J/A+A/460/783ivo://CDS.VizieR/J/A+A/460/783doi:10.26093/cds/vizier.34600783CDSBeuermann K.2007-01-11T11:17:28Z2007-01-11T12:16:05ZCDS support team

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

cds-question@unistra.frastronomical-modelsdwarf-starsBarnes-Evans type relations provide an empirical relationship between the surface brightness of stars and their color. They are widely used for measuring the distances to stars of known radii, as the Roche-lobe filling secondaries in cataclysmic variables (CVs). The calibration of the surface brightness of field dwarfs of near-solar metalicity with spectral types A0 to L8 covers all secondary spectral types detectable in CVs and related objects and will aid in the measurement of their distances. The calibrations are based on the radii of field dwarfs measured by the Infrared Flux Method and by interferometry. Published photometry is used and homogenized to the Cousins Rc and Ic and the CIT JHK photometric systems. The narrow band surface brightness at 7500{AA} is based on our own and published spectrophotometry. Care is taken to select the dwarfs for near-solar metalicity, appropriate to CVs, and to avoid errors caused by unrecognized binarity.2006A&A...460..783Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/460/783CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/460/783https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/460/783http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/460/783https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/460/783https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/460/783http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/460/783GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/460/783/table2Parameters of polynomial fits of surface brightness vs. V-K or spectral typerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLineLine numbermeta.idintDepVDependant variable (1)meta.notecharX[X V-K] Independent variable used in polynomial fit (2)stat.paramcharRangelRange of independant variable (lower limit)stat.paramfloatRangeuRange of independant variable (upper limit)stat.paramfloatSpTypelLower spectral type rangeinstr.bandwidthcharSpTypeuUpper spectral type rangeinstr.bandwidthchara0a0 coefficient of polynomial fit (2)stat.fit.param;meta.modelleddoublea1a1 coefficient of polynomial fit (2)stat.fit.param;meta.modelleddoublea2? a2 coefficient of polynomial fit (2)stat.fit.param;meta.modelleddoublenullablea3? a3 coefficient of polynomial fit (2)stat.fit.param;meta.modelleddoublenullablea4? a4 coefficient of polynomial fit (2)stat.fit.param;meta.modelleddoublenullablea5? a5 coefficient of polynomial fit (2)stat.fit.param;meta.modelleddoublenullable