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<ri:Resource created="2014-04-04T16:15:51Z" 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 and radial velocities of M13 giants</title><shortName>J/ApJ/754/L38</shortName><identifier>ivo://CDS.VizieR/J/ApJ/754/L38</identifier><altIdentifier>doi:10.26093/cds/vizier.17549038</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Johnson C.I.</name></creator><creator><name>Pilachowski C.A.</name></creator><date role="Updated">2021-08-04T12:53:33Z</date><date role="Created">2014-04-04T16:15:51Z</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>radial-velocity</subject><subject>effective-temperature</subject><subject>globular-star-clusters</subject><description>We present O, Na, and Fe abundances, as well as radial velocities, for 113 red giant branch (RGB) and asymptotic giant branch (AGB) stars in the globular cluster M13. The abundances and velocities are based on spectra obtained with the WIYN-Hydra spectrograph, and the observations range in luminosity from the horizontal branch (HB) to RGB tip. The results are examined in the context of recent globular cluster formation scenarios. We find that M13 exhibits many key characteristics that suggest its formation and chemical enrichment are well described by current models. Some of these observations include the central concentration of O-poor stars, the notable decrease in [O/Fe] (but small increase in [Na/Fe]) with increasing luminosity that affects primarily the "extreme" population, the small fraction of stars with halo-like composition, and the paucity of O-poor AGB stars. In agreement with recent work, we conclude that the most O-poor M13 giants are likely He-enriched and that most (all?) O-poor RGB stars evolve to become extreme HB and AGB-manqu\'e stars. In contrast, the "primordial" and "intermediate" population stars appear to experience standard HB and AGB evolution.</description><source format="bibcode">2012ApJ...754L..38J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/754/L38</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/248">II/248 : UBV photometry and proper motions in M13 (Kadla, 1966)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/26">IV/26 : Hercules Messier 13 (M13) photometry (Ludendorff, 1905)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/139/2374">J/AJ/139/2374 : Evolved stars in M13 (Sandquist+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/4282">J/AJ/137/4282 : Red giant stars in clusters. 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M13 and M92 (Meszaros+, 2009)</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/ApJ/638/1018">J/ApJ/638/1018 : Equivalent widths for giant stars in M13 and M71 (Yong+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/129/303">J/AJ/129/303 : Abundances of stars in M3 and M13 (Cohen+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/1579">J/AJ/127/1579 : Abundances of faint M13 stars (Briley+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/398/541">J/A+A/398/541 : VI light-curves of the variable stars in M13 (Kopacki+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/122/3219">J/AJ/122/3219 : M3 and M13 CCD BV photometry (Rey+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/120/1364">J/AJ/120/1364 : Abundances in M3 and M13 (Cavallo+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/113/669">J/AJ/113/669 : Stars in M13 core (Cohen+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/113/279">J/AJ/113/279 : Proton Capture Chains. II (Kraft+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/112/545">J/AJ/112/545 : Proton capture chains in GCs. I. 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