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<ri:Resource created="2005-05-09T07:04:18Z" 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>Galactic stellar abundances</title><shortName>J/AJ/128/1177</shortName><identifier>ivo://CDS.VizieR/J/AJ/128/1177</identifier><altIdentifier>doi:10.26093/cds/vizier.51281177</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Venn K.A.</name></creator><creator><name>Irwin M.</name></creator><creator><name>Shetrone M.D.</name></creator><creator><name>Tout C.A.</name></creator><creator><name>Hill V.</name></creator><creator><name>Tolstoy E.</name></creator><date role="Updated">2021-08-10T11:54:35Z</date><date role="Created">2005-05-09T07:04:18Z</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>milky-way-galaxy</subject><description>To compare the chemistries of stars in the Milky Way dwarf spheroidal (dSph) satellite galaxies with stars in the Galaxy, we have compiled a large sample of Galactic stellar abundances from the literature. When kinematic information is available, we have assigned the stars to standard Galactic components through Bayesian classification based on Gaussian velocity ellipsoids. As found in previous studies, the [{alpha}/Fe] ratios of most stars in the dSph galaxies are generally lower than similar metallicity Galactic stars in this extended sample.</description><source format="bibcode">2004AJ....128.1177V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/128/1177</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></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/AJ/128/1177</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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