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<ri:Resource created="2018-01-11T11:56:41Z" status="active" updated="2026-03-17T20:05:37Z" 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>First analysis of the binary IK Boo</title><shortName>J/PASJ/69/62</shortName><identifier>ivo://CDS.VizieR/J/PASJ/69/62</identifier><altIdentifier>doi:10.26093/cds/vizier/bj-25-1y</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kriwattanawong W.</name></creator><creator><name>Sanguansak N.</name></creator><creator><name>MaungKorn S.</name></creator><date role="Updated">2026-03-17T20:05:37Z</date><date role="Created">2018-01-11T11:56:41Z</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>ephemerides</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>With new CCD observations of the W UMa type binary IK Boo, we present the first investigation of photometric parameters and orbital period change. The BVRc light curve fit shows that IK Boo is a W-type contact system with a mass ratio of q=1.146 and a shallow contact with a fill-out factor of f=2.22%. The orbital period decrease is found at a rate of -3.28x10^-7^d/yr, corresponding to a mass transfer from the more massive to the less massive component with a rate of -2.83x10^-6^M_{sun}/yr. The inner and outer critical Roche lobes will contract and cause the contact degree to increase. Therefore, IK Boo may evolve into a deeper contact system. Furthermore, a possible cyclic variation is found to have a period of 9.74yr, that could be explained by the light-travel time effect, due to the existence of a third companion in the system.</description><source format="bibcode">2017PASJ...69...62K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASJ/69/62</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/J/A+A/311/523">J/A+A/311/523 : Photometry of W UMa (Maceroni+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/336/920">J/A+A/336/920 : HD 163151: a new W UMa type system (Rodriguez+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/357/497">J/MNRAS/357/497 : Kinematics of W UMa-type binaries (Bilir+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/99">J/AJ/143/99 : Photometry of W UMa eclipsing binaries (Terrell+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/149">J/AJ/144/149 : CCD photometry of W UMa type TY Boo (Christopoulou+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/70">J/AJ/146/70 : Spectroscopy of W UMa-type binary stars (Rucinski+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/430/2029">J/MNRAS/430/2029 : Initial masses of W UMa type contact binaries (Yildiz+ 2013)</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></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/PASJ/69/62</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASJ/69/62</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASJ/69/62</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/PASJ/69/62</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/PASJ/69/62</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/PASJ/69/62</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/PASJ/69/62/table1</name><description>Times of minimum light for IK Boo</description><column><name>Min</name><description>Types of minimum</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">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>HJD</name><description>Heliocentric Julian date at light minimum</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ref</name><description>References for the sources</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>E</name><description>Epoch</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>O-C</name><description>O-C</description><unit>d</unit><ucd>time;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/PASJ/69/62/table5</name><description>CCD photometric observations in BVRc filter bands for IK Boo</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>Heliocentric Julian date of B band observation (HJD-2457000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dBmag</name><description>Differential B band magnitude</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>Heliocentric Julian date of V band observation (HJD-2457000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dVmag</name><description>Differential V band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HJD-Rc</name><description>Heliocentric Julian date of Rc band observation (HJD-2457000)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dRcmag</name><description>Differential Rc band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>