J/A+A/543/A108ivo://CDS.VizieR/J/A+A/543/A108doi:10.26093/cds/vizier.35430108CDSLagarde N.Decressin T.Charbonnel C.Eggenberger P.Ekstroem S.,Palacios A.2012-12-08T21:54:06Z2012-09-01T17:05:35ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelsThe availability of asteroseismic constraints for a large sample of stars from the missions CoRoT and Kepler paves the way for various statistical studies of the seismic properties of stellar populations. We evaluate the impact of rotation-induced mixing and thermohaline instability on the global asteroseismic parameters at different stages of the stellar evolution from the zero age main sequence to the thermally pulsating asymptotic giant branch to distinguish stellar populations.2012A&A...543A.108Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/543/A108CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/543/A108https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/543/A108http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/543/A108https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/543/A108https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/543/A108http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/543/A108GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/543/A108/modelsGrids of stellar modelsZInitial Z abundancephys.atmol.initialfloattAgeyrtime.agedoubleXHe4cCentral abundance of 4He (mass fraction)phys.abunddoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintT[rs] s: standard prescriptions or r: th+rot prescriptionsmeta.id;stat.fitcharMass[1/6] Initial mass (1.0, 1.25, 1.5, 2.0, 2.5, 3.0, 4.0, 6.0)solMassphys.massfloatModModel numbermeta.id;meta.mainintLSurface luminositysolLumphys.luminositydoubleReffPhotospheric radiussolRadphys.size.radiusfloatTeffEffective temperatureKphys.temperature.effectiveintrhoeffPhotospheric densityg.cm**-3phys.densitydoublelog(g)Photospheric gravitylog(cm.s**-2)phys.gravityfloatMlossMass-loss ratesolMass/yrphys.mass.lossdoubleMStellar masssolMassphys.massdoublevsurfSurface velocitykm/sphys.velocdoubleAmaxMaximum amplitudesrc.var.amplitudedoublednu.aThe large separation from asymptotic relationHzem.freq;src.vardoublednu.sThe large separation from scaling relationHzem.freq;src.vardoubleTtotThe total acoustic radius {tau}_t_sphys.size.radius;arith.ratiodoubletBCEThe acoustic radius at the base of the convective envelopesphys.size.radius;arith.ratiodoubletHeThe acoustic radius at the location of helium second-ionisation regionsphys.size.radius;arith.ratiodoublenumaxThe frequency with the maximum amplitudeHzem.freq;src.vardoubleDpgThe asymptotic period spacing of g-modesstime.perioddoubleTcCentral temperatureKphys.temperaturedoubleTmaxMaximum of temperatureKphys.temperaturedoubleMrTmaxMass coordinate of TmaxsolMassphys.massdoublerhocCentral densityg.cm**-3phys.densitydoublerhomaxDensity at the location of Tmaxg.cm**-3phys.densitydoublePcCentral pressure (cgs)dPaphys.pressuredoubleMbenvMass at the base of convective envelopesolMassphys.massdoubleXHcCentral abundance of H (mass fraction)phys.abunddoubleXHe3cCentral abundance of 3He (mass fraction)phys.abunddoubleXC12cCentral abundance of 12C (mass fraction)phys.abunddoubleXC13cCentral abundance of 13C (mass fraction)phys.abunddoubleXC14cCentral abundance of 14C (mass fraction)phys.abunddoubleXN14cCentral abundance of 14N (mass fraction)phys.abunddoubleXO16cCentral abundance of 16O (mass fraction)phys.abunddoubleXO17cCentral abundance of 17O (mass fraction)phys.abunddoubleXO18cCentral abundance of 18O (mass fraction)phys.abunddoubleXF19cCentral abundance of 19F (mass fraction)phys.abunddoubleXNe20cCentral abundance of 20Ne (mass fraction)phys.abunddoubleXNe21cCentral abundance of 21Ne (mass fraction)phys.abunddoubleXNe22cCentral abundance of 22Ne (mass fraction)phys.abunddoubleXNa23cCentral abundance of 23Na (mass fraction)phys.abunddoubleXMg24cCentral abundance of 24Mg (mass fraction)phys.abunddoubleXMg25cCentral abundance of 25Mg (mass fraction)phys.abunddoubleXMg26cCentral abundance of 26Mg (mass fraction)phys.abunddoubleXAl26cCentral abundance of 26Al (mass fraction)phys.abunddoubleXAl27cCentral abundance of 27Al (mass fraction)phys.abunddoubleXSi28cCentral abundance of 28Si (mass fraction)phys.abunddoubleXHsSurface abundance of H (mass fraction)phys.abunddoubleXH2sSurface abundance of 2H (mass fraction)phys.abunddoubleXHe3sSurface abundance of 3He (mass fraction)phys.abunddoubleXHe4sSurface abundance of 4He (mass fraction)phys.abunddoubleXLi6sSurface abundance of 6Li (mass fraction)phys.abunddoubleXLi7sSurface abundance of 7Li (mass fraction)phys.abunddoubleXBe7sSurface abundance of 7Be (mass fraction)phys.abunddoubleXBe9sSurface abundance of 9Be (mass fraction)phys.abunddoubleXB10sSurface abundance of 10B (mass fraction)phys.abunddoubleXB11sSurface abundance of 11B (mass fraction)phys.abunddoubleXC12sSurface abundance of 12C (mass fraction)phys.abunddoubleXC13sSurface abundance of 13C (mass fraction)phys.abunddoubleXC14sSurface abundance of 14C (mass fraction)phys.abunddoubleXN14sSurface abundance of 14N (mass fraction)phys.abunddoubleXO16sSurface abundance of 16O (mass fraction)phys.abunddoubleXO17sSurface abundance of 17O (mass fraction)phys.abunddoubleXO18sSurface abundance of 18O (mass fraction)phys.abunddoubleXF19sSurface abundance of 19F (mass fraction)phys.abunddoubleXNe20sSurface abundance of 20Ne (mass fraction)phys.abunddoubleXNe21sSurface abundance of 21Ne (mass fraction)phys.abunddoubleXNe22sSurface abundance of 22Ne (mass fraction)phys.abunddoubleXNa23sSurface abundance of 23Na (mass fraction)phys.abunddoubleXMg24sSurface abundance of 24Mg (mass fraction)phys.abunddoubleXMg25sSurface abundance of 25Mg (mass fraction)phys.abunddoubleXMg26sSurface abundance of 26Mg (mass fraction)phys.abunddoubleXAl26sSurface abundance of 26Al (mass fraction)phys.abunddoubleXAl27sSurface abundance of 27Al (mass fraction)phys.abunddoubleXSi28sSurface abundance of 28Si (mass fraction)phys.abunddoubletrackEvolution track of this modelmeta.ref.urlchar