J/MNRAS/403/1413ivo://CDS.VizieR/J/MNRAS/403/1413doi:10.26093/cds/vizier.74031413CDSKarakas A.I.2024-07-10T20:17:28Z2010-11-09T11:10:49ZCDS support team

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

cds-question@unistra.frastronomical-modelsgiant-starschemical-abundancesAn updated grid of stellar yields for low- to intermediate-mass thermally pulsing asymptotic giant branch (AGB) stars is presented. The models cover a range in metallicity Z=0.02, 0.008, 0.004 and 0.0001, and masses between 1 and 6M_{sun}_. New intermediate-mass (M>=3M_{sun}_) Z=0.0001 AGB models are also presented, along with a finer mass grid than used in previous studies. The yields are computed using an updated reaction rate network that includes the latest NeNa and MgAl proton capture rates.2010MNRAS.403.1413Khttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/403/1413CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/107/445 : Envelopes of oxygen-rich AGB stars (Hashimoto, 1994)J/ApJS/92/125 : Post-AGB evolution (Vassiliadis+, 1994)J/A+AS/126/39 : Models of circumstellar dust shells (Steffen+ 1997)J/A+A/512/A10 : Evolution of massive AGB stars. III. (Siess, 2010)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/403/1413https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/403/1413http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/403/1413https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/403/1413https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/403/1413http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/403/1413GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/MNRAS/403/1413/tablea1Structural information from the new AGB modelsM0[1/6] Initial masssolMassphys.massfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZ0Initial metallicity (0.0200, 0.0080, 0.0040, 0.0001)phys.abund.ZfloatPulsePulse numbermeta.idintMcoreCore masssolMassphys.massfloatMcshMaximum mass of the intershell convection zonesolMassphys.massdoubletcshDuration of intershell convectionyrtime.intervalfloatDdredgeMass dredged into the envelopesolMassphys.massdoublelamExtent of the partial mixing zone, lambdastat.fit.paramdoublelam.dup{lambda}_dup_ defined by Goriely & Mowlavi (2000A&A...362..599G) (1)stat.fit.paramdoubleT(He-sh)Maximum temperature in the He-shellKphys.temperaturedoubleTbceMaximum temperature at the base of the convective envelope during the previous interpulse periodKphys.temperaturedoubleT(H-sh)Maximum temperature in the H-shell during the previous interpulse periodKphys.temperaturedoubleiPulseInterpulse period (note that the first entry is set to zero)yrtime.perioddoubleMtotTotal masssolMassphys.massfloatLmaxMaximum radiated luminosity during the previous interpulse periodsolLumphys.luminositydoubleLHe.maxMaximum He-luminosity during a thermal pulsesolLumphys.luminositydoubleRmaxMaximum stellar radius during the previous interpulse periodsolRadphys.size.radius;stat.maxdoubleMbolBolometric magnitudemagphys.magAbs.bolfloatTeffEffective temperatureKphys.temperature.effectivefloatYieldsYields for the various elementsmeta.ref.urlcharJ/MNRAS/403/1413/yieldsStellar yieldsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintM0[1/6.5] Initial masssolMassphys.massfloatMixSimbad column added by the CDSstat.paramcharZ0Initial metallicityphys.abund.ZfloatM1Final mass (1)solMassphys.massfloatElSpecies i (2)phys.atmol.elementcharAAtomic mass of the species iphys.massintYieldNet yieldsolMassphys.composition.yielddoubleM(i)lostMass of species i lost in the windsolMassphys.massdoubleM(i)0Mass of species i initially present in the windsolMassphys.massdouble<X(i)>Average abundance of species i in the wind (mass fraction)phys.abunddoubleX0(i)initial mass fraction of species i (mass fraction)phys.massdoublefProduction factor, f=log10(<X(i)>/X0(i))arith.factordouble