Evolutionary SequencesVI/96ivo://CDS.VizieR/VI/96CDSBressan A.Fagotto F.Bertelli G.Chiosi C.Girardi L.Nasi E.2003-11-24T20:39:57Z2003-11-24T21:38:52ZCDS support teamCDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, Francecds-question@unistra.frstellar-evolutionary-modelshertzsprung-russell-diagramchemical-abundancesThe tracks cover the mass interval from 0.6 to 120M_{sun}_, for 7 different metallicities The isochrones are derived from the evolutionary tracks listed in the item above.1993A&AS..100..647Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/VI/96CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/106/275 : Theoretical isochrones (Bertelli+ 1994)http://pleiadi.pd.astro.it : Padova database of stellar evolutionaryhttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=VI/96https://vizier.iucaa.in/viz-bin/VizieR-2?-source=VI/96http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=VI/96https://vizier.cds.unistra.fr/viz-bin/votable?-source=VI/96https://vizier.iucaa.in/viz-bin/votable?-source=VI/96http://vizieridia.saao.ac.za/viz-bin/votable?-source=VI/96GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefault
VI/96/table1Evolutionary sequences of low mass stars up to the tip of the RGBAgeAge of modelsyrtime.agedoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZInitial metallicity (G1)phys.abund.ZfloatMassInitial masssolMassphys.massfloatlog(L)Logarithm (base 10) of total luminositylog(solLum)phys.luminosityfloatlog(Teff)Logarithm (base 10) of effective temperaturelog(K)phys.temperature.effectivefloatlogGLogarithm (base 10) of surface gravitylog(cm.s**-2)phys.gravityfloatlogTcLogarithm (base 10) of central temperaturelog(K)phys.temperaturefloatlog(rhoc)Logarithm (base 10) of central densityphys.densityfloatCOMPCentral abundance (by mass) of hydrogen or heliumphys.abundfloatXCCentral abundance of ^12^Cphys.abunddoubleXOCentral abundance of ^16^Ophys.abunddoubleConvFractionary mass of the convective core (inclusive of overshoot)phys.mass;arith.ratiofloatQdiscFractionary mass of the first mesh point where the chemical composition differs from the surface valuephys.mass;arith.ratiofloatlog(LH)Logarithm (base 10) of hydrogen luminositylog(solLum)phys.luminosityfloatQ1HFractionary mass of the inner border of the hydrogen rich regionphys.mass;arith.ratiofloatQ2HFractionary mass of the outer border of the H-burning region (1)phys.mass;arith.ratiofloatlog(LHe)Logarithm (base 10) of helium luminositylog(solLum)phys.luminosityfloatQ1HeFractionary mass of the inner border of the He-burning region (when greater than zero He-burning is in a shell) (1)phys.mass;arith.ratiofloatQ2HeFractionary mass of the upper border of the He-burning region (1)phys.mass;arith.ratiofloatlog(LC)Logarithm (base 10) of carbon luminositylog(solLum)phys.luminosityfloatlog(Lnu)Logarithm (base 10) of neutrinos luminosity (absolute value)log(solLum)phys.luminosityfloatQTmaxFractionary mass of the point where the temperature attains the maximum valuephys.mass;arith.ratiofloat
VI/96/table2Evolutionary sequences of low mass stars during the core helium-burning and EAGB phasesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZInitial metallicity (G1)phys.abund.ZfloatMassInitial masssolMassphys.massfloatAgeAge of modelsyrtime.agedoublelog(L)Logarithm (base 10) of total luminositylog(solLum)phys.luminosityfloatlog(Teff)Logarithm (base 10) of effective temperaturelog(K)phys.temperature.effectivefloatlogGLogarithm (base 10) of surface gravitylog(cm.s**-2)phys.gravityfloatlogTcLogarithm (base 10) of central temperaturelog(K)phys.temperaturefloatlog(rhoc)Logarithm (base 10) of central densityphys.densityfloatCOMPCentral abundance (by mass) of hydrogen or heliumphys.abundfloatXCCentral abundance of ^12^Cphys.abunddoubleXOCentral abundance of ^16^Ophys.abunddoubleConvFractionary mass of the convective core (inclusive of overshoot)phys.mass;arith.ratiofloatQdiscFractionary mass of the first mesh point where the chemical composition differs from the surface valuephys.mass;arith.ratiofloatlog(LH)Logarithm (base 10) of hydrogen luminositylog(solLum)phys.luminosityfloatQ1HFractionary mass of the inner border of the hydrogen rich regionphys.mass;arith.ratiofloatQ2HFractionary mass of the outer border of the H-burning region (1)phys.mass;arith.ratiofloatlog(LHe)Logarithm (base 10) of helium luminositylog(solLum)phys.luminosityfloatQ1HeFractionary mass of the inner border of the He-burning region (when greater than zero He-burning is in a shell) (1)phys.mass;arith.ratiofloatQ2HeFractionary mass of the upper border of the He-burning region (1)phys.mass;arith.ratiofloatlog(LC)Logarithm (base 10) of carbon luminositylog(solLum)phys.luminosityfloatlog(Lnu)Logarithm (base 10) of neutrinos luminosity (absolute value)log(solLum)phys.luminosityfloatQTmaxFractionary mass of the point where the temperature attains the maximum valuephys.mass;arith.ratiofloat
VI/96/table3Evolutionary sequences of intermediate mass stars up to the TP-AGB and of massive stars (those with no mass-loss) up to the carbon-ignitionZInitial metallicity (G1)phys.abund.ZfloatAgeAge of modelsyrtime.agedoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMassInitial masssolMassphys.massfloatlog(L)Logarithm (base 10) of total luminositylog(solLum)phys.luminosityfloatlog(Teff)Logarithm (base 10) of effective temperaturelog(K)phys.temperature.effectivefloatlogGLogarithm (base 10) of surface gravitylog(cm.s**-2)phys.gravityfloatlogTcLogarithm (base 10) of central temperaturelog(K)phys.temperaturefloatlog(rhoc)Logarithm (base 10) of central densityphys.densityfloatCOMPCentral abundance (by mass) of hydrogen or heliumphys.abundfloatXCCentral abundance of ^12^Cphys.abunddoubleXOCentral abundance of ^16^Ophys.abunddoubleConvFractionary mass of the convective core (inclusive of overshoot)phys.mass;arith.ratiofloatQdiscFractionary mass of the first mesh point where the chemical composition differs from the surface valuephys.mass;arith.ratiofloatlog(LH)Logarithm (base 10) of hydrogen luminositylog(solLum)phys.luminosityfloatQ1HFractionary mass of the inner border of the hydrogen rich regionphys.mass;arith.ratiofloatQ2HFractionary mass of the outer border of the H-burning region (1)phys.mass;arith.ratiofloatlog(LHe)Logarithm (base 10) of helium luminositylog(solLum)phys.luminosityfloatQ1HeFractionary mass of the inner border of the He-burning region (when greater than zero He-burning is in a shell) (1)phys.mass;arith.ratiofloatQ2HeFractionary mass of the upper border of the He-burning region (1)phys.mass;arith.ratiofloatlog(LC)Logarithm (base 10) of carbon luminositylog(solLum)phys.luminosityfloatlog(Lnu)Logarithm (base 10) of neutrinos luminosity (absolute value)log(solLum)phys.luminosityfloatQTmaxFractionary mass of the point where the temperature attains the maximum valuephys.mass;arith.ratiofloat
VI/96/table4Evolutionary sequences for massive stars with mass lossrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZInitial metallicity (G1)phys.abund.ZfloatIMassInitial masssolMassphys.massfloatAgeAge of modelsyrtime.agedoubleMassCurrent value of the masssolMassphys.massfloatlog(L)Logarithm (base 10) of total luminositylog(solLum)phys.luminosityfloatlog(Teff)Logarithm (base 10) of effective temperaturelog(K)phys.temperature.effectivefloatlogGLogarithm (base 10) of surface gravitylog(cm.s**-2)phys.gravityfloatlogTcLogarithm (base 10) of central temperaturelog(K)phys.temperaturefloatlog(rhoc)Logarithm (base 10) of the central densityphys.densityfloatCOMPCentral abundance (by mass) of hydrogen or heliumphys.abundfloatXCCentral abundance of ^12^Cphys.abunddoubleXOCentral abundance of ^16^Ophys.abunddoubleConvFractionary mass of the convective core (inclusive of overshoot)phys.mass;arith.ratiofloatQdiscFractionary mass of the first mesh point where the chemical composition differs from the surface valuephys.mass;arith.ratiofloatlog(LH)Logarithm (base 10) of hydrogen luminositylog(solLum)phys.luminosityfloatQ1HFractionary mass of the inner border of the hydrogen rich regionphys.mass;arith.ratiofloatlog(LHe)Logarithm (base 10) of helium luminositylog(solLum)phys.luminosityfloatlog(dM/dt)Logarithm (base 10) of the absolute value of the mass loss ratelog(solMass.yr**-1)phys.mass.lossfloatXsurSurface abundance (by mass) of ^1^Hphys.abund.XdoubleYsurSurface abundance (by mass) of ^4^Hephys.abund.YdoubleXCsurSurface abundance (by mass) of ^12^Cphys.densitydoubleXNsurSurface abundance (by mass) of ^14^Nphys.densitydoubleXOsurSurface abundance (by mass) of ^16^Ophys.densitydouble
VI/96/table5aEvolutionary sequences for intermediate and massive stars up to the starting of TPAGB or carbon-ignition with the semiconvective scheme of mixing (only for Z=0.02)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZInitial metallicity (G1)phys.abund.ZfloatMassInitial masssolMassphys.massfloatAgeAge of modelsyrtime.agedoublelog(L)Logarithm (base 10) of total luminositylog(solLum)phys.luminosityfloatlog(Teff)Logarithm (base 10) of effective temperaturelog(K)phys.temperature.effectivefloatlogGLogarithm (base 10) of surface gravitylog(cm.s**-2)phys.gravityfloatlogTcLogarithm (base 10) of central temperaturelog(K)phys.temperaturefloatlog(rhoc)Logarithm (base 10) of central densityphys.densityfloatCOMPCentral abundance (by mass) of hydrogen or heliumphys.abundfloatXCCentral abundance of ^12^Cphys.abunddoubleXOCentral abundance of ^16^Ophys.abunddoubleConvFractionary mass of the convective core (inclusive of overshoot)phys.mass;arith.ratiofloatQdiscFractionary mass of the first mesh point where the chemical composition differs from the surface valuephys.mass;arith.ratiofloatlog(LH)Logarithm (base 10) of hydrogen luminositylog(solLum)phys.luminosityfloatQ1HFractionary mass of the inner border of the hydrogen rich regionphys.mass;arith.ratiofloatQ2HFractionary mass of the outer border of the H-burning region (1)phys.mass;arith.ratiofloatlog(LHe)Logarithm (base 10) of helium luminositylog(solLum)phys.luminosityfloatQ1HeFractionary mass of the inner border of the He-burning region (when greater than zero He-burning is in a shell) (1)phys.mass;arith.ratiofloatQ2HeFractionary mass of the upper border of the He-burning region (1)phys.mass;arith.ratiofloatlog(LC)Logarithm (base 10) of carbon luminositylog(solLum)phys.luminosityfloatlog(Lnu)Logarithm (base 10) of neutrinos luminosity (absolute value)log(solLum)phys.luminosityfloatQTmaxFractionary mass of the point where the temperature attains the maximum valuephys.mass;arith.ratiofloat
VI/96/table5bEvolutionary sequences for intermediate and massive stars up to the starting of TPAGB or carbon-ignition with the semiconvective scheme of mixing (only for Z=0.02)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZInitial metallicity (G1)phys.abund.ZfloatIMassInitial masssolMassphys.massfloatAgeAge of modelsyrtime.agedoubleMassCurrent value of the masssolMassphys.massfloatlog(L)Logarithm (base 10) of total luminositylog(solLum)phys.luminosityfloatlog(Teff)Logarithm (base 10) of effective temperaturelog(K)phys.temperature.effectivefloatlogGLogarithm (base 10) of surface gravitylog(cm.s**-2)phys.gravityfloatlogTcLogarithm (base 10) of central temperaturelog(K)phys.temperaturefloatlog(rhoc)Logarithm (base 10) of the central densityphys.densityfloatCOMPCentral abundance (by mass) of hydrogen or heliumphys.abundfloatXCCentral abundance of ^12^Cphys.abunddoubleXOCentral abundance of ^16^Ophys.abunddoubleConvFractionary mass of the convective core (inclusive of overshoot)phys.mass;arith.ratiofloatQdiscFractionary mass of the first mesh point where the chemical composition differs from the surface valuephys.mass;arith.ratiofloatlog(LH)Logarithm (base 10) of hydrogen luminositylog(solLum)phys.luminosityfloatQ1HFractionary mass of the inner border of the hydrogen rich regionphys.mass;arith.ratiofloatlog(LHe)Logarithm (base 10) of helium luminositylog(solLum)phys.luminosityfloatlog(dM/dt)Logarithm (base 10) of the absolute value of the mass loss ratelog(solMass.yr**-1)phys.mass.lossfloatXsurSurface abundance (by mass) of ^1^Hphys.abund.XdoubleYsurSurface abundance (by mass) of ^4^Hephys.abund.YdoubleXCsurSurface abundance (by mass) of ^12^Cphys.densitydoubleXNsurSurface abundance (by mass) of ^14^Nphys.densitydoubleXOsurSurface abundance (by mass) of ^16^Ophys.densitydouble
VI/96/isoIsochronesAgeAgeGyrtime.agefloatVmagV magnitudemagphot.mag;em.opt.VfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZInitial metallicity (G1)phys.abund.ZfloatMassInitial masssolMassphys.massfloatLogTeEffective temperaturelog(K)phys.temperature.effectivefloatMbolBolometric magnitudemagphys.magAbs.bolfloatU-BU-B colour indexmagphot.color;em.opt.U;em.opt.BfloatB-VB-V colour indexmagphot.color;em.opt.B;em.opt.VfloatV-RV-R colour indexmagphot.color;em.opt.V;em.opt.RfloatV-IV-I colour indexmagphot.color;em.opt.V;em.opt.IfloatV-JV-J colour indexmagphot.color;em.opt.V;em.IR.JfloatV-HV-H colour indexmagphot.color;em.opt.V;em.IR.HfloatV-KV-K colour indexmagphot.color;em.opt.V;em.IR.KfloatFLUMNormalized integrated mass function (1)phys.luminosity.fundoubleMwindWind masssolMassphys.massfloat