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<ri:Resource created="2000-01-19T20:59:13Z" 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>Abundances of HR 4487, 14 Hyd and 3 Cen A</title><shortName>J/A+AS/129/563</shortName><identifier>ivo://CDS.VizieR/J/A+AS/129/563</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pintado O.I.</name></creator><creator><name>Adelman S.J.</name></creator><creator><name>Gulliver A.F.</name></creator><date role="Updated">2000-01-19T19:59:32Z</date><date role="Created">2000-01-19T20:59:13Z</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>peculiar-variable-stars</subject><subject>chemically-peculiar-stars</subject><description>Ussing CASLEO echelle spectrograms, elemental abundances are derived for the sharp-lined non-magnetic CP stars HR 4487, 14 Hya and 3 Cen A. The first two stars are members of the Mercury-Manganese subgroup and have abundances which are similar to other such peculiar stars. The third is a hotter related star. The detection of Mn II lines in its spectrum adds to this relationship.</description><source format="bibcode">1998A&amp;AS..129..563P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/129/563</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/A+AS/107/353">J/A+AS/107/353 : CP stars (Lopez-Garcia+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/125/219">J/A+AS/125/219 : Abundances of mu Lep, 7 Sex, HR 4817, 28 Her (Adelman+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/137/227">J/A+AS/137/227 : HD 133029 &amp; HD 192913 abundances (Lopez-Garcia+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/354/899">J/A+A/354/899 : Elemental abundance analyses. IV. (Adelman+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/316/514">J/MNRAS/316/514 : 28 And &amp; 99 Her elemental abundances (Adelman+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/367/597">J/A+A/367/597 : ups Her, phi Her &amp; HR 7018 abundances (Adelman+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/367/859">J/A+A/367/859 : {alpha} Scl and HD 170973 abundances (Lopez-Garcia+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/394/187">J/A+A/394/187 : {gamma} Ser &amp; 101 Her elemental abundances (Caliskan+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/406/975">J/A+A/406/975 : theta And, eps Del, eps Aqr, iota And (Kocer+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/406/987">J/A+A/406/987 : xi Oct, alpha Sex, 68 Tau elemental abund. (Pintado+, 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/A+AS/129/563</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/129/563</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/129/563</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/129/563</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/129/563</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/129/563</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/A+AS/129/563/abund</name><description>Atomic abundances</description><column><name>Ion</name><description>Ion</description><ucd>phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType><flag>primary</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>Name</name><description>Star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Nline</name><description>Number of lines</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Element</name><description>Element (identical to bytes 9-10)</description><ucd>phys.atmol.element</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>log(Nel/Ntot)</name><description>Derived abundance of Element (ratio of number of atoms to the total number of atoms per unit volume)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log(Nel/Ntot)</name><description>? rms uncertainty on log(Nel/Ntot)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_e_log(Nel/Ntot)</name><description>Uncertainty flag on e_log(Nel/Ntot)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/A+AS/129/563/table3</name><description>Elemental abundances of HR 4487, 14 Hya, and 3 Cen A</description><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>Name</name><description>Star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Ion</name><description>Ion</description><ucd>phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType><flag>primary</flag></column><column><name>Mult</name><description>? 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Equivalent width</description><unit>0.0001nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>log(N/Ntot)</name><description>Derived abundance in relative number of atoms</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>