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<ri:Resource created="2003-04-30T22:04:23Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Chemical abundances in barium stars</title><shortName>J/AZh/79/909</shortName><identifier>ivo://CDS.VizieR/J/AZh/79/909</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Boyarchuk A.A.</name></creator><creator><name>Pakhomov Yu.V.</name></creator><creator><name>Antipova L.I.</name></creator><creator><name>Boyarchuk M.E.</name></creator><date role="Updated">2003-04-30T22:04:28Z</date><date role="Created">2003-04-30T22:04:23Z</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>barium-stars</subject><subject>line-intensities</subject><description>We used high-resolution spectra to compute model atmospheres to derive the atmospheric abundances of moderate barium stars. Comparing our results with analogous data for normal red giants, we find that the moderate barium stars appear to not differ systematically from normal red giants. Their chemical abundance anomalies show the same patterns and can be interpreted in terms of evolutionary effects: the evolutionary stage, mass, luminosity, and metallicity of the objects.</description><source format="bibcode">2002AZh....79..909B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/79/909</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/80/704">J/AZh/80/704 : Studies of classical barium stars (Antipova+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/81/658">J/AZh/81/658 : Equivalent widths of 9 barium stars (Antipova+, 2004)</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/AZh/79/909</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AZh/79/909</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AZh/79/909</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AZh/79/909</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AZh/79/909</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AZh/79/909</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AZh/79/909/table2</name><description>Elemental abundances in the atmosphere of program stars relative to solar abundances</description><column><name>EWkOph</name><description>? Equivalent width of kappa Oph</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>El</name><description>Element and ionization stage</description><ucd>phys.atmol.element</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Lambda</name><description>Wavelength</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ExcPot</name><description>Excitation potentials of the lower level</description><unit>eV</unit><ucd>phys.energy;phys.atmol.excitation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggf</name><description>Oscillator strength (log gf)</description><ucd>phys.atmol.wOscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EW18Mon</name><description>? Equivalent width of 18 Mon</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWiHya</name><description>? Equivalent width of iota Hya</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWbBoo</name><description>? Equivalent width of beta Boo</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWlHer</name><description>? Equivalent width of lam Her</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWeAql</name><description>? 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