J/A+A/557/A106ivo://CDS.VizieR/J/A+A/557/A106doi:10.26093/cds/vizier.35570106CDSGil-Pons P.Doherty C.Lau H.Campbell S.Suda T.Guilani S.,Gutierrez J.Lattanzio J.C.2017-06-27T06:38:07Z2013-09-11T08:57:37ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelschemical-abundancesOur main goals are to get a deeper insight into the evolution and final fates of intermediate-mass, extremely metal-poor (EMP) stars. We also aim to investigate the C, N, and O yields of these stars. Using the Monash University Stellar Evolution code MONSTAR we computed and analysed the evolution of stars of metallicity Z=10^-5^ and masses between 4 and 9M_{sun}_, from their main sequence until the late thermally pulsing (super)asymptotic giant branch, TP-(S)AGB phase.2013A&A...557A.106Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/557/A106CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/123/305 : Yields of intermediate mass stars (van den Hoek+ 1997)J/A+A/416/1117 : Abundances in the early Galaxy (Cayrel+, 2004)J/ApJS/155/651 : Evolution of extremely metal-poor stars (Herwig+, 2004)J/A+A/432/861 : Yields of low and intermediate mass stars (Gavilan+, 2005)J/ApJ/608/405 : Massive star explosive yields (z=0-z_{Sun}_) (Chieffi+, 2005)J/A+A/490/769 : Yields from extremely metal-poor stars (Campbell+, 2008)J/ApJ/696/797 : Evolution and yields of low-mass AGB stars (Cristallo+, 2009)J/MNRAS/403/1413 : Updated stellar yields from AGB models (Karakas, 2010)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/557/A106https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/557/A106http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/557/A106https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/557/A106https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/557/A106http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/557/A106GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/557/A106/evohr040Model stars for Z=10^-5^ and M=4M_{sun}_recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogTeffEffective temperaturelog(K)phys.temperature.effectivedoublelogLSurface luminositylog(solLum)phys.luminositydoubleJ/A+A/557/A106/evohr050Model stars for Z=10^-5^ and M=5M_{sun}_recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogTeffEffective temperaturelog(K)phys.temperature.effectivedoublelogLSurface luminositylog(solLum)phys.luminositydoubleJ/A+A/557/A106/evohr060Model stars for Z=10^-5^ and M=6M_{sun}_recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogTeffEffective temperaturelog(K)phys.temperature.effectivedoublelogLSurface luminositylog(solLum)phys.luminositydoubleJ/A+A/557/A106/evohr070Model stars for Z=10^-5^ and M=7M_{sun}_recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogTeffEffective temperaturelog(K)phys.temperature.effectivedoublelogLSurface luminositylog(solLum)phys.luminositydoubleJ/A+A/557/A106/evohr080Model stars for Z=10^-5^ and M=8M_{sun}_recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogTeffEffective temperaturelog(K)phys.temperature.effectivedoublelogLSurface luminositylog(solLum)phys.luminositydoubleJ/A+A/557/A106/evohr090Model stars for Z=10^-5^ and M=9M_{sun}_recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogTeffEffective temperaturelog(K)phys.temperature.effectivedoublelogLSurface luminositylog(solLum)phys.luminositydoubleJ/A+A/557/A106/esurf040Time evolution of surface abundances M=4M_{sun}_xsH? H surface abundancephys.abund.XdoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTimeTimeyrtime.agedoublexs3He? ^3^He surface abundancemeta.notedoublenullablexs4He? ^4^He surface abundancemeta.notedoublenullablexs12C? ^12^C surface abundancephys.abunddoublenullablexs14N? ^14^N surface abundancephys.abunddoublenullablexs16O? ^16^O surface abundancephys.abunddoublenullablexsZotZ_other_ surface abundancephys.abunddoubleJ/A+A/557/A106/esurf050Time evolution of surface abundances M=5M_{sun}_recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTimeTimeyrtime.agedoublexsH? H surface abundancephys.abund.Xdoublenullablexs3He? ^3^He surface abundancemeta.notedoublenullablexs4He? ^4^He surface abundancemeta.notedoublenullablexs12C? ^12^C surface abundancephys.abunddoublenullablexs14N? ^14^N surface abundancephys.abunddoublenullablexs16O? ^16^O surface abundancephys.abunddoublenullablexsZotZ_other_ surface abundancephys.abunddoubleJ/A+A/557/A106/esurf060Time evolution of surface abundances M=6M_{sun}_recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTimeTimeyrtime.agedoublexsH? H surface abundancephys.abund.Xdoublenullablexs3He? ^3^He surface abundancemeta.notedoublenullablexs4He? ^4^He surface abundancemeta.notedoublenullablexs12C? ^12^C surface abundancephys.abunddoublenullablexs14N? ^14^N surface abundancephys.abunddoublenullablexs16O? ^16^O surface abundancephys.abunddoublenullablexsZotZ_other_ surface abundancephys.abunddoubleJ/A+A/557/A106/esurf070Time evolution of surface abundances M=7M_{sun}_recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTimeTimeyrtime.agedoublexsH? H surface abundancephys.abund.Xdoublenullablexs3He? ^3^He surface abundancemeta.notedoublenullablexs4He? ^4^He surface abundancemeta.notedoublenullablexs12C? ^12^C surface abundancephys.abunddoublenullablexs14N? ^14^N surface abundancephys.abunddoublenullablexs16O? ^16^O surface abundancephys.abunddoublenullablexsZotZ_other_ surface abundancephys.abunddoubleJ/A+A/557/A106/esurf080Time evolution of surface abundances M=8M_{sun}_recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTimeTimeyrtime.agedoublexsH? H surface abundancephys.abund.Xdoublenullablexs3He? ^3^He surface abundancemeta.notedoublenullablexs4He? ^4^He surface abundancemeta.notedoublenullablexs12C? ^12^C surface abundancephys.abunddoublenullablexs14N? ^14^N surface abundancephys.abunddoublenullablexs16O? ^16^O surface abundancephys.abunddoublenullablexsZotZ_other_ surface abundancephys.abunddoubleJ/A+A/557/A106/esurf090Time evolution of surface abundances M=9M_{sun}_xsZotZ_other_ surface abundancephys.abunddoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTimeTimeyrtime.agedoublexsH? H surface abundancephys.abund.Xdoublenullablexs3He? ^3^He surface abundancemeta.notedoublenullablexs4He? ^4^He surface abundancemeta.notedoublenullablexs12C? ^12^C surface abundancephys.abunddoublenullablexs14N? ^14^N surface abundancephys.abunddoublenullablexs16O? ^16^O surface abundancephys.abunddoublenullable