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<ri:Resource created="2016-01-19T08:15:28Z" 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>V471 Tau system: RVs and BVRI LCs</title><shortName>J/ApJ/810/157</shortName><identifier>ivo://CDS.VizieR/J/ApJ/810/157</identifier><altIdentifier>doi:10.26093/cds/vizier.18100157</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Vaccaro T.R.</name></creator><creator><name>Wilson R.E.</name></creator><creator><name>Van Hamme W.</name></creator><creator><name>Terrell D.</name></creator><date role="Updated">2017-06-12T08:25:08Z</date><date role="Created">2016-01-19T08:15:28Z</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>radial-velocity</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>V471 Tauri, a white dwarf-red dwarf eclipsing binary (EB) in the Hyades, is well known for stimulating development of common envelope theory, whereby novae and other cataclysmic variables form from much wider binaries by catastrophic orbit shrinkage. Our evaluation of a recent imaging search that reported negative results for a much postulated third body shows that the object could have escaped detection or may have actually been seen. The balance of evidence continues to favor a brown dwarf companion about 12 AU from the EB. A recently developed algorithm finds unified solutions from three data types. New radial velocities (RVs) of the red dwarf and BVRcIc light curves are solved simultaneously along with white dwarf and red dwarf RVs from the literature, uvby data, the Microvariability and Oscillations of Stars mission light curve, and 40 years of eclipse timings. Precision-based weighting is the key to proper information balance among the various data sets. Timewise variation of modeled starspots allows unified solution of multiple data eras. Light-curve amplitudes strongly suggest decreasing spottedness from 1976 to about 1980, followed by approximately constant spot coverage from 1981 to 2005. An explanation is proposed for lack of noticeable variation in 1981 light curves, in terms of competition between spot and tidal variations. Photometric-spectroscopic distance is estimated. The red dwarf mass comes out larger than normal for a K2 V star, and even larger than adopted in several structure and evolution papers. An identified cause for this result is that much improved red dwarf RV curves now exist.</description><source format="bibcode">2015ApJ...810..157V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/810/157</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/B/vsx">B/vsx : AAVSO International Variable Star Index VSX (Watson+, 2006-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/sb9">B/sb9 : 9th Catalogue of Spectroscopic Binary Orbits (Pourbaix+ 2004-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/gcvs">B/gcvs : General Catalogue of Variable Stars (Samus+ 2007-2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/559/A43">J/A+A/559/A43 : Pan-STARRS1 (PS1) observations of the Hyades (Goldman+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/187/149">J/ApJS/187/149 : StarCAT: STIS UV echelle spectra of stars (Ayres, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/A+ARV/17.251">J/other/A+ARV/17.251 : Stars observed with Doppler imaging (Strassmeier, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/5802">J/other/IBVS/5802 : Minima and maxima of 735 variables (Hubscher+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/2353">J/AJ/134/2353 : Observations of contact binaries (Rucinski+, 2007)</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/A+A/446/785">J/A+A/446/785 : Catalogue of eclipsing variables (Malkov+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/54/207">J/AcA/54/207 : Ephemerids of eclipsing binaries (Kreiner, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/349/1069">J/MNRAS/349/1069 : Chromospherically active binaries (Karatas+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/381/446">J/A+A/381/446 : Astrometric Radial Velocities. III. (Madsen+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/367/111">J/A+A/367/111 : A Hipparcos study of the Hyades cluster (de Bruijne+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/281/811">J/A+A/281/811 : Long-term variations in V471 Tau (Ibanoglu+ 1994)</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/ApJ/810/157</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/810/157</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/810/157</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/810/157</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/810/157</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/810/157</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>Infrared</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/810/157/table1</name><description>Red dwarf 1998 radial velocities (RVs)</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>HJD</name><description>Heliocentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>HJED</name><description>Heliocentric Julian Ephemeris Date</description><unit>d</unit><ucd>time.epoch;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RV</name><description>[-122/187] Radial Velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RV</name><description>[1/5] Individual RV standard error</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/810/157/table2</name><description>B, V, R_c_, I_c_ 1998 light curves (LCs)</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>HJD(B)</name><description>B band Heliocentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>HJED(B)</name><description>B band Heliocentric Julian Ephemeris Date (1)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dBmag</name><description>[-0.5/-0.2] Differential B magnitude (2)</description><unit>mag</unit><ucd>phot.mag;em.opt.B;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HJD(V)</name><description>V band Heliocentric Julian Date</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>HJED(V)</name><description>V band Heliocentric Julian Ephemeris Date (1)</description><unit>d</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dVmag</name><description>[-0.2/0.02]? 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