J/A+AS/135/405ivo://CDS.VizieR/J/A+AS/135/405CDSCharbonnel C.Dappen W.Schaerer D.Bernasconi P.A.Maeder A.,Meynet G.Mowlavi N.2017-07-11T13:09:27Z1999-03-17T06:02:23ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelsstellar-mass-losshertzsprung-russell-diagramWe present stellar evolutionary models covering the mass range from 0.4 to 1M_{sun}_ calculated for metallicities Z=0.020 and 0.001 with the MHD equation of state (Hummer & Mihalas, 1988ApJ...331..794H, Mihalas et al., 1988ApJ...331..815M, Daeppen et al., 1988ApJ...332..261D). A parallel calculation using the OPAL (Rogers et al., 1996ApJ...456..902R) equation of state has been made to demonstrate the adequacy of the MHD equation of state in the range of 1.0 to 0.8M_{sun}_ (the lower end of the OPAL tables). Below, down to 0.4M_{sun}_, we have justified the use of the MHD equation of state by theoretical arguments and the findings of Chabrier & Baraffe (1997A&A...327.1039C). We use the radiative opacities by Iglesias & Rogers (1996ApJ...464..943I), completed with the atomic and molecular opacities by Alexander & Fergusson (1994ApJ...437..879A). We follow the evolution from the Hayashi fully convective configuration up to the redgiant tip for the most massive stars, and up to an age of 20Gyr for the less massive ones. We compare our solar-metallicity models with recent models computed by other groups and with observations.1999A&AS..135..405Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/135/405CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/96/269 : Paper I. 0.8 to 120 M_{sun}_, Z=0.020 (Schaller+, 1992)J/A+AS/98/523 : Paper II. 0.8 to 120 M_{sun}_, Z=0.008 (Schaerer+ 1993)J/A+AS/101/415 : Paper III. 0.8 to 120 M_{sun}_, Z=0.004 (Charbonnel+ 1993)J/A+AS/102/339 : Paper IV. 0.8 to 120 M_{sun}_, Z=0.040 (Schaerer+, 1993)J/A+AS/103/97 : Paper V. 12 to 120 M_{sun}_,J/A+AS/115/339 : Paper VI. HB abd AGB, Z=0.020, 0.001 (Charbonnel+, 1996)J/A+AS/128/471 : Paper VII. 0.8 to 60M_{sun}_, Z=0.10 (Mowlavi+ 1998)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/135/405https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/135/405http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/135/405https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/135/405https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/135/405http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/135/405GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+AS/135/405/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)log(luminosity)log(solLum)phys.luminosityfloatlog(Te)log(effective temperature)log(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.notedoubleQCCCore mass fractionphys.massdoublelog(Mdot)log(mass loss rate)log(solMass.yr**-1)phys.mass.lossfloatrhoclog(central density)log(g.cm**-3)arith.zpfloatlog(Tc)log(central temperature)log(K)arith.zpfloatHcH central abundance (mass fraction)phys.abund.FedoubleHecHe central abundance (mass fraction)phys.abund.YdoubleC12c^12^C central abundance (mass fraction)phys.abund;em.wl.centraldoubleC13c^13^C central abundance (mass fraction)phys.abund;em.wl.centraldoubleN14c^14^N central abundance (mass fraction)phys.abund;em.wl.centraldoubleO16c^16^O central abundance (mass fraction)phys.abund;em.wl.centraldoubleO17c^17^O central abundance (mass fraction)phys.abund;em.wl.centraldoubleO18c^18^O central abundance (mass fraction)phys.abund;em.wl.centraldoubleNe20c^20^Ne central abundance (mass fraction)phys.abund;em.wl.centraldoubleNe22c^22^Ne central abundance (mass fraction)phys.abund;em.wl.centraldouble