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<ri:Resource created="2013-04-29T12:24:34Z" 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 six RGB stars in M22</title><shortName>J/ApJ/742/37</shortName><identifier>ivo://CDS.VizieR/J/ApJ/742/37</identifier><altIdentifier>doi:10.26093/cds/vizier.17420037</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Roederer I.U.</name></creator><creator><name>Marino A.F.</name></creator><creator><name>Sneden C.</name></creator><date role="Updated">2017-11-29T11:48:31Z</date><date role="Created">2013-04-29T12:24:34Z</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>globular-star-clusters</subject><subject>chemical-abundances</subject><subject>giant-stars</subject><subject>radial-velocity</subject><description>We present an empirical s-process abundance distribution derived with explicit knowledge of the r-process component in the low-metallicity globular cluster M22. We have obtained high-resolution, high signal-to-noise spectra for six red giants in M22 using the Magellan Inamori Kyocera Echelle spectrograph on the Magellan-Clay Telescope at Las Campanas Observatory. In each star we derive abundances for 44 species of 40 elements, including 24 elements heavier than zinc (Z=30) produced by neutron-capture reactions. Previous studies determined that three of these stars (the "r+s group") have an enhancement of s-process material relative to the other three stars (the "r-only group"). We confirm that the r+s group is moderately enriched in Pb relative to the r-only group. Both groups of stars were born with the same amount of r-process material, but s-process material was also present in the gas from which the r+s group formed. The s-process abundances are inconsistent with predictions for asymptotic giant branch (AGB) stars with M&lt;=3M_{sun}_ and suggest an origin in more massive AGB stars capable of activating the ^22^Ne({alpha},n)^25^Mg reaction. We calculate the s-process "residual" by subtracting the r-process pattern in the r-only group from the abundances in the r+s group. In contrast to previous r- and s-process decompositions, this approach makes no assumptions about the r- and s-process distributions in the solar system and provides a unique opportunity to explore s-process yields in a metal-poor environment.</description><source format="bibcode">2011ApJ...742...37R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/742/37</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/541/A15">J/A+A/541/A15 : Abundances of M22 subgiants (Marino+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/62/357">J/AcA/62/357 : Proper motions of 6 globular clusters (Zloczewski+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/1481">J/ApJ/705/1481 : Spectroscopy of stars in 6 GCs (Da Costa+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/349/1278">J/MNRAS/349/1278 : BVI photometry of M22 (Monaco+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/373/899">J/A+A/373/899 : New variables in M22 globular cluster (Kaluzny+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/107/32">J/PASP/107/32 : uvby-hk photometry in M22 (Anthony-Twarog+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/99/637">J/ApJS/99/637 : Equivalent widths for 54 red giants (Norris+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/109/487">J/A+AS/109/487 : Color-magnitude study of M 22 (Samus+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/303/468">J/A+A/303/468 : Spec. &amp; IR-phot. in globular clusters (Minniti, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/420/612">J/ApJ/420/612 : Proper motions + radial velocities in M22 (Peterson+ 1994)</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/742/37</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/742/37</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/742/37</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/742/37</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/742/37</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/742/37</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/742/37/table1 (Photometry, atmospheric parameters, radial velocities, exposure times, and S/N estimates)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/742/37/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/742/37/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/742/37/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>279.1274583</ra><dec>-23.88025</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/28972 28973</spatial><spectral>3.322582951404819e-19 3.852589004194616e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/742/37?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/742/37/table2</name><description>Line-by-line abundances</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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