J/A+A/346/586ivo://CDS.VizieR/J/A+A/346/586doi:10.26093/cds/vizier.33460586CDSPerez Hernandez F.Claret A.Hernandez M.M.Michel E.1999-06-12T18:48:19Z1999-06-12T18:44:05ZCDS support team

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

cds-question@unistra.frastronomical-modelsstellar-atmospheresa-starsvisible-astronomymedium-band-photometrynarrow-band-photometryWide-band photometryMagnitude differences between rotating and non-rotating copartners for a grid of models with solar metallicity are tabulated here. The results are expressed in terms of the dimensionless angular velocity w-bar- defined in Eq.(1) of the paper, the angle of inclination i and the atmospheric parameters T_e_ and g_e_ defined in Eqs.(22) and (21), respectively. To obtain the absolute magnitudes for a given rotating model, the magnitudes of a non-rotating model with T_eff_=T_e_, g=g_e_ and the same intrinsic luminosity must be added. Results are given for the filters in the Geneva, Johnson and Stroemgren systems. Eq (1): w-bar = {Omega}/{Omega}_c_, where {Omega} is the angular velocity of the star, and {Omega}_c_^2^=8GM/(27R^3^_p_), where M is the mass and R_p_ the polar radius.1999A&A...346..586Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/346/586CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/346/586https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/346/586http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/346/586https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/346/586https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/346/586http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/346/586GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/346/586/table1Geneva photometryiAngle of inclinationdegsrc.orbital.inclinationfloatDGmagMagnitude difference in filter Gmagphot.mag;arith.difffloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogTeElectron temperature atmospheric parameter (1)log(K)phys.temperature;phys.electronfloatloggeElectron surface gravity atmospheric parameterlog(cm.s**-2)phys.gravityfloatw-barDimensionless angular velocityphys.veloc.angfloatDBmagMagnitude difference in filter Bmagphot.mag;arith.difffloatDUmagMagnitude difference in filter Umagphot.mag;arith.difffloatDVmagMagnitude difference in filter Vmagphot.mag;arith.difffloatDB1magMagnitude difference in filter B1magphot.mag;arith.difffloatDB2magMagnitude difference in filter B2magphot.mag;arith.difffloatDV1magMagnitude difference in filter V1magphot.mag;arith.difffloatIndicesLink to all photometric indexes for the set of (log(T_e_), log(g_e_), w-bar and i)meta.refcharJ/A+A/346/586/table2Johnson and Stroemgren photometryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogTeElectron temperature atmospheric parameter (1)log(K)phys.temperature;phys.electronfloatloggeElectron surface gravity atmospheric parameterlog(cm.s**-2)phys.gravityfloatw-barDimensionless angular velocityphys.veloc.angfloatiAngle of inclinationdegsrc.orbital.inclinationfloatDUmagMagnitude difference in filter Umagphot.mag;arith.difffloatDBmagMagnitude difference in filter Bmagphot.mag;arith.difffloatDVmagMagnitude difference in filter Vmagphot.mag;arith.difffloatDumagMagnitude difference in filter umagphot.mag;arith.difffloatDvmagMagnitude difference in filter vmagphot.mag;arith.difffloatDbmagMagnitude difference in filter bmagphot.mag;arith.difffloatDymagMagnitude difference in filter ymagphot.mag;arith.difffloatIndicesLink to all photometric indexes for the set of (log(T_e_), log(g_e_), w-bar and i)meta.refchar