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<ri:Resource created="1998-05-02T16:55:05Z" 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>G and K dwarfs abundances</title><shortName>J/A+AS/129/237</shortName><identifier>ivo://CDS.VizieR/J/A+AS/129/237</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Feltzing S.</name></creator><creator><name>Gustafsson B.</name></creator><date role="Updated">1998-05-02T16:57:22Z</date><date role="Created">1998-05-02T16:55:05Z</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>dwarf-stars</subject><description>The table presents the abundances of all 47 dwarf stars analysed in the paper. We give abundances relative to the Sun in the standard notation of [X/H]=log(X/H)_star_-log(X/H)_{sun}_. The 5 K dwarf stars and 3 stars in common with Barbuy &amp; Grenon (1990) appear at the end of the table. The label of each column indicates the ion the quoted abundances are derived from. For each star we give the abundance, [X/H], the line-to-line scatter (if more than one line is used) and the number of lines used. The stars are ordered in the same way as in Table 1 in the paper, ie. the K dwarf stars and the stars in common with Barbuy &amp; Grenon (1990) are found at the end.</description><source format="bibcode">1998A&amp;AS..129..237F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/129/237</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+AS/102/603">J/A+AS/102/603 : Chemical evolution of the galactic disk II. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HD</name><description>HD (Cat. &lt;III/135&gt;) number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType><flag>primary</flag></column><column><name>m_HD</name><description>Multiplicity index on HD</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Ion</name><description>Ion designation</description><ucd>phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>[X/H]</name><description>? Abundance (log(X/H)_star-log(X/H)_{sun}_)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Sc</name><description>? 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