></creator><creator><name>Lucatello S.</name></creator><creator><name>D'Orazi V.</name></creator><date role="Updated">2023-04-20T15:51:59Z</date><date role="Created">2014-01-29T08:10:00Z</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>giant-stars</subject><subject>globular-star-clusters</subject><description>We present aluminum, magnesium, and silicon abundances in the metal-poor globular cluster NGC 6752 for a sample of more than 130 red giants with homogeneous oxygen and sodium abundances. We find that [Al/Fe] shows a spread of about 1.4 dex among giants in NGC 6752 and is anticorrelated with [Mg/Fe] and [O/Fe] and correlated with [Na/Fe] and [Si/Fe]. These relations are not continuous in nature, but the distribution of stars is clearly clustered around three distinct Al values, low, intermediate, and high. These three groups nicely correspond to the three distinct sequences previously detected using Stromgren photometry along the red giant branch. These two independent findings strongly indicate the existence of three distinct stellar populations in NGC 6752. Comparing the abundances of O and Mg, we find that the population with intermediate chemical abundances cannot originate from material with the same composition of the most O- and Mg-poor population, diluted by material with that of the most O- and Mg-rich one. This calls for different polluters.</description><source format="bibcode">2012ApJ...750L..14C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/750/L14</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/other/Nat/498.198">J/other/Nat/498.198 : Na abundances in NGC6752 (Campbell+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/423/2901">J/MNRAS/423/2901 : NGC 6752 multiwavelength survey (Thomson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/524/A44">J/A+A/524/A44 : CN and CH line strengths in 12 globulars (Pancino+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/517/A81">J/A+A/517/A81 : 2nd &amp; 3d parameters of HB of GCs (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/A+A/505/117">J/A+A/505/117 : Abundances of red giants in 15 GCs (Carretta+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/464/927">J/A+A/464/927 : Abundances of red giants in NGC 6752 (Carretta+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/1693">J/AJ/130/1693 : HST-ACS observations of 5 globular clusters (Brown+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/440/901">J/A+A/440/901 : Reddening and metallicity of NGC 6752 (Gratton, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/404/187">J/A+A/404/187 : Equivalent widths for metal-poor stars (Gratton+, 2003)</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/750/L14</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/750/L14</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/750/L14</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/750/L14</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/750/L14</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/750/L14</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/750/L14/table1 ([Mg/Fe], [Al/Fe], and [Si/Fe] ratios for red giants in NGC 6752)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/750/L14/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/750/L14/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/750/L14/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>288.0030833333</ra><dec>-60.0032916667</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/47125 47168</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/750/L14?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJ/750/L14/table1</name><description>[Mg/Fe], [Al/Fe], and [Si/Fe] ratios for red giants in NGC 6752</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>ID</name><description>[1217/48975] Star identification number (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>o_[Mg/Fe]</name><description>[0/3] Number of lines used to determine [Mg/Fe]</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Mg/Fe]</name><description>[0.07/0.6]? Log of Mg to Fe abundance</description><unit>log(Sun)</unit><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Mg/Fe]</name><description>[0.004/0.3]? 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