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<ri:Resource created="2026-06-12T10:11:31Z" status="active" updated="2026-06-12T09:12:48Z" 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>n-catpure abundances in NGC 6752</title><shortName>J/MNRAS/520/5938</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/520/5938</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Schiappacasse-Ulloa J.</name></creator><creator><name>Lucatello S.</name></creator><date role="Updated">2026-06-12T09:12:48Z</date><date role="Created">2026-06-12T10:11:31Z</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>milky-way-galaxy</subject><subject>globular-star-clusters</subject><subject>population-ii-stars</subject><subject>stellar-populations</subject><subject>supergiant-stars</subject><subject>giant-stars</subject><subject>chemically-peculiar-stars</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><description>Globular clusters have been widely studied in terms of light element variations present in their different stellar populations. However, the nature of the polluter(s) responsible for this phenomenon is still debated. The study of heavy elements and their relation to light ones can provide further constraints. In particular, we aim to explore the possible contribution of asymptotic giant branch stars of different stellar masses to the internal pollution in the cluster. We derive abundances of elements from different nucleosynthetic chains, such as Na, Mg, Ca, Sc, Cu, Y, and Ba. We did not find clear relations between the light s-process elements (represented by Y II) or heavy ones (represented by Ba II) with light elements (Li, Na, or Al). This indicates that the polluter(s) responsible for the Na (Al) or Li production does not produce large amounts of Y II and Ba II. Furthermore, the comparison with models discards a possible significant contribution to the cluster pollution from AGB stars with masses lower than 5 M_{Sun}_. In addition, we found a potential CH star in our sample.</description><source format="bibcode">2023MNRAS.520.5938S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/520/5938</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/791/39">J/ApJ/791/39 : NGC 6218 and NGC 5904 lithium abundances (D'Orazi+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/750/L14">J/ApJ/750/L14 : Abundances of red giants in NGC 6752 (Carretta+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/567/A72">J/A+A/567/A72 : Stellar parameters and abundances in NGC 6752</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A69">J/A+A/533/A69 : Spectroscopy of 124 RGB stars in NGC 1851 (Carretta+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/511/231">J/MNRAS/511/231 : Lithium study with GC NGC 6752 (Schiappacasse-Ulloa+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/117">J/A+A/505/117 : Abundances of red giants in 15 globular clusters</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/139">J/A+A/505/139 : Abundances of red giants in 17 globular clusters</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/MNRAS/449/4038">J/MNRAS/449/4038 : Li abundance of giants in 3 globular clusters</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/350/955">J/A+A/350/955 : Atmospheric parameters in metal-poor stars. II</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/175">J/AJ/141/175 : Abundances in M15 RGB/RHB stars (Sobeck+, 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/MNRAS/520/5938</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/520/5938</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/520/5938</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/520/5938</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/520/5938</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/520/5938</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/MNRAS/520/5938/table2 (Abundances and errors obtained from spectra of NGC 6752 stars sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/520/5938/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/520/5938/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/520/5938/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>287.7843667</ra><dec>-59.9277086</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/MNRAS/520/5938?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/520/5938/table2</name><description>Abundances and errors obtained from spectra of NGC 6752 stars sample</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>Identifier name from NGC 6752 IDs and 2MASS JHHMMSS.ss+DDMMSS.s designation (ID)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>l_[O/Fe]</name><description>Upper limit flag of [O/Fe]</description><ucd>meta.code.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[O/Fe]</name><description>? Oxygen to iron abundance ratio ([O/Fe])</description><unit>log(Sun)</unit><ucd>phys.abund;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_[Na/Fe]</name><description>Upper limit flag of [Na/Fe]</description><ucd>meta.code.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[Na/Fe]</name><description>? Sodium to iron abundance ratio ([Na/Fe])</description><unit>log(Sun)</unit><ucd>phys.abund;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Na/Fe]</name><description>? 1{sigma} uncertainty of [Na/Fe] ({sigma})</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_[Mg/Fe]</name><description>Upper limit flag of [Mg/Fe]</description><ucd>meta.code.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[Mg/Fe]</name><description>? Magnesium to iron abundance ratio ([Mg/Fe])</description><unit>log(Sun)</unit><ucd>phys.abund;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Mg/Fe]</name><description>? 1{sigma} uncertainty of [Mg/Fe] ({sigma})</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ca/Fe]</name><description>? Calcium to iron abundance ratio ([Ca/Fe])</description><unit>log(Sun)</unit><ucd>phys.abund;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Ca/Fe]</name><description>? 1{sigma} uncertainty of [Ca/Fe] ({sigma})</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Sc/Fe]</name><description>? Scandium to iron abundance ratio ([Sc/Fe])</description><unit>log(Sun)</unit><ucd>phys.abund;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Sc/Fe]</name><description>? 1{sigma} uncertainty of [Sc/Fe] ({sigma})</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_[Cu/Fe]</name><description>Upper limit flag of [Cu/Fe]</description><ucd>meta.code.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[Cu/Fe]</name><description>? Copper to iron abundance ratio ([Cu/Fe])</description><unit>log(Sun)</unit><ucd>phys.abund;meta.modelled;arith</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Cu/Fe]</name><description>? 1{sigma} uncertainty of [Cu/Fe] ({sigma})</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_[Y/Fe]</name><description>Upper limit flag of [Y/Fe]</description><ucd>meta.code.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[Y/Fe]</name><description>? 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