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<ri:Resource created="2022-12-13T09:18:27Z" 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>Extremely Low Mass Ratio Contact Binaries I. 10 systems</title><shortName>J/AJ/164/202</shortName><identifier>ivo://CDS.VizieR/J/AJ/164/202</identifier><altIdentifier>doi:10.26093/cds/vizier.51640202</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Li K.</name></creator><creator><name>Gao X.</name></creator><creator><name>Liu X.-Y.</name></creator><creator><name>Gao X.</name></creator><creator><name>Li L.-Z.</name></creator><creator><name>Chen Xu</name></creator><creator><name>Sun G.-Y.</name></creator><date role="Updated">2023-03-20T14:35:40Z</date><date role="Created">2022-12-13T09:18:27Z</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>visible-astronomy</subject><subject>spectroscopy</subject><description>The photometric and spectroscopic investigations of ten contact binaries were presented for the first time. It is discovered that the mass ratios of all the ten targets are smaller than 0.15, they are extremely low mass ratio contact binaries. Seven of them are deep contact binaries, two are medium contact binaries, while only one is a shallow contact system. Five of them show the O'Connell effect, and a dark spot on one of the two components can lead to a good fit of the asymmetric light curves. The orbital period studies of the ten binaries reveal that they all exhibit long-term period changes, six of them are increasing, while the others are shrinking. The LAMOST spectra were analyzed by the spectral subtraction method, and all the ten targets exhibit excess emissions in the H{alpha} line, indicating chromospheric activity. The evolutionary states of the two components of the ten binaries were studied, and it is found that their evolutionary states are identical to those of the other contact binaries. Based on the study of the relation between orbital angular momentum and total mass, we discovered the ten systems may be at the late evolutionary stage of a contact binary. The initial masses of the two components and the ages of them were obtained. By calculating the instability parameters, we found that the ten contact binaries are relatively stable at present.</description><source format="bibcode">2022AJ....164..202L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/164/202</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/366">II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)</relatedResource><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/146">V/146 : LAMOST DR1 catalogs (Luo+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/106/2096">J/AJ/106/2096 : Limb-darkening coefficients in binaries (Van Hamme 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/629/1055">J/ApJ/629/1055 : Evolution of close binary systems (Yakut+, 2005)</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/ApJ/696/870">J/ApJ/696/870 : Catalina Real-time Transient Survey (CRTS) (Drake+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/494/209">J/A+A/494/209 : Pre-main sequence evolutionary tracks (Landin+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/RAA/11.924">J/other/RAA/11.924 : Atmospheric parameters for 771 stars (Wu+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/157">J/AJ/146/157 : Differential BVRI photometry of FI Boo (Christopoulou+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/430/2029">J/MNRAS/430/2029 : Initial masses of WUMa type contact binaries (Yildiz+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/788/48">J/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/437/185">J/MNRAS/437/185 : W UMa-type contact binaries ages and masses (Yildiz, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/157/207">J/AJ/157/207 : BVR_c_I_c_ light curve observations for VZ Lib (Liao+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/244/43">J/ApJS/244/43 : Binary stars parameters LAMOST &amp; Kepler obs. (Zhang+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/159/189">J/AJ/159/189 : Eclipse timings for 9 contact binaries (Li+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/162/13">J/AJ/162/13 : Parameters estimation for 173 eclipsing binaries (Li+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/221">J/AJ/161/221 : Photometry &amp; spectroscopy of 4 binaries stars (Panchal+, 2021)</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/164/202</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/164/202</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/164/202</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/164/202</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/164/202</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/164/202</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/164/202/table1 (Information of the 10 systems from ASAS-SN database)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/164/202/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/164/202/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/164/202/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>3.5937958</ra><dec>41.8920164</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/1266 1916 2332 2726 4947 5962 6742 8480 20046 27708</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/164/202?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/164/202/table1</name><description>Information of the 10 systems from ASAS-SN database</description><column><name>ASAS</name><description>ASAS-SN Name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="28*">char</dataType></column><column><name>OName</name><description>Other name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="26*">char</dataType></column><column><name>ID</name><description>Identifier in this work</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType><flag>primary</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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