II/150Aivo://CDS.VizieR/II/150ACDSBrancewicz H.K.Dworak T.Z.1999-06-29T14:09:12Z1999-06-29T14:07:43ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.freclipsing-binary-starsAn iterative method has been used to compute the geometric and physical parameters of 1048 eclipsing binary stars.1980AcA....30..501Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/II/150ACatalogResearchIsServedByTAP VizieR generic servicerelated-toII/139 : General Catalog of Variable Stars (GCVS), 4th Ed. (Kholopov+ 1988)V/46 : Classical (Evolved) Algol-Type Binary Candidates (Budding 1984)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=II/150Ahttps://vizier.iucaa.in/viz-bin/VizieR-2?-source=II/150Ahttp://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=II/150Ahttps://vizier.cds.unistra.fr/viz-bin/votable?-source=II/150Ahttps://vizier.iucaa.in/viz-bin/votable?-source=II/150Ahttp://vizieridia.saao.ac.za/viz-bin/votable?-source=II/150AGETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultII/150A/catalogThe catalogueSpSpectrumsrc.spTypecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName of starmeta.id;meta.maincharCester[*] * if the star is present in Cester's (1979, 1980) catalogue & first supplementmeta.codecharPerPeriod in daysdtime.perioddoublePlxParallax1e-05arcsecpos.parallax.trigintSepSeparation between the components in Solar radiisolRadphys.size.radiusfloatR1Radius of brighter componentsolRadphys.size.radiusfloatR2Radius of fainter componentsolRadphys.size.radiusfloatRL1Percent of filling up of Roche-lobe%stat.fit.paramintRL2Percent of filling up of Roche-lobe%stat.fit.paramintL1Absolute bolometric luminositysolLumphys.luminositydoubleL2Absolute bolometric luminositysolLumphys.luminositydoubleT1Effective temperatureKphys.temperature.effectiveintT2Effective temperatureKphys.temperature.effectiveintMSum of masses in solar unitssolMassphys.massfloatqMass ratio q = M2/M1phys.mass;arith.ratiofloatM1Mass of brighter component (solar masses)solMassphys.massfloatClass[ABEW] Traditional Classification from GCVS (Kukarkin et al, cat. <II/139>)meta.code;src.varcharKopal[CDS] Kopal's geometrical classificationsrc.class.structchar