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<ri:Resource created="2024-02-23T09:25:17Z" 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>Surface line identifications for HD 99803A</title><shortName>J/AJ/166/54</shortName><identifier>ivo://CDS.VizieR/J/AJ/166/54</identifier><altIdentifier>doi:10.26093/cds/vizier.51660054</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Monier R.</name></creator><creator><name>Niemczura E.</name></creator><creator><name>Kurtz D.W.</name></creator><creator><name>Rappaport S.</name></creator><creator><name>Bowman D.M.,Murphy S.J.</name></creator><creator><name>Lebreton Y.</name></creator><creator><name>Stuik R.</name></creator><creator><name>Deal M.</name></creator><creator><name>Merle T.</name></creator><creator><name>Kilicoglu T.,Gebran M.</name></creator><creator><name>Le Ster E.</name></creator><date role="Updated">2024-11-06T20:18:50Z</date><date role="Created">2024-02-23T09:25:17Z</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>multiple-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>chemical-abundances</subject><subject>spectral-energy-distribution</subject><description>We report on a detailed abundance study of six bright, mostly southern, slowly rotating late B-stars: HD1279 (B8III), HD99803 (B9V), HD123445 (B9V), HD147550 (B9V), HD171961 (B8III), and HD202671 (B5II/III), hitherto reported as normal stars. We compare them to the two classical HgMn stars {mu}Lep and {beta}Scl, and to the superficially normal star {nu}Cap. In the spectra of the six stars, the HgII line at 3984{AA} line is clearly seen and numerous lines of P, Ti, Mn, Fe, Ga, Sr, Y, and Zr appear to be strong absorbers. A comparison of newly acquired and archival spectra of these objects with a grid of synthetic spectra for selected unblended lines reveals large overabundances of P, Ti, Cr, Mn, Sr, Y, Zr, Ba, Pt, and Hg, and underabundances of He, Mg, Sc, and Ni. The effective temperatures, surface gravities, low projected rotational velocities, and the peculiar abundance patterns of the six investigated stars show that they are new chemically peculiar stars, mostly new HgMn stars, and are reclassified as such. The evolutionary status of these stars has been inferred, and their ages and masses estimated. The two most massive objects, HD1279 and HD202671, might have evolved away from the main sequence recently, the other stars are main-sequence objects. HD99803A is a sharp lined HgMn star with grazing eclipses. From TESS and MASCARA photometry, we determine an orbital period of Porb=26.12022{+/-}0.00004day.</description><source format="bibcode">2023AJ....166...54M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/54</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/III/117">III/117 : MK Classifications of Close Visual Binaries (Corbally, 1984)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/215">II/215 : uvby-beta Catalogue (Hauck+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/274/335">J/A+A/274/335 : Abundances in normal late-B and HgMn stars (Smith+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/107/1556">J/AJ/107/1556 : Late B-type stars classification (Garrison+, 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 &amp; 28 Her (Adelman+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/425/263">J/A+A/425/263 : Spectroscopic atlas of HD17564 (Castelli+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/162/227">J/ApJS/162/227 : Transition probabilities for SmII (Lawler+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/418/863">J/MNRAS/418/863 : NLTE corrections for Mg and Ca lines (Merle+ 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/537/A146">J/A+A/537/A146 : Stellar models with rot. 0.8&lt;M&lt;120, Z=0.014 (Ekstrom+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/158/157">J/AJ/158/157 : Fairly bright slow rotators compositions (Monier+, 2019)</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/AJ/166/54</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/166/54</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/166/54</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/166/54</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/166/54</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/166/54</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/AJ/166/54/table10</name><description>Line identifications for HD 99803A (HR 4423)</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>WaveObs</name><description>[3901/6682]? Observed wavelength, Angstroms</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>WaveLab</name><description>[3900/6681]? Laboratory wavelength, Angstroms</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Ion</name><description>Species identification</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>loggf</name><description>log, statistical weight*oscillator strength</description><ucd>stat.weight;phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Elow</name><description>[0/281124]? Energy, lower level</description><unit>eV</unit><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Flux</name><description>[0.13/0.99]? Relative Flux</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>