J/A+A/541/A41ivo://CDS.VizieR/J/A+A/541/A41doi:10.26093/cds/vizier.35410041CDSMowlavi N.Eggenberger P.Meynet G.Ekstrom S.Georgy C.Maeder A.,Charbonnel C.Eyer L.2018-02-12T08:45:33Z2012-04-26T08:24:39ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelsWe present dense grids of stellar models suitable for comparison with observable quantities measured with great precision, such as those derived from binary systems or planet-hosting stars. We computed new Geneva models without rotation at metallicities Z=0.006, 0.01, 0.014, 0.02, 0.03, and 0.04 (i.e. [Fe/H] from -0.33 to +0.54) and with mass in small steps from 0.5 to 3.5M_{sun}_. Great care was taken in the procedure for interpolating between tracks in order to compute isochrones.2012A&A...541A..41Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/541/A41CatalogResearchIsServedByTAP VizieR generic servicerelated-toVI/65 : Evolutionary models of evolved stars (Dorman+ 1993)VI/96 : Evolutionary Sequences (Fagotto+ 1993-96)VI/102 : Geneva stellar evolution tracks & isochrones (Lejeune+, 2001)VI/109 : Population Synthesis Models at very low metallicitiesVI/118 : Stellar Models until He burning (Claret+ 1995-1998)VI/120 : High-resolution synthetic stellar library (Coelho+, 2005)J/A+A/299/755 : Stellar evolution. II. Post-AGB (Bloecker+, 1995)J/A+A/424/919 : Stellar models grids. Z=0.02, M=0.8 to 125 (Claret, 2004)J/A+A/440/647 : New grids of stellar models. II. (Claret, 2005)J/A+A/453/769 : New grids of stellar models. III. (Claret+, 2006)J/A+A/467/1389 : New grids of stellar models. IV. (Claret, 2007)J/A+A/537/A146 : Stellar models with rotation. 0.8<M<120, Z=0.014J/A+A/540/A26 : Low-mass stars Pisa Evolution Models (Dell'Omodarme+, 2012)J/A+AS/96/269 : Stellar Models from 0.8 to 120 Msolar (Schaller+, 1992)J/A+AS/98/523 : Grids of stellar models. II. (Schaerer+ 1993)J/A+AS/101/415 : Grids of stellar models III. (Charbonnel+ 1993)J/A+AS/102/339 : Grids of stellar models IV (Schaerer+, 1993)J/A+AS/103/97 : Grids of stellar models V. (Meynet+ 1994)J/A+AS/115/339 : Stellar models VI. (Charbonnel+, 1996)J/A+AS/128/471 : Grids of stellar models. VII. (Mowlavi+ 1998)J/A+AS/135/405 : Grids of stellar models. VIII. (Charbonnel+ 1999)J/A+AS/109/441 : Stellar models until He burning - I. (Claret, 1995)J/A+AS/114/549 : Stellar models until He burning - II. (Claret+, 1995)J/A+AS/125/439 : Stellar models until He burning - III. (Claret+, 1997)J/MNRAS/298/525 : Stellar evolution models for Z=0.0001 to 0.03 (Pols+ 1998)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/541/A41https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/541/A41http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/541/A41https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/541/A41https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/541/A41http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/541/A41GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/541/A41/modelsList of models (39 tracks by table)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintFileNameName of the file, in subdirectory gridsmeta.id;meta.filecharZinitInitial Z abundancephys.atmol.initialfloatMinitIntitial masssolMassphys.massfloatModelModel for this composition and initial massmeta.ref.urlchartrackEvolutionary track for this (Zinit,Minit)meta.ref.urlcharAge20Phase 20 starting age (with first model at 0)yrtime.startdoubleAge21Phase 21 starting age (with first model at 100)yrtime.startdoubleAge22Phase 22 starting age (with first model at 200)yrtime.startdoubleAge23Phase 23 starting age (with first model at 300)yrtime.startdoubleAge30Phase 30 starting age (with first model at 380)yrtime.startdoubleAge31Phase 31 starting age (with first model at 600)yrtime.startdoubleJ/A+A/541/A41/gridsAll evolutionary tracksMass[0.5/3.5] Stellar masssolMassphys.massfloatPhase[20/31] Phase of the modelstat.paramintMinit[0.5/3.5] Stellar mass of the initial model of the evolutionary track from which this model has been computedlog(solMass)phys.massfloatprimaryZinit[0.006/0.04] Metallicity mass fraction of the initial model of the evolutionary track from which this model has been computedphys.abund.Z;meta.modelledfloatprimaryAgeAgeyrtime.age;meta.maindoubleprimarylogLLogarithm of the surface luminositylog(solLum)phys.luminosityfloatlogTeLogarithm of the effective temperaturelog(K)phys.temperature.effectivefloatlogrhocLogarithm of the central densitylog(g.cm**-3)phys.densityfloatlogTcLogarithm of the central temperaturelog(K)phys.temperaturefloatQccMass of the convective core relative to the stellar massphys.mass;arith.ratiofloatXc(H)Hydrogen mass fraction at the centerphys.mass;arith.ratiodoubleXc(3He)Helium (^3^He) mass fraction at the centerphys.mass;arith.ratiodoubleXc(4He)Helium (^4^He) mass fraction at the centerphys.mass;arith.ratiodoubleXc(12C)Carbon (^12^C) mass fraction at the centerphys.mass;arith.ratiodoubleXc(13C)Carbon (^13^C) mass fraction at the centerphys.mass;arith.ratiodoubleXc(14N)Nitrogen (^14^N) mass fraction at the centerphys.mass;arith.ratiodoubleXc(16O)Oxygen (^16^O) mass fraction at the centerphys.mass;arith.ratiodoubleXc(17O)Oxygen (^17^O) mass fraction at the centerphys.mass;arith.ratiodoubleXc(18O)Oxygen (^18^O) mass fraction at the centerphys.mass;arith.ratiodoubleXc(20Ne)Neon (^20^Ne) mass fraction at the centerphys.mass;arith.ratiodoubleXc(22Ne)Neon (^22^Ne) mass fraction at the centerphys.mass;arith.ratiodoubleXs(H)Hydrogen mass fraction at the surfacephys.mass;arith.ratiodoubleXs(3He)Helium (^3^He) mass fraction at the surfacephys.mass;arith.ratiodoubleXs(4He)Helium (^4^He) mass fraction at the surfacephys.mass;arith.ratiodoubleXs(12C)Carbon (^12^C) mass fraction at the surfacephys.mass;arith.ratiodoubleXs(13C)Carbon (^13^C) mass fraction at the surfacephys.mass;arith.ratiodoubleXs(14N)Nitrogen (^14^N) mass fraction at the surfacephys.mass;arith.ratiodoubleXs(16O)Oxygen (^16^O) mass fraction at the surfacephys.mass;arith.ratiodoubleXs(17O)Oxygen (^17^O) mass fraction at the surfacephys.mass;arith.ratiodoubleXs(18O)Oxygen (^18^O) mass fraction at the surfacephys.mass;arith.ratiodoubleXs(20Ne)Neon (^20^Ne) mass fraction at the surfacephys.mass;arith.ratiodoubleXs(22Ne)Neon (^22^Ne) mass fraction at the surfacephys.mass;arith.ratiodoubleXinit[0.66/0.75] Hydrogen mass fraction of the initial model of the evolutionary track from which this model has been computedphys.abund.X;meta.modelleddoubleYinit[0.25/0.30] Helium mass fraction of the initial model of the evolutionary track from which this model has been computedphys.abund.Y;meta.modelleddoubleZsurfSurface metallicityphys.abund.ZdoubleRStellar radiussolRadphys.size.radiusdoublelogrhoLogarithm of the mean stellar density relative to the solar mean density, with {rho}_{sun}_=1.411g/cm3log(Sun)phot.mag.sb;phys.density;arith.ratiofloat