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<ri:Resource created="2014-11-26T14:48:30Z" 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>Spectroscopy of HD 5980</title><shortName>J/AJ/148/62</shortName><identifier>ivo://CDS.VizieR/J/AJ/148/62</identifier><altIdentifier>doi:10.26093/cds/vizier.51480062</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Koenigsberger G.</name></creator><creator><name>Morrell N.</name></creator><creator><name>Hillier D.J.</name></creator><creator><name>Gamen R.</name></creator><creator><name>Schneider F.R.N.,Gonzalez-Jimenez N.</name></creator><creator><name>Langer N.</name></creator><creator><name>Barba R.</name></creator><date role="Updated">2017-07-05T06:59:39Z</date><date role="Created">2014-11-26T14:48:30Z</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>wolf-rayet-stars</subject><subject>eclipsing-binary-stars</subject><subject>radial-velocity</subject><description>New spectroscopic observations of the LBV/WR multiple system HD 5980 in the Small Magellanic Cloud are used to address the question of the masses and evolutionary status of the two very luminous stars in the 19.3 day eclipsing binary system. Two distinct components of the NV4944{AA} line are detected in emission and their radial velocity variations are used to derive masses of 61 and 66M_{sun}_, under the assumption that binary interaction effects on this atomic transition are negligible. We propose that this binary system is the product of quasi-chemically homogeneous evolution with little or no mass transfer. Thus, both of these binary stars may be candidates for gamma-ray burst progenitors or even pair instability supernovae. Analysis of the photospheric absorption lines belonging to the third-light object in the system confirm that it consists of an O-type star in a 96.56day eccentric orbit (e=0.82) around an unseen companion. The 5:1 period ratio and high eccentricities of the two binaries suggest that they may constitute a hierarchical quadruple system.</description><source format="bibcode">2014AJ....148...62K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/148/62</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/ApJ/745/173">J/ApJ/745/173 : UV absorption sight lines of LMC and SMC (Welty+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/28">J/AJ/143/28 : Analysis of B6-A9 stars from INES UV spectra (Freire+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/187/149">J/ApJS/187/149 : StarCAT: STIS UV echelle spectra of stars (Ayres, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/121/634">J/PASP/121/634 : FUSE observations in Magellanic Clouds (Blair+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/144/21">J/ApJS/144/21 : Galaxy and Magellanic Clouds OB and WR stars (Robert+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/366/508">J/A+A/366/508 : S Dor variables (van Genderen+, 2001)</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/148/62</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/148/62</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/148/62</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/148/62</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/148/62</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/148/62</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/148/62/spectra</name><description>Las Campanas Observatory (LCO) spectra</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>Disp</name><description>Simbad column added by the CDS</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Year</name><description>[2006/2013] Year of observation</description><unit>yr</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Tel</name><description>Telescope (Baade Mag 1, Clay Mag 2, DuPont) (1)</description><ucd>meta.id;instr.tel</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Inst</name><description>Instrument (IMACS, MagE=Magellan Echellette)</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>HJD</name><description>Heliocentric Julian Date (HJD-2450000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Phase</name><description>[0/1] Orbital phase (computed with P=19.26d)</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/148/62/vel_C</name><description>Radial velocity measurements for star C</description><column><name>HJD</name><description>Heliocentric Julian Date (HJD-2450000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</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>Inst</name><description>Simbad column added by the CDS</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Phase1</name><description>[0/1] Orbital phase computed with P=19.2654d</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Phase2</name><description>[0/1] Orbital phase computed with P=96.56d</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RV5592</name><description>[68/251]? Radial velocity obtained by fitting Gaussians to the core of the OIII{lambda}5592{AA} absorption line</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>u_RV5592</name><description>[:] Uncertainty flag on RV5592</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RV4471</name><description>[69/268]? Radial velocity obtained by fitting Gaussians to the core of the HeI{lambda}4471{AA} absorption line</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>u_RV4471</name><description>[:] Uncertainty flag on RV4471</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RV5875</name><description>[44/296]? 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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>HJD</name><description>Heliocentric Julian Date (HJD-2450000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Phase</name><description>[0/1] Orbital phase (computed with P=19.2654d)</description><ucd>time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RVA</name><description>[-98/399]? Primary radial velocity (1)</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RVB</name><description>[-142/344]? Secondary radial velocity (1)</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>