J/A+AS/103/67ivo://CDS.VizieR/J/A+AS/103/67CDSde Loore C.Vanbeveren D.2000-01-21T04:21:03Z2000-01-21T05:20:54ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelsmultiple-starsmagellanic-cloudsTables of evolutionary sequences for massive stars with metallicities Z=0.002 and Z=0.01 in the mass range 9 to 40 M_{sun}_ and mass ratios 0.9 and 0.6 are presented. The orbital periods are chosen such that mass transfer according to case B occurs, i.e. mass exchange after core hydrogen exhaustion, during semi-detached and contact phases. The evolutionary code used by de Loore & De Greve (1992A&AS...94..453D) for galactic massive close binaries was updated, i.e. new thermodynamic quantities and new opacities were installed. The evolution of both components is followed simultaneously. Stellar wind mass loss rates during the OB phase are scaled according to the radiatively driven wind theory. Wolf-Rayet mass loss rates are assumed to be independent of metallicity. The models presented here may be used to interpret and evaluate the observations of Wolf-Rayet stars and massive binary X-ray sources in the Small and Large Magellanic Clouds.1994A&AS..103...67Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/103/67CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/103/67https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/103/67http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/103/67https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/103/67https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/103/67http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/103/67GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+AS/103/67/lmcLMC abundances (Table3 to Table15)recnoRecord number assigned by the VizieR team. Should Not be used for identification.intIM1Initial mass of the primarySunintIM2Initial mass of the secondarySunfloatPhaseSee note (1)charAgeEvolutionary stageyrdoubleM1Mass of the primarysolMassfloatML1Mass loss rate of the primarysolMass/yrdoublelogTeff1Effective temperature of the primarylog(K)floatlogL1Luminosity of the primarylog(solLum)floatXC1Central hydrogen content of the primaryfloatYC1Central helium content of the primaryfloatXAT1Surface hydrogen abundance of the primaryfloatRad1Radius of the primarysolRadfloatMCC1Convective core mass of the primarySunfloatPeriod? Orbital periodddoublenullableM2? Mass of the secondarysolMassfloatnullableML2? Mass loss rate of the secondarysolMass/yrdoublenullablelogTeff2? Effective temperature of the secondarylog(K)floatnullablelogL2? Luminosity of the secondarylog(solLum)floatnullableXC2? Central hydrogen content of the secondaryfloatnullableYC2? Central helium content of the secondaryfloatnullableXAT2? Surface hydrogen content of the secondaryfloatnullableRad2? Radius of the secondarysolRadfloatnullableMCC2? Convective core mass of the secondarysolMassfloatnullableJ/A+AS/103/67/smcSMC abundances (Table16 to Table29)recnoRecord number assigned by the VizieR team. Should Not be used for identification.intIM1Initial mass of the primarySunintIM2Initial mass of the secondarySunfloatPhaseSee note (1)charAgeEvolutionary stageyrdoubleM1Mass of the primarysolMassfloatML1Mass loss rate of the primarysolMass/yrdoublelogTeff1Effective temperature of the primarylog(K)floatlogL1Luminosity of the primarylog(solLum)floatXC1Central hydrogen content of the primaryfloatYC1Central helium content of the primaryfloatXAT1Surface hydrogen abundance of the primaryfloatRad1Radius of the primarysolRadfloatMCC1Convective core mass of the primarySunfloatPeriod? Orbital periodddoublenullableM2? Mass of the secondarysolMassfloatnullableML2? Mass loss rate of the secondarysolMass/yrdoublenullablelogTeff2? Effective temperature of the secondarylog(K)floatnullablelogL2? Luminosity of the secondarylog(solLum)floatnullableXC2? Central hydrogen content of the secondaryfloatnullableYC2? Central helium content of the secondaryfloatnullableXAT2? Surface hydrogen content of the secondaryfloatnullableRad2? Radius of the secondarysolRadfloatnullableMCC2? Convective core mass of the secondarysolMassfloatnullable