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<ri:Resource created="2020-07-20T06:44:24Z" 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>Late-type contact binaries in CSS DR1</title><shortName>J/ApJS/247/50</shortName><identifier>ivo://CDS.VizieR/J/ApJS/247/50</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sun W.</name></creator><creator><name>Chen X.</name></creator><creator><name>Deng L.</name></creator><creator><name>de Grijs R.</name></creator><date role="Updated">2021-09-07T07:03:43Z</date><date role="Created">2020-07-20T06:44:24Z</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>stellar-masses</subject><subject>effective-temperature</subject><subject>stellar-radii</subject><subject>visible-astronomy</subject><description>We present the physical parameters of 2335 late-type contact binary (CB) systems extracted from the Catalina Sky Survey (CSS). Our sample was selected from the CSS Data Release 1 by strictly limiting the prevailing temperature uncertainties and light-curve fitting residuals, allowing us to almost eliminate any possible contaminants. We developed an automatic Wilson-Devinney-type code to derive the relative properties of CBs based on their light-curve morphology. By adopting the distances derived from CB (orbital) period-luminosity relations (PLRs), combined with the well-defined mass-luminosity relation for the systems' primary stars and assuming solar metallicity, we calculated the objects' masses, radii, and luminosities. Our sample of fully eclipsing CBs contains 1530 W-, 710 A-, and 95 B-type CBs. A comparison with literature data and with the results from different surveys confirms the accuracy and coherence of our measurements. The period distributions of the various CB subtypes are different, hinting at a possible evolutionary sequence. W-type CBs are clearly located in a strip in the total mass versus mass-ratio plane, while A-type CBs may exhibit a slightly different dependence. There are no significant differences among the PLRs of A- and W-type CBs, but the PLR zero-points are affected by their mass ratios and fill-out factors. Determination of zero-point differences for different types of CBs may help us improve the accuracy of the resulting PLRs. We demonstrate that automated approaches to deriving CB properties could be a powerful tool for application to the much larger CB samples expected to result from future surveys.</description><source format="bibcode">2020ApJS..247...50S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/247/50</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/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</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/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/426/1001">J/A+A/426/1001 : Catalog of contact binary stars (Csizmadia+, 2004)</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/AJ/131/621">J/AJ/131/621 : Catalog of 1022 bright contact binary stars (Gettel+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/528/A90">J/A+A/528/A90 : SuperWASP short period eclipsing binaries (Norton+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/32">J/ApJ/763/32 : Galactic halo RRab stars from CSS (Drake+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/101">J/AJ/146/101 : LINEAR. III. Periodic variables (Palaversa+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/9">J/ApJS/208/9 : Intrinsic colors &amp; temperatures of PMS stars (Pecaut+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/430/2029">J/MNRAS/430/2029 : Initial masses of W UMa 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/148/81">J/AJ/148/81 : APASS BVgri photometry of RAVE stars. I. 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VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CRTS</name><description>Catalina Sky Survey (CSS) identifier (JHHMMSS.s+DDMMSS)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-19.7/70.1] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Period</name><description>[0.196/0.56] Orbital period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Teff1</name><description>[3436/15530] Primary effective temperature (1)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Teff2</name><description>[3520/11079] Secondary effective temperature (1)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Teff1</name><description>[8/4226]? Uncertainty in Teff1 (1)</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Teff2</name><description>[13/3290]? Uncertainty in Teff2 (1)</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>inc</name><description>[70/90] Inclination angle</description><unit>deg</unit><ucd>src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_inc</name><description>[0.1/22.2] Uncertainty in inc</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Omega</name><description>[1.8/15] Surface potential ({Omega}={Omega}_1_={Omega}_2_)</description><ucd>arith.factor;phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Omega</name><description>[0/0.8] Uncertainty in Omega</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>q</name><description>[0.07/0.8] Mass ratio; M2/M1</description><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_q</name><description>[0.09] Uncertainty in q</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_f</name><description>[0.01/4.1] Uncertainty in f</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LFrac</name><description>[0.4/1] Primary to total V band luminosity ratio</description><ucd>phys.luminosity;em.opt.V;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_LFrac</name><description>[0/0.4] Uncertainty in LFrac</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>OT</name><description>CB classification (1530 W-, 710 A-, and 95 B-type CBs)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>M1</name><description>[0.8/2.5] Primary mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M2</name><description>[0.08/1.4] Secondary mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_M1</name><description>[0.02/0.1] Uncertainty in M1</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_M2</name><description>[0.07/0.3] Uncertainty in M2</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r1</name><description>[0.7/2.2] Primary radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r2</name><description>[0.3/1.5] Secondary radius</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_r1</name><description>[0.02/0.07] Uncertainty in r1</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_r2</name><description>[0.01/0.03] Uncertainty in r2</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L1</name><description>[0.3/26.8] Primary luminosity</description><unit>solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L2</name><description>[0.05/9.2] Secondary luminosity</description><unit>solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_L1</name><description>[0.08/6.4] Uncertainty in L1</description><unit>solLum</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_L2</name><description>[0.02/4.6] Uncertainty in L2</description><unit>solLum</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>[1.5/4.2] Semi-major axis</description><unit>solRad</unit><ucd>phys.angSize.smajAxis</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_a</name><description>[0.03/0.1] Uncertainty in a</description><unit>solRad</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>