<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2003-08-22T09:18:07Z" status="active" updated="2025-06-13T15:25:00Z" 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>Elemental abundances of four A-B stars</title><shortName>J/A+A/406/975</shortName><identifier>ivo://CDS.VizieR/J/A+A/406/975</identifier><altIdentifier>doi:10.26093/cds/vizier.34060975</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kocer D.</name></creator><creator><name>Adelman S.J.</name></creator><creator><name>Caliskan H.</name></creator><creator><name>Gulliver A.F.</name></creator><creator><name>Tektunali. G.H.</name></creator><date role="Updated">2003-08-22T09:18:56Z</date><date role="Created">2003-08-22T09:18:07Z</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>The superficially normal stars {theta} And (A2 V), {epsilon} Del (B6 III), {epsilon} Aqr (A1.5 V), and {iota} And (B9 V), which have rotationally broadened line profiles, are analyzed in a manner consistent with previous studies of this series using 2.4{AA}/mm spectrograms obtained with CCD detectors and S=N&gt;=200. Their variable radial velocities strongly suggest they are spectroscopic binaries. As no evidence is seen for lines of their companions they are analyzed as single stars. Their derived abundances are generally near solar. But those for {theta} And suggest that it is possibly a fast rotating Am star.</description><source format="bibcode">2003A&amp;A...406..975K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/406/975</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/129/563">J/A+AS/129/563 : Abundances of HR 4487, 14 Hyd and 3 Cen A (Pintado+ 1998)</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/406/987">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+A/406/975</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/406/975</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/406/975</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/406/975</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/406/975</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/406/975</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+A/406/975/table5</name><description>Abundances in {theta} And, {epsilon} Del, {epsilon} Aqr, and {iota} And</description><column><name>Mult</name><description>Multiplet number</description><ucd>phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></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>Ion</name><description>Ion designation</description><ucd>phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">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>loggf</name><description>Oscillator strength</description><ucd>phys.atmol.wOscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_loggf</name><description>Reference for loggf (2)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>EW1</name><description>? {theta} And equivalent width</description><unit>nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(El/Ntot)1</name><description>? {theta} And elemental abundance (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_log(El/Ntot)1</name><description>Uncertainty flag on log(ElN/Ntot)1</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>EW2</name><description>? {epsilon} Del equivalent width</description><unit>nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(El/Ntot)2</name><description>? {epsilon} Del elemental abundance (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EW3</name><description>? {epsilon} Aqr equivalent width</description><unit>nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(El/Ntot)3</name><description>? {epsilon} Aqr elemental abundance (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_log(El/Ntot)3</name><description>Uncertainty flag on log(El/Ntot)3</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>EW4</name><description>? {iota} And equivalent width</description><unit>nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(El/Ntot)4</name><description>? {iota} And elemental abundance (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/A+A/406/975/table6</name><description>Comparison of Derived and Solar Abundances as logN/H Species</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>Ion</name><description>Ion</description><ucd>phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>logEl/H2</name><description>? {epsilon} Del derived abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logEl/H2</name><description>? rms uncertainty on logEl/H2</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logEl/H4</name><description>? {iota} And derived abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logEl/H4</name><description>? rms uncertainty on logEl/H4</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logEl/H3</name><description>? {epsilon} Aqr derived abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_logEl/H3</name><description>Uncertainty flag on logEl/H3</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>e_logEl/H3</name><description>? rms uncertainty on logEl/H3</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logEl/H1</name><description>? {theta} And derived abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_logEl/H1</name><description>Uncertainty flag on logEl/H1</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>e_logEl/H1</name><description>? rms uncertainty on logEl/H1</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logEl/HS</name><description>Sun abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/406/975/abund</name><description>Atomic abundances</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>log(Nel/H)</name><description>Derived abundance of Element</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>u_log(Nel/H)</name><description>Uncertainty flag on log(Nel/H)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>e_log(Nel/H)</name><description>? rms uncertainty on log(Nel/H)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>