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<ri:Resource created="2014-12-12T13:12:11Z" 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>Potassium abundance in red giants of GCs</title><shortName>J/ApJ/769/40</shortName><identifier>ivo://CDS.VizieR/J/ApJ/769/40</identifier><altIdentifier>doi:10.26093/cds/vizier.17690040</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Carretta E.</name></creator><creator><name>Gratton R.G.</name></creator><creator><name>Bragaglia A.</name></creator><creator><name>D'Orazi V.</name></creator><creator><name>Lucatello S.,Sollima A.</name></creator><creator><name>Sneden C.</name></creator><date role="Updated">2017-10-03T05:12:35Z</date><date role="Created">2014-12-12T13:12:11Z</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><subject>line-intensities</subject><description>Two independent studies recently uncovered two distinct populations among giants in the distant, massive globular cluster (GC) NGC 2419. One of these populations has normal magnesium (Mg) and potassium (K) abundances for halo stars: enhanced Mg and roughly solar K. The other population has extremely depleted Mg and very enhanced K. To better anchor the peculiar NGC 2419 chemical composition, we have investigated the behavior of K in a few red giant branch stars in NGC 6752, NGC 6121, NGC 1904, and {omega} Cen. To verify that the high K abundances are intrinsic and not due to some atmospheric features in giants, we also derived K abundances in less evolved turn-off and subgiant stars of clusters 47 Tuc, NGC 6752, NGC 6397, and NGC 7099. We normalized the K abundance as a function of the cluster metallicity using 21 field stars analyzed in a homogeneous manner. For all GCs of our sample, the stars lie in the K-Mg abundance plane on the same locus occupied by the Mg-normal population in NGC 2419 and by field stars. This holds for both giants and less-evolved stars. At present, NGC 2419 seems unique among GCs.</description><source format="bibcode">2013ApJ...769...40C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/769/40</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/VII/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/572/A108">J/A+A/572/A108 : 47 Tuc red giants chemical composition (Thygesen+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/550/A34">J/A+A/550/A34 : Abundances of red giants in M4 and 47 Tuc (Carretta+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/760/86">J/ApJ/760/86 : Equivalent widths for 13 NGC2419 RGB stars (Cohen+, 2012)</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/ApJ/742/37">J/ApJ/742/37 : Abundances of six RGB stars in M22 (Roederer+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/740/60">J/ApJ/740/60 : EWs for NGC2419 and NGC7099 RGB stars (Cohen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/81">J/AJ/141/81 : NGC 2419 variable star population (Di Criscienzo+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A148">J/A+A/527/A148 : NGC6397 red giants chemical composition (Lind+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/712/L21">J/ApJ/712/L21 : Calcium abundances in 17 globular clusters (Carretta+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/520/A95">J/A+A/520/A95 : Abundances of red giants in M54 and Sgr dSph (Carretta+, 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/ApJ/698/2048">J/ApJ/698/2048 : Abundances of red giants in {omega} Cen (Johnson+, 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/464/927">J/A+A/464/927 : Abundances of red giants in NGC 6752 (Carretta+, 2007)</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><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/354/169">J/A+A/354/169 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