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<ri:Resource created="2007-01-26T13:22:03Z" 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>Radial velocities of DW Car</title><shortName>J/A+A/461/1077</shortName><identifier>ivo://CDS.VizieR/J/A+A/461/1077</identifier><altIdentifier>doi:10.26093/cds/vizier.34611077</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Southworth J.</name></creator><creator><name>Clausen J.V.</name></creator><date role="Updated">2017-06-01T08:52:16Z</date><date role="Created">2007-01-26T13:22:03Z</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>spectroscopic-binary-stars</subject><subject>radial-velocity</subject><description>We have studied the high-mass short-period detached eclipsing binary DW Carinae using high-resolution echelle spectroscopy and photoelectric Stroemgren uvby light curves. We derived masses and radii accurate to 1% as well as the effective temperatures and reddening of the system. The high rotational velocities of the component stars meant that blending was a major problem when deriving radial velocities from the spectroscopy. Only helium lines provided good results, and a critique of different methods of measurement showed that spectral disentangling and fitting double Gaussians showed that these were the best able to provide reliable results in this case. The final spectroscopic orbit was calculated using spectral disentangling but we also provided radial velocities by fitting double Gaussians to the He-I 4472-A spectral line in each spectrum as this gives a good idea as to the quality of the data whilst providing a result very close to that adopted to calculate the masses. The light curves of DW Car are published as part of an accompanying paper (Clausen et al., 2006, Cat. &lt;J/A+A/461/1065&gt;).</description><source format="bibcode">2007A&amp;A...461.1077S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/461/1077</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+A/461/1065">J/A+A/461/1065 : uvby diff. photometry of 4 eclipsing binaries (Clausen+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/469/285">J/A+A/469/285 : Differential Stroemgren photometry of U Oph (Vaz+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/487/1095">J/A+A/487/1095 : Radial velocities of QD Boo, VZ Hya, WZ Oph (Clausen+, 2008)</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/461/1077</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/461/1077</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/461/1077</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/461/1077</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/461/1077</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/461/1077</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/461/1077/table1</name><description>Radial velocities for He 4471 line</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>HJD</name><description>Heliocentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Weight</name><description>Weight assigned for calculating orbits</description><ucd>stat.weight;phys.atmol.weight</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RV(A)</name><description>Measured radial velocity of star A</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RV(B)</name><description>Measured radial velocity of star B</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>res(A)</name><description>(O-C) residual from best-fit solution star A</description><unit>km/s</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>res(B)</name><description>(O-C) residual from best-fit solution star B</description><unit>km/s</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>