J/A+AS/128/471ivo://CDS.VizieR/J/A+AS/128/471CDSMowlavi N.Schaerer D.Meynet G.Bernasconi P.A.Charbonnel C.Maeder A.2017-07-12T07:00:07Z1998-04-25T15:05:55ZCDS 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 a new grid of stellar models from 0.8 to 60M_{sun}_ at Z=0.10, with mass loss and moderate overshooting, from the zero age main sequence to either the helium flash (low mass stars), the early AGB phase (intermediate-mass stars or the end of carbon burning (massive stars). The calculations are done with opacities provided by Iglesias & Rogers (1993ApJ...412..752I), completed by those of Alexander & Ferguson (1994ApJ...437..879A) at low temperatures. This grid is a homogeneous extension to very high metallicity of the previous grids published by the Geneva group. It is useful for the study of galactic bulges, elliptical galaxies and eventually quasars. Calculations of stars more massive than 60M_{sun}_ are not presented as these objects lose almost their entire mass during their main sequence phase, and are likely to end their life as white dwarfs.1998A&AS..128..471Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/128/471CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/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/135/405 : Grids of stellar models. VIII. (Charbonnel+ 1999)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/128/471https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/128/471http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/128/471https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/128/471https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/128/471http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/128/471GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+AS/128/471/modelsCombined table from original tablesO17^17^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.massfloatrecnoRecord 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 mass in solar massessolMassphys.massdoublelog(L)log(luminosity) in solar unitslog(solLum)phys.luminosityfloatlog(Te)log(effective temperature)log(K)phys.temperature.effectivefloatXH surface abundance (mass fraction)phys.abund.FedoubleYHe 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.notedoublelog(Tu)? log(uncorrected Teff) (WR stars only)log(K)arith.zpfloatnullablelog(Mdot)log(mass loss rate)log(solMass.yr**-1)phys.mass.lossfloatlog(rho.c)log(central density)log(g.cm**-3)arith.zpfloatlog(Tc)log(central temperature)log(K)arith.zpfloatXcH central abundance (mass fraction)phys.abund.FedoubleYcHe 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