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<ri:Resource created="2014-05-23T13:49:02Z" 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>Initial masses of W UMa type contact binaries</title><shortName>J/MNRAS/430/2029</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/430/2029</identifier><altIdentifier>doi:10.26093/cds/vizier.74302029</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yildiz M.</name></creator><creator><name>Dogan T.</name></creator><date role="Updated">2024-07-21T20:14:06Z</date><date role="Created">2014-05-23T13:49:02Z</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>eclipsing-binary-stars</subject><subject>stellar-masses</subject><description>W UMa type binaries have two defining characteristics. These are (i) the effective temperatures of both components are very similar, and (ii) the secondary (currently less massive) component is overluminous for its current mass. We consider the latter to be an indication of its mass before the mass transfer event. For these stars, we define a mass difference ({delta}M) between the mass determined from its luminosity and the present mass determined from fitting the binary orbit. We compare the observed values of the mass difference to stellar models with mass-loss. The range of initial secondary masses that we find for observed W UMa type binaries is 1.3-2.6M_{sun}_. We discover that the A- and the W-subtype contact binaries have different ranges of initial secondary masses. Binary systems with an initial mass higher than 1.8+/-0.1M_{sun}_ become A-subtype while systems with initial masses lower than this become W-subtype. Only 6 per cent of systems violate this behaviour. We also obtain the initial masses of the primaries using the following constraint for the reciprocal of the initial mass ratio: 0&lt;1/q_i_&lt;1. The range of initial masses we find for the primaries is 0.2-1.5M_{sun}_, except for two systems. Finally in comparing our models to observed systems, we find evidence that the mass transfer process is not conservative. We find that only 34 per cent of the mass from the secondary is transferred to the primary. The remainder is lost from the system.</description><source format="bibcode">2013MNRAS.430.2029Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/430/2029</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/V/119">V/119 : Catalogue of field contact binary stars (Pribulla+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/120">V/120 : Catalog of early-type contact binaries (Bondarenko+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/108/332">J/PASP/108/332 : Photometric analysis of contact binaries (Lapasset+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/51/259">J/AcA/51/259 : Contact binaries in OGLE-I database (Szymanski+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/426/1001">J/A+A/426/1001 : Catalog of contact binary stars (Csizmadia+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/621">J/AJ/131/621 : Catalog of 1022 bright contact binary stars (Gettel+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/633">J/AJ/131/633 : A ROSAT survey of contact binary stars (Geske+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/2986">J/AJ/131/2986 : Multiplicity of contact binaries (Pribulla+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/56/253">J/AcA/56/253 : Period changes of OGLE contact binaries (Kubiak+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/373/1483">J/MNRAS/373/1483 : W UMa type and CAB stars dynamical evolution (Eker+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/2353">J/AJ/134/2353 : Observations of contact binaries (Rucinski+, 2007)</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/MNRAS/430/2029</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/430/2029</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/430/2029</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/430/2029</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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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>Star</name><description>Star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>Type</name><description>[AW] Contact binary subtype</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Per</name><description>[0.2/0.9] Orbital period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>T1</name><description>Effective temperature of primary</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_T1</name><description>? rms uncertainty on T1</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>T2</name><description>Effective temperature of secondary</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_T2</name><description>? 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