J/A+AS/115/339ivo://CDS.VizieR/J/A+AS/115/339CDSCharbonel C.Meynet G.Maeder A.Schaerer D.2017-07-11T13:08:17Z1999-02-27T12:12:09ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelschemical-abundancesNew grids of models covering the evolution of low mass stars (0.8 to 1.7M{sun}) with metallicities Z=0.020 and 0.001 from the zero age main sequence up to the end of the early asymptotic giant branch are presented. The evolutionary tracks have been calculated with the new OPAL radiative opacities by Iglesias & Rogers (1992ApJ...397..717I) and Kurucz (1991). They complete the base of extensive grids of stellar models computed by the Geneva Group with up-to-date input physics (Schaller et al. 1992, Cat. J/A+AS/115/339; Schaerer et al. 1992, Cat. J/A+AS/98/523; Charbonnel et al. 1993, Cat. J/A+AS/101/415; Schaerer et al. 1993, Cat. J/A+AS/102/339; Meynet et al. 1994, Cat. J/A+AS/103/97).1996A&AS..115..339Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/115/339CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/96/269 : (I) z=0.01, 0.02 (Schaller et al., 1992)J/A+AS/98/523 : (II) z=0.008 (Schaerer et al., 1992)J/A+AS/101/415 : (III) z=0.004 (Charbonnel et al., 1993)J/A+AS/102/339 : (IV) z=0.04 (Schaerer et al., 1993)J/A+AS/103/97 : (V) z=0.001, 0.004, 0.008, 0.020 and 0.040J/A+AS/128/471 : (VII) z=0.10 (Mowlavi et al., 1998)J/A+AS/135/405 : (VIII) z=0.020, 0.001 (Charbonnel et al., 1999)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/115/339https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/115/339http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/115/339https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/115/339https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/115/339http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/115/339GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+AS/115/339/modelsCombined table from original tablesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTnoNumber of table in the publicationmeta.id;meta.datasetcharMoStar initial masssolMassphys.massfloatnullableZoStar initial metallicity: 0.001 or 0.020phys.abund.ZfloatnullableOSimbad column added by the CDSmeta.notecharMdSimbad column added by the CDSmeta.noteintnullableNoNumber of selected pointmeta.idintAgeAgeyrtime.agedoubleMassActual masssolMassphys.massdoublelog(L)Luminositylog(solLum)phys.luminosityfloatlog(Te)Effective temperaturelog(K)phys.temperature.effectivefloatHsH surface abundance (mass fraction)phys.abund.FedoubleHesHe surface abundance (mass fraction)phys.abund.YdoubleC12^12^C surface abundance (mass fraction)meta.notedoubleC13^13^C surface abundance (mass fraction)meta.notedoubleN14^14^N surface abundance (mass fraction)meta.notedoubleO16^16^O surface abundance (mass fraction)meta.notedoubleO17^17^O surface abundance (mass fraction)meta.notedoubleO18^18^O surface abundance (mass fraction)meta.notedoubleNe20^20^Ne surface abundance (mass fraction)meta.notedoubleNe22^22^Ne surface abundance (mass fraction)meta.notedoubleMcoreCore mass fractionphys.massfloatlog(Tu)? Uncorrected Teff (WR stars only)log(K)phys.temperature.effectivefloatnullablelog(Mdot)Mass loss ratelog(solMass.yr**-1)phys.mass.lossfloatlog(rho)Central densitylog(g.cm**-3)phys.densityfloatlog(Tc)Central temperaturelog(K)phys.temperaturefloatHcH central abundance (mass fraction)phys.abund.FedoubleHec? He central abundance (mass fraction)phys.abund.YdoublenullableC12c? ^12^C central abundance (mass fraction)phys.abund;em.wl.centraldoublenullableC13c? ^13^C central abundance (mass fraction)phys.abund;em.wl.centraldoublenullableN14c? ^14^N central abundance (mass fraction)phys.abund;em.wl.centraldoublenullableO16c? ^16^O central abundance (mass fraction)phys.abund;em.wl.centraldoublenullableO17c? ^17^O central abundance (mass fraction)phys.abund;em.wl.centraldoublenullableO18c? ^18^O central abundance (mass fraction)phys.abund;em.wl.centraldoublenullableNe20c? ^20^Ne central abundance (mass fraction)phys.abund;em.wl.centraldoublenullableNe22c? ^22^Ne central abundance (mass fraction)phys.abund;em.wl.centraldoublenullable