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<ri:Resource created="2022-02-21T12:22:32Z" 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>Photometric obs. &amp; LAMOST sp. of 4 W UMa binaries</title><shortName>J/ApJ/901/169</shortName><identifier>ivo://CDS.VizieR/J/ApJ/901/169</identifier><altIdentifier>doi:10.26093/cds/vizier.19010169</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lu H.-P.</name></creator><creator><name>Zhang L.-Y.</name></creator><creator><name>Michel R.</name></creator><creator><name>Han X.L.</name></creator><date role="Updated">2022-09-30T21:34:27Z</date><date role="Created">2022-02-21T12:22:32Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>spectroscopy</subject><subject>metallicity</subject><subject>astronomical-reference-materials</subject><description>We present new photometric data and LAMOST spectra for the W UMa binaries UV Lyn, V781 Tau, NSVS 4484038, and 2MASS J15471055+5302107. The orbital and starspot parameters are obtained using the Wilson-Devinney program. Comparing the starspot parameters at different times, there are magnetic activities in these four binaries. The orbital period of UV Lyn is increasing at a rate of dP/dt=+8.9(5)x10^-8^d/yr, which maybe due to mass transfer from the less massive component to the more massive component (dM1/dt=-6.4x10^-8^M_{sun}_/yr). The period variation of 2MASSJ15471055+5302107 is also increasing at a rate of 6.0(4)x10^-7^d/yr, which can be explained by mass transfer from the less massive component to the more massive component (dM1/dt=-2.8x10^-7^M_{sun}_/yr). The period variation of V781 Tau presents the downward parabola superimposed the cyclic oscillation. The period of V781 Tau is decreasing (dP/dt=-3.2(4)x10^-8^d/yr), which can be explained by mass transfer from the more massive component to the less massive component (dM2/dt=-2.2x10^-8^M_{sun}_/yr). The cyclic oscillation may be due to the magnetic activity with a period of 30.8(5)yr rather than a third body. The period variation of NSVS4484038 also shows the cyclic oscillation, which could be explained by the magnetic activity with 10.8(1)yr or a black hole candidate. Interestingly, there is a depth variation between the light minimum times of NSVS 4484038, which may also be caused by stellar magnetic activity.</description><source format="bibcode">2020ApJ...901..169L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/901/169</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/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/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/other/IBVS/5438">J/other/IBVS/5438 : 162-nd list of minima of EBs (Diethelm, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/5493">J/other/IBVS/5493 : 2003 CCD minima of eclipsing binaries (Nelson+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/426">J/AJ/128/426 : Subdwarfs in the SDSS (West+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/429/309">J/A+A/429/309 : HR 1099 radial velocities (Frasca+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/5592">J/other/IBVS/5592 : Eclipsing binary stars photoelectric minima (Krajci+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/372/1117">J/MNRAS/372/1117 : SuperWASP exoplanetary transit survey (Christian+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/5731">J/other/IBVS/5731 : Minima and maxima of 816 variables (Hubscher+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/452/959">J/A+A/452/959 : BV light curve of V781 Tau (Kallrath+, 2006)</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/AJ/134/2398">J/AJ/134/2398 : Stellar SEDs in SDSS and 2MASS filters (Covey+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/5761">J/other/IBVS/5761 : Minima and maxima of 389 variables (Hubscher+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/467/785">J/A+A/467/785 : SuperWASP/ROSAT periodic variable stars (Norton+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/1089">J/AJ/136/1089 : UBVRI light curves of TU Boo (Coughlin+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/466">J/AJ/138/466 : NSVS variables automated classification (Hoffman+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/5889">J/other/IBVS/5889 : Minima and maxima of 380 variables (Hubscher+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/99">J/AJ/142/99 : BVRI observations of TZ Boo (Christopoulou+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/5984">J/other/IBVS/5984 : Minima and maxima of 503 variables (Hubscher, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/IBVS/5959">J/other/IBVS/5959 : Minima and maxima of 436 variables (Huebscher+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/97">J/AJ/141/97 : SDSS DR7 M dwarfs (West+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/79">J/AJ/146/79 : Differential BVRI light curves of EP And (Liao+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A86">J/A+A/549/A86 : Period change for 143 SuperWASP EBs (Lohr+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/66">J/AJ/147/66 : LCs of Algol-type binaries. 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Logg uncertainty</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]</name><description>[0.05/0.4]? Log of Fe/H abundance</description><unit>log(Sun)</unit><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Fe/H]</name><description>[0.01/0.1]? Fe/H uncertainty</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWHa</name><description>[-1.6/-0.34]? H{alpha} equivalent width in Angstrom units</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_EWHa</name><description>[0.02/2]? 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