J/MNRAS/298/525ivo://CDS.VizieR/J/MNRAS/298/525doi:10.26093/cds/vizier.72980525CDSPols O.R.Schroeder K.-P.Hurley J.R.Tout C.A.Eggleton P.P.2024-06-25T20:18:03Z2009-04-25T22:45:49ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelsWe have calculated a grid of empirically well tested evolutionary tracks with masses M between 0.5 and 50M_{sun}_, spaced by approximately 0.1 in log M, and with metallicities Z=0.0001, 0.0003, 0.001, 0.004, 0.01, 0.02 and 0.03. We use a robust and fast evolution code with a self-adaptive non-Lagrangian mesh, which employs the mixing-length theory but treats convective mixing as a diffusion process, solving simultaneously for the structure and the chemical composition. The hydrogen and helium abundances are chosen as functions of the metallicity: X=0.76-3.0Z and Y=0.24+2.0Z. Two sets of models were computed, one without and one with a certain amount of enhanced mixing or 'overshooting'.1998MNRAS.298..525Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/298/525CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/125/229 : A standard stellar library (Lejeune+ 1997)J/A+AS/130/65 : A standard stellar library. II. (Lejeune+ 1998)VI/102 : Geneva stellar evolution tracks and isochrones (Lejeune+, 2001)VI/54 : Horizontal Branch Stellar Model Calculations (Dorman 1992)VI/65 : Evolutionary models of evolved stars (Dorman+ 1993)VI/96 : Evolutionary Sequences (Fagotto+ 1993-96)VI/113 : Evolutionary models of Population II stars (Cariulo+, 2004)VI/118 : Stellar Models until He burning (Claret+ 1995-1998)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/298/525https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/298/525http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/298/525https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/298/525https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/298/525http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/298/525GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/MNRAS/298/525/zamsZero-Age Main Sequence parametersrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintModModel number (see paper)meta.id;meta.mainintMStar masssolMassphys.massfloatlog.TeEffective temperaturelog(K)phys.temperature.effectivefloatlog.LStar Luminositylog(solLum)phys.luminosityfloatlog.RStar radiuslog(solRad)meta.idfloatk2Dimensionless moment of inertia I/(MR^2^)stat.variance;pos.distance;phys.sizefloatTcCore temperaturelog(T)phys.temperaturefloatDcCore densitylog(g.cm**-3)phys.densityfloatH1.cCore mass fraction of Hydrogen (^1^H)phys.mass;arith.ratiodoubleHe4.cCore mass fraction of Helium (^4^He)phys.mass;arith.ratiodoubleC12.cCore mass fraction of Carbon (^12^C)phys.mass;arith.ratiodoubleN14.cCore mass fraction of Nitrogen (^14^N)phys.mass;arith.ratiodoubleO16.cCore mass fraction of Oxygen (^16^O)phys.mass;arith.ratiodoubleJ/MNRAS/298/525/summarySummary of critical turning pointsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintO[OS] Standard or Overshooting modelmeta.id;stat.fitcharZInitial metallicity (1)phys.abund.ZfloatMassStar mass (no mass loss taken into account)solMassphys.massfloatMod"Model" (evolution) number (see paper)meta.id;meta.mainintn_Mod[A-Z] Critical phase of evolution (2)meta.notecharfModFinal model numbermeta.idintAgeStar ageyrtime.agedoublelog.TeEffective temperature at Agelog(K)phys.temperature.effectivefloatlog.LStar Luminosity at Agelog(solLum)phys.luminosityfloatlog.RStar radius at Agelog(solRad)meta.idfloatMc.HeHelium core masslog(solMass)phys.massfloatMc.COCarbon/Oxygen core masslog(solMass)phys.massfloatk2Dimensionless moment of inertia I/(MR^2^)stat.variance;pos.distance;phys.sizefloatTcCore temperaturelog(T)phys.temperaturefloatDcCore densitylog(g.cm**-3)phys.densityfloatH1.cCore mass fraction of Hydrogen (^1^H)phys.mass;arith.ratiodoubleHe4.cCore mass fraction of Helium (^4^He)phys.mass;arith.ratiodoubleC12.cCore mass fraction of Carbon (^12^C)phys.mass;arith.ratiodoubleN14.cCore mass fraction of Nitrogen (^14^N)phys.mass;arith.ratiodoubleO16.cCore mass fraction of Oxygen (^16^O)phys.mass;arith.ratiodoubleH1.sShell mass fraction of Hydrogen (^1^H)phys.mass;arith.ratiodoubleHe4.sShell mass fraction of Helium (^4^He)phys.mass;arith.ratiodoubleC12.sShell mass fraction of Carbon (^12^C)phys.mass;arith.ratiodoubleN14.sShell mass fraction of Nitrogen (^14^N)phys.mass;arith.ratiodoubleO16.sShell mass fraction of Oxygen (^16^O)phys.mass;arith.ratiodoubleTrackPlot this trackmeta.ref.urlcharJ/MNRAS/298/525/ubvri_k*Synthetic Johnson-Cousins BVRI colors (Kurucz)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint[Fe/H]Metallicitylog(Sun)phys.abund.ZfloatTeffEffective temperatureKphys.temperature.effectiveintlog.gSurface gravitylog(cm.s**-2)phys.gravityfloatBC(V)Bolometric correctionmagphot.mag.bcfloatU-BJohnson color index U-Bmagphot.color;em.opt.U;em.opt.BfloatB-VJohnson color index B-Vmagphot.color;em.opt.B;em.opt.VfloatV-RJohnson-Cousins color index V-Rmagphot.color;em.opt.V;em.opt.RfloatR-ICousins color index R-Imagphot.color;em.opt.R;em.opt.IfloatJ/MNRAS/298/525/ubvri_c*Synthetic Johnson-Cousins BVRI colors (corrected)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint[Fe/H]Metallicitylog(Sun)phys.abund.ZfloatTeffEffective temperatureKphys.temperature.effectiveintlog.gSurface gravitylog(cm.s**-2)phys.gravityfloatBC(V)Bolometric correctionmagphot.mag.bcfloatU-BJohnson color index U-Bmagphot.color;em.opt.U;em.opt.BfloatB-VJohnson color index B-Vmagphot.color;em.opt.B;em.opt.VfloatV-RJohnson-Cousins color index V-Rmagphot.color;em.opt.V;em.opt.RfloatR-ICousins color index R-Imagphot.color;em.opt.R;em.opt.Ifloat