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<ri:Resource created="2014-12-10T15:20:00Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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 velocity curves of LMC ellipsoidal variables</title><shortName>J/AJ/148/118</shortName><identifier>ivo://CDS.VizieR/J/AJ/148/118</identifier><altIdentifier>doi:10.26093/cds/vizier.51480118</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Nie J.D.</name></creator><creator><name>Wood P.R.</name></creator><date role="Updated">2017-09-22T16:16:15Z</date><date role="Created">2014-12-10T15:20:00Z</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>magellanic-clouds</subject><subject>multiple-stars</subject><subject>giant-stars</subject><subject>radial-velocity</subject><description>Ellipsoidal red giant binaries are close binary systems where an unseen, relatively close companion distorts the red giant, leading to light variations as the red giant moves around its orbit. These binaries are likely to be the immediate evolutionary precursors of close binary planetary nebula and post-asymptotic giant branch and post-red giant branch stars. Due to the MACHO and OGLE photometric monitoring projects, the light variability nature of these ellipsoidal variables has been well studied. However, due to the lack of radial velocity curves, the nature of their masses, separations, and other orbital details has so far remained largely unknown. In order to improve this situation, we have carried out spectral monitoring observations of a large sample of 80 ellipsoidal variables in the Large Magellanic Cloud and we have derived radial velocity curves. At least 12 radial velocity points with good quality were obtained for most of the ellipsoidal variables. The radial velocity data are provided with this paper. Combining the photometric and radial velocity data, we present some statistical results related to the binary properties of these ellipsoidal variables.</description><source format="bibcode">2014AJ....148..118N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/148/118</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/247">II/247 : Variable Stars in the Large Magellanic Clouds (MACHO, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/244">I/244 : OGLE General Catalog of Stars. I. (Szymanski+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/421/2616">J/MNRAS/421/2616 : LMC eccentric ellipsoidal red giant binaries</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/405/1770">J/MNRAS/405/1770 : LMC red giants in E sequence (Nicholls+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/399/2063">J/MNRAS/399/2063 : LMC red giants in D sequence (Nicholls+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/1242">J/AJ/136/1242 : LMC long-period variables from MACHO (Fraser+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/439/559">J/A+A/439/559 : OGLE eclipsing binaries (Groenewegen+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/353/705">J/MNRAS/353/705 : OGLE Variables in Magellanic Clouds (Ita+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/348/1439">J/MNRAS/348/1439 : OGLE II Galactic center proper motions (Sumi+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/53/1">J/AcA/53/1 : OGLE eclipsing binaries in LMC (Wyrzykowski+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/52/129">J/AcA/52/129 : DIA OGLE2 candidate variable stars catalog (Wozniak+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/49/223">J/AcA/49/223 : BVI photometry of OGLE LMC Cepheids (Udalski+, 1999)</relatedResource><relatedResource>http://macho.anu.edu.au/ : MACHO Home Page</relatedResource><relatedResource>http://ogle.astrouw.edu.pl/ : OGLE Home Page</relatedResource><relatedResource>ftp://ftp.astrouw.edu.pl/ogle/ogle2 : OGLE-II</relatedResource><relatedResource>ftp://ftp.astrouw.edu.pl/ogle/ogle3 : OGLE-III</relatedResource><relatedResource>ftp://ftp.astrouw.edu.pl/ogle/ogle4 : OGLE-IV</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/148/118</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/148/118</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/148/118</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/148/118</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/148/118</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/148/118</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/148/118/table2 (Properties of the observed ellipsoidal variables)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/148/118/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/148/118/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/148/118/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>75.2795</ra><dec>-69.3435833</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/8274 6/33053 33055 33077 33089 33090 33091 33120 33121</spatial><spectral>8.650015785639275e-20 4.920466254354166e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/148/118?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/148/118/table1</name><description>Radial velocities Vr and 1{sigma} errors {sigma}_Vr_ in km/s</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Full radial velocity amplitude</description><unit>km/s</unit><ucd>phys.veloc;src.orbital</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Lum</name><description>Luminosity</description><unit>solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Teff</name><description>Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>&lt;Rad&gt;</name><description>[40/156] Mean radius</description><unit>solRad</unit><ucd>phys.size.radius;stat.mean</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Loc</name><description>[1/2] Location of the star on the Imag-logPeriod and W-logPeriod planes (Figure1 in the paper) (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LC</name><description>Object which has OGLE III light curve data</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>S04</name><description>Display the data from Soszynski et al. 2004 (cat. 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