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<ri:Resource created="2012-04-26T15:21:16Z" 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>Calcium abundances in 17 globular clusters</title><shortName>J/ApJ/712/L21</shortName><identifier>ivo://CDS.VizieR/J/ApJ/712/L21</identifier><altIdentifier>doi:10.26093/cds/vizier.17129021</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.</name></creator><creator><name>Lucatello S.</name></creator><creator><name>Bellazzini M.,D'Orazi V.</name></creator><date role="Updated">2017-10-11T05:13:21Z</date><date role="Created">2012-04-26T15:21:16Z</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>chemical-abundances</subject><subject>globular-star-clusters</subject><subject>giant-stars</subject><description>We use abundances of Ca, O, Na, and Al from high-resolution UVES spectra of 200 red giants in 17 globular clusters (GCs) to investigate the correlation found by Lee et al. (2009Icar..199..413C) between chemical enrichment from SNII and star-to-star variations in light elements in GC stars. We find that (1) the [Ca/H] variations between first and second generation stars are tiny in most GCs (~0.02-0.03dex, comparable with typical observational errors). In addition, (2) using a large sample of red giants in M4 (NGC 6121) with abundances from UVES spectra from Marino et al. (2008, Cat. J/A+A/490/625), we find that Ca and Fe abundances in the two populations of Na-poor and Na-rich stars are identical.</description><source format="bibcode">2010ApJ...712L..21C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/712/L21</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/505/139">J/A+A/505/139 : Abundances of red giants in 17 globular clusters (Carretta+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/503/545">J/A+A/503/545 : Equivalent widths of Li, Na, Fe, Ca in NGC 6397 (Lind+, 2009)</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/A+A/490/777">J/A+A/490/777 : Abundances of Population II stars in NGC 6397 (Lind+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/486/941">J/A+A/486/941 : Abundances in M71 (NGC 6838) (Alves-Brito+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/464/939">J/A+A/464/939 : Abundances of red giants in NGC 6218 (Carretta+, 2007)</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/131/1766">J/AJ/131/1766 : Abundances and equivalent widths in NGC 2808 (Carretta, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/434/235">J/A+A/434/235 : Abundances of BHB stars in NGC 1904 (Fabbian+, 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></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/712/L21</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/712/L21</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/712/L21</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/712/L21</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/712/L21</mirrorURL><mirrorURL title="VizieR at SAAO: 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