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<ri:Resource created="2019-07-05T08:07:23Z" 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>Study of three early-type contact twin binaries</title><shortName>J/AJ/157/111</shortName><identifier>ivo://CDS.VizieR/J/AJ/157/111</identifier><altIdentifier>doi:10.26093/cds/vizier.51570111</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yang Y.</name></creator><creator><name>Yuan H.</name></creator><creator><name>Dai H.</name></creator><date role="Updated">2019-07-15T11:28:16Z</date><date role="Created">2019-07-05T08:07:23Z</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>early-type-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-astronomy</subject><description>Three eclipsing binaries, CT Tau, GU Mon, and V701 Sco, are early-type contact binaries with infrared excess from circumbinary matter. We present the multi-color photometry for CT Tau and GU Mon, whose spectral types of B1V are identified by the low-precision spectra. Combining these new light curves (LCs) with previously reported LCs and radial velocity curves, we perform a synthesized analysis to estimate/update the stellar absolute parameters of the three systems. Their mass ratios are close to unity (i.e., q~1), which indicates that the binary system comprising of twin components may be undergoing a slow Case A mass transfer. From the period analysis, the light-time orbit in the (O-C) curve may result from the third condense companion around the binary system although no evidence could be provided by the third light l_3_. From the spectral energy distribution for three binaries, the excess infrared (IR) emissions are above the photospheric emissions, which can be seen at the 22.1 {mu}m for CT Tau and GU Mon, and 11.6 {mu}m, 14.5 {mu}m, and 22.1 {mu}m for V701 Sco, respectively. This kind of infrared excess for the early-type star may be attributed to the circumbinary matter by stellar wind.</description><source format="bibcode">2019AJ....157..111Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/157/111</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/V/120">V/120 : Catalog of early-type contact binaries (Bondarenko+, 1996)</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/A+A/590/A45">J/A+A/590/A45 : GU Mon BV light curves (Lorenzo+, 2016)</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/157/111</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/157/111</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/157/111</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/157/111</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/157/111</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/157/111</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><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/157/111/table4</name><description>All available light minimum times for three eclipsing binaries</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>Star</name><description>Stellar identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>HJD</name><description>[2427688.268/2458082.4029] Heliocentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_HJD</name><description>[0.0001/0.042]? Uncertainty in HJD</description><unit>d</unit><ucd>stat.error;time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Meth</name><description>Detection method (1)</description><ucd>meta.code;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Epoch</name><description>[-28450/15789.5] Epoch number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Type</name><description>[I] Eclipse type</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>(O-C)i</name><description>[-0.1566/0.0992] Initial residuals (2)</description><unit>d</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>(O-C)f</name><description>[-0.1672/0.0431]? Final residuals</description><unit>d</unit><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_(O-C)f</name><description>[d] Indicates the (O-C)f is discarded</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/AJ/157/111/table6</name><description>Measured fluxes for the three eclipsing binaries</description><column><name>Band</name><description>Band</description><ucd>instr.bandpass</ucd></column><column><name>Star</name><description>Stellar identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</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>lambda</name><description>[0.353/22.1] Wavelength {lambda}</description><unit>um</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux</name><description>[0.184/149] Flux density</description><unit>0.01Jy</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Flux</name><description>[0.014/5.1]? 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