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<ri:Resource created="2024-01-29T07:18:55Z" 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>TESS photometry &amp; radial velocities for 6 K-binaries</title><shortName>J/AJ/165/259</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/259</identifier><altIdentifier>doi:10.26093/cds/vizier.51650259</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Liu N.-P.</name></creator><creator><name>Qian S.-B.</name></creator><creator><name>Liao W.-P.</name></creator><creator><name>Huang Y.</name></creator><creator><name>Yuan Z.-L.</name></creator><date role="Updated">2024-11-06T20:17:20Z</date><date role="Created">2024-01-29T07:18:55Z</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>k-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><description>High-precision light curves were extracted from TESScut images. Together with APOGEE and LAMOST medium-resolution spectra, a joint study was made for six early K-type contact binary candidates selected unbiasedly with orbital periods around 0.268 day. It is found that all of them (RV-CVn, EK-Com, V384-Ser, V1038-Her, EH-CVn, and CSS_J125403.7+503945) are W-subtype shallow contact systems, though with different mass ratios (1/q=0.27-0.62). The effective temperature differences between the binary components are around a few hundred kelvins. The original definitions of the A and W subtypes were compared with the customarily used methods, which rely on the shape or photometric solutions of the light curves. The latter two methods are not always reliable; therefore, the radial velocity analysis is strongly recommended. Through a collection of all available K-type contact binaries with both photometric and spectroscopic measurements, it is found that almost all of them are W-subtype systems, except for a few objects that have nearly identical temperatures for binary components. This W-subtype phenomenon for K-type contact binaries should be further checked with more samples in the future. Finally, the physical parameters of the targets were determined with joint data analysis, and the multiplicity is discussed for these targets. Objects V384-Ser and RV-CVn are confirmed to very likely be triple systems from comprehensive analysis, while V1038-Her is a candidate of a triple system based on photometric and spectroscopic solutions.</description><source format="bibcode">2023AJ....165..259L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/259</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/374/164">J/A+A/374/164 : BH Cas VRI differential magnitudes (Zola+, 2001)</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/other/PASA/23.154">J/other/PASA/23.154 : BV light curves XY Leo, EE Cet, AQ Psc (Djurasevic+ 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/1977">J/AJ/133/1977 : Radial velocities of 10 close binaries (Pribulla+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/465/943">J/A+A/465/943 : BVI and RV curves of 5 eclipsing binaries (Szalai+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/586">J/AJ/136/586 : Radial velocities of 10 close binaries (Rucinski+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/3655">J/AJ/137/3655 : Radial velocities of 8 close binaries (Pribulla+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/3646">J/AJ/137/3646 : Radial velocities of 10 close binaries (Pribulla+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/184">J/AJ/140/184 : RAVE double-lined spectroscopic binaries (Matijevic+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/723/1469">J/ApJ/723/1469 : Flux calibrations and WZ Oph photometry (Wilson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/412/1787">J/MNRAS/412/1787 : Physical parameters of 62 eclipsing binaries (Deb+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/525/A66">J/A+A/525/A66 : 4 close binaries BVR light curves (Djurasevic+, 2011)</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/ApJS/213/9">J/ApJS/213/9 : Catalina Surveys periodic variable stars (Drake+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/104">J/AJ/147/104 : Photometry &amp; velocities of 1SWASPJ093010A and B (Koo+, 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/147/130">J/AJ/147/130 : Minimum times of 7 eclipsing systems (Zasche+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/57">J/AJ/152/57 : VRI light curves of 4 contact binaries (Djurasevic+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/859/140">J/ApJ/859/140 : Multi-band magnitudes for W UMa EB* candidates (Chen+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/479/5491">J/MNRAS/479/5491 : Absolute parameters of 509 main-sequence stars (Eker+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/90">J/AJ/156/90 : Catalog of APOGEE radial velocity std stars (Huang+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/102">J/AJ/156/102 : TESS Input Catalog &amp; Candidate Target List (Stassun+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/158/106">J/AJ/158/106 : Eclips. binaries RVs from APOGEE spectra (Cunningham+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/871/63">J/ApJ/871/63 : How to constrain M dwarf. 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