J/ApJS/155/651ivo://CDS.VizieR/J/ApJS/155/651doi:10.26093/cds/vizier.21550651CDSHerwig F.2017-06-13T11:08:34Z2007-04-15T17:04:40ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelschemical-abundancesIntermediate-mass stellar evolution tracks from the main sequence to the tip of the AGB for five initial masses (2-6M_{sun}_) and metallicity Z=0.0001 have been computed. The detailed one-dimensional structure and evolution models include exponential overshooting, mass loss, and a detailed nucleosynthesis network with updated nuclear reaction rates. The network includes a two-particle heavy neutron sink for approximating neutron density in the He-shell flash. It is shown how the neutron-capture nucleosynthesis is important in models of very low metallicity for the formation of light neutron-heavy species, like sodium or the heavy neon and magnesium isotopes. The models have high resolution, as required for modeling the third dredge-up. All sequences have been followed from the pre-main sequence to the end of the AGB when all envelope mass is lost. Detailed structural and chemical model properties as well as yields are presented. This set of stellar models is based on standard assumptions and updated input physics. It can be confronted with observations of extremely metal-poor stars and may be used to assess the role of AGB stars in the origin of abundance anomalies of some globular cluster members of correspondingly low metallicity.2004ApJS..155..651Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/155/651CatalogResearchIsServedByTAP VizieR generic servicerelated-toVI/65 : Evolutionary models of evolved stars (Dorman+ 1993)VI/96 : Evolutionary Sequences (Fagotto+ 1993-96)VI/109 : Population Synthesis Models at very low metallicitiesVI/118 : Stellar Models until He burning (Claret+ 1995-1998)J/A+A/299/755 : Stellar evolution. II. Post-AGB (Bloecker+, 1995)J/A+A/401/1063 : Evolutionary synthesis models. III. (Anders+, 2003)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)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/155/651https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/155/651http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/155/651https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/155/651https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/155/651http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/155/651GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/ApJS/155/651/table1Reaction networkrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTypeType of reactionmeta.noteIDIdentification number of the reactionmeta.idintReactReaction descriptionmeta.notecharr_ReactReference for React (1)meta.bibcharJ/ApJS/155/651/table5YieldsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNumSequential number of the speciesmeta.idintSpeciesSpecies name (as in table6)phys.atmol.elementcharE82The 2 solar mass (E82) model yield (1)solMassphys.composition.yielddoubleE84The 3 solar mass (E84) model yield (1)solMassphys.composition.yielddoubleE85The 4 solar mass (E85) model yield (1)solMassphys.composition.yielddoubleE79The 5 solar mass (E79) model yield (1)solMassphys.composition.yielddoubleE86The 6 solar mass (E86) model yield (1)solMassphys.composition.yielddoubleJ/ApJS/155/651/table6Structure and abundance evolution of computed tracksG63G63 surface abundancephys.abunddoubleL1L1 surface abundancephys.abunddoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSequence name (E79, E82, E84, E85, E86)meta.id;stat.fitcharModelModel numbermeta.idintMassStellar masssolMassphys.massfloatAgeAge (Zero at first TP (thermal-pulse))yrtime.agedoublelogTeffLog of the effective temperaturelog(K)phys.temperature.effectivefloatlogLLog of the luminosity in solar unitslog(solLum)phys.luminosityfloatHH surface abundancephys.abund.XdoubleHe4He4 surface abundancephys.abunddoubleC12C12 surface abundancemeta.notedoubleC13C13 surface abundancemeta.notedoubleN14N14 surface abundancemeta.notedoubleN15N15 surface abundancephys.abunddoubleO16O16 surface abundancemeta.notedoubleO17O17 surface abundancemeta.notedoubleO18O18 surface abundancemeta.notedoubleNe20Ne20 surface abundancemeta.notedoubleNe21Ne21 surface abundancephys.abunddoubleNe22Ne22 surface abundancemeta.notedoubleNa23Na23 surface abundancephys.abunddoubleMg24Mg24 surface abundancephys.abunddoubleMg25Mg25 surface abundancephys.abunddoubleMg26Mg26 surface abundancephys.abunddoubleAl26GAl26G surface abundancephys.abunddoubleAl27Al27 surface abundancephys.abunddoubleSi28Si28 surface abundancephys.abunddoubleSi29Si29 surface abundancephys.abunddoubleSi30Si30 surface abundancephys.abunddouble