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<ri:Resource created="2005-02-20T21:59:48Z" 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>Equivalent widths of 9 barium stars</title><shortName>J/AZh/81/658</shortName><identifier>ivo://CDS.VizieR/J/AZh/81/658</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Antipova L.I.</name></creator><creator><name>Boyarchuk A.A.</name></creator><creator><name>Pakhomov Yu.V.</name></creator><creator><name>Panchuk V.E.</name></creator><date role="Updated">2017-12-06T07:38:30Z</date><date role="Created">2005-02-20T21:59:48Z</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>giant-stars</subject><subject>line-intensities</subject><description>We present our analysis of elemental abundances in the atmospheres of 16 classical barium stars derived from high-resolution spectra and model atmospheres. Comparison of the results with analogous data for moderate barium stars and normal red giants shows that the abundance patterns for elements before the iron peak are the same for all three groups of red giants, testifying to a similar origin. For binary systems, we confirm the influence of the orbital period and, hence, the component separation, on the overabundance of s-process elements. The amount of enrichment in s-process elements is also in influenced by mass, metallicity, and evolutionary phase. Any of these parameters can be important in individual objects.</description><source format="bibcode">2004AZh....81..658A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/81/658</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/AZh/78/807">J/AZh/78/807 : Chemical composition of eta Ser (Antipova+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/79/909">J/AZh/79/909 : Chemical abundances in barium stars (Boyarchuk+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/80/704">J/AZh/80/704 : Studies of classical barium stars (Antipova+, 2003)</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/81/658</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AZh/81/658</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AZh/81/658</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AZh/81/658</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AZh/81/658</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AZh/81/658</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/AZh/81/658/stars (List of the 9 stars studied)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AZh/81/658/stars?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AZh/81/658/stars?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AZh/81/658/stars?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>41.94875</ra><dec>81.448611</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/4041 5624 13244 28959 30640 30659 40311 44488 45027</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AZh/81/658?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AZh/81/658/stars</name><description>List of the 9 stars studied</description><column><name>Bmag</name><description>Blue magnitude (from Simbad)</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HD</name><description>HD (Cat. III/135)</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right Ascension J2000 (hours)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination J2000 (degrees)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Vmag</name><description>Visible magnitude (from Simbad)</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SpType</name><description>MK Spectral classification (from Simbad)</description><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/AZh/81/658/table2</name><description>The equivalent widths</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>El</name><description>Element</description><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Lambda</name><description>Wavelength expressed in Angstroems</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ExcPot</name><description>Excitation potentials of the lower level</description><unit>eV</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Loggf</name><description>Oscillator strength (log gf)</description><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W1</name><description>? Equivalent width of HD 16458</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W2</name><description>? Equivalent width of HD 88562</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W3</name><description>? Equivalent width of HD 101013</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W4</name><description>? Equivalent width of HD 130386</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W5</name><description>? Equivalent width of HD 139409</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W6</name><description>? Equivalent width of HD 175190</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W7</name><description>? Equivalent width of HD 178717</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W8</name><description>? Equivalent width of HD 183915</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W9</name><description>? Equivalent width of HD 196673</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>