<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2001-05-04T21:43:08Z" 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>ups Her, phi Her &amp; HR 7018 abundances</title><shortName>J/A+A/367/597</shortName><identifier>ivo://CDS.VizieR/J/A+A/367/597</identifier><altIdentifier>doi:10.26093/cds/vizier.33670597</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Adelman S.J.</name></creator><creator><name>Gulliver A.F.</name></creator><creator><name>Rayle K.E.</name></creator><date role="Updated">2001-05-04T21:43:20Z</date><date role="Created">2001-05-04T21:43:08Z</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><subject>line-intensities</subject><description>Elemental abundances analyses are performed for the Mercury-Manganese stars {upsilon} Her, {phi} Her, and HR 7018 consistent with previous studies of this series using spectrograms obtained with Reticon and CCD detectors. Comparisons of the first two analyses with those performed using coadded photographic plates show the general consistency of the derived elemental abundances. For {upsilon} Her and for {phi} Her, abundances were newly found for O, and for Al, V, Zn, and Ce, respectively. HR 7018 is discovered to be a single-lined spectroscopic binary. Its Sc abundance is the smallest of any class member with derived abundances and its Sr abundance the largest of any known HgMn star. A correlation analysis of the most complete abundance sets for 20 HgMn stars shows that the abundances of some elements are correlated with one another and some are functions of the stellar effective temperature.</description><source format="bibcode">2001A&amp;A...367..597A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/367/597</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 : mu Lep, 7 Sex, HR 4817 &amp; 28 Her abundances (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/MNRAS/316/514">J/MNRAS/316/514 : 28 And + 99 Her elemental abundances (Adelman+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/371/1078">J/A+A/371/1078 : alpha Dra, tau Her, gamma Lyr, HR 7926 (Adelman+, 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+A/367/597</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/367/597</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/367/597</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/367/597</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/367/597</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/367/597</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/367/597/table6a</name><description>Elemental 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>Ion</name><description>Ion designation</description><ucd>phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Mult</name><description>Multiplet number from Moore (1945) if first line of multiplet, if not from Moore an initial indicating the paper (1)</description><ucd>phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>lambda</name><description>Laboratory wavelength (air)</description><unit>0.1nm</unit><ucd>em.wl;phys.atmol.transition</ucd><dataType xsi:type="vs:VOTableType">double</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 to oscillator strength (2)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>EW1</name><description>? Equivalent width for {upsilon} Her</description><unit>pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(N/Ntot)1</name><description>? Relative abundance value for {upsilon} Her</description><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EW2</name><description>? Equivalent width for {phi} Her</description><unit>pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(N/Ntot)2</name><description>? Relative abundance value for {phi} Her</description><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EW3</name><description>? Equivalent width for HR 7018</description><unit>pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(N/Ntot)3</name><description>? Relative abundance value for HR 7018</description><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/A+A/367/597/table6b</name><description>Relative 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>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>El</name><description>Element</description><ucd>phys.atmol.element</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>log(El/Ntot)1</name><description>? Elemental abundance for {upsilon} Her (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_log(El/Ntot)1</name><description>? rms uncertainty on log(El/Ntot)1</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(El/Ntot)2</name><description>? Elemental abundance for {phi} Her (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_log(El/Ntot)2</name><description>? rms uncertainty on log(El/Ntot)2</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(El/Ntot)3</name><description>? Elemental abundance for HR 7018 (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_log(El/Ntot)3</name><description>? rms uncertainty on log(El/Ntot)2</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>