J/A+A/341/709ivo://CDS.VizieR/J/A+A/341/709doi:10.26093/cds/vizier.33410709CDSLindner U.Fritze - von Alvensleben U.Fricke K.J.1999-01-24T15:09:07Z1999-01-24T16:08:54ZCDS support team

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

cds-question@unistra.frchemical-abundancesstellar-evolutionary-modelsWe have extended our chemical and cosmological galaxy evolution model to calculate the abundance evolution for altogether 16 different elements in spiral galaxies in a chemically consistent way which is a considerable step towards a more realistic galaxy modeling. All observed element abundances in Damped Lyman {alpha} (LDA) systems have been compiled.1999A&A...341..709Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/341/709CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/123/305 : Yields of intermediate mass stars (van den Hoek+ 1997)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/341/709https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/341/709http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/341/709https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/341/709https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/341/709http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/341/709GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/341/709/table5SNII yields calculated by Woosley & Weaver (1995ApJS..101..181W) for models A, B and C (see text) and two different metallicities Z=Z_{sun}_ and Z=0.01 Z_{sun}_.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNote[AS] A: model A; S: SNIa (1)meta.notecharZ? Initial metallicitySunphys.abund.ZfloatnullableMass? Stellar masssolMassphys.massintnullablen_Mass[** ] Note on model (2)meta.notecharHH yield (3)phys.composition.yieldfloatHeHe yield (3)phys.composition.yieldfloatCC yield (3)phys.composition.yieldfloatNN yield (3)phys.composition.yieldfloatOO yield (3)phys.composition.yieldfloatMgMg yield (3)phys.composition.yieldfloatAlAl yield (3)phys.composition.yieldfloatSiSi yield (3)phys.composition.yieldfloatSS yield (3)phys.composition.yieldfloatArAr yield (3)phys.composition.yieldfloatCaCa yield (3)phys.composition.yieldfloatFeFe yield (3)phys.composition.yieldfloatNiNi yield (3)phys.composition.yieldfloatZnZn yield (3)phys.composition.yieldfloatCrCr yield (3)phys.composition.yieldfloatMnMn yield (3)phys.composition.yieldfloatMeject? Total ejected mass (4)solMassphys.massfloatnullableDiff? Difference between Meject and the sum of ejecta given in this table for elements H, He, ..., Mn%stat.paramfloatnullableJ/A+A/341/709/table6Stellar yields for various stellar masses and three different initial metallicities Z=1, 0.2 and 0.05Z_{sun}_ from van den Hoek & Groenewegen (1997, Cat. <J/A+AS/123/305>)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMassStellar masssolMassphys.massfloatH1H yield for Z=1.0 Z_{sun}_phys.composition.yieldfloatH2H yield for Z=0.2 Z_{sun}_phys.composition.yieldfloatH3H yield for Z=0.05Z_{sun}_phys.composition.yieldfloatHe1He yield for Z=1.0 Z_{sun}_phys.composition.yieldfloatHe2He yield for Z=0.2 Z_{sun}_phys.composition.yieldfloatHe3He yield for Z=0.05Z_{sun}_phys.composition.yieldfloatC1C yield for Z=1.0 Z_{sun}_phys.composition.yieldfloatC2C yield for Z=0.2 Z_{sun}_phys.composition.yieldfloatC3C yield for Z=0.05Z_{sun}_phys.composition.yieldfloatN1N yield for Z=1.0 Z_{sun}_phys.composition.yieldfloatN2N yield for Z=0.2 Z_{sun}_phys.composition.yieldfloatN3N yield for Z=0.05Z_{sun}_phys.composition.yieldfloatO1O yield for Z=1.0 Z_{sun}_phys.composition.yieldfloatO2O yield for Z=0.2 Z_{sun}_phys.composition.yieldfloatO3O yield for Z=0.05Z_{sun}_phys.composition.yieldfloatJ/A+A/341/709/table7Stellar lifetimes for two different initial metallicities.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintl_Mass[~] Limit flag on massmeta.code.errorcharMassStellar masssolMassphys.massfloatl_Tau1[~] Limit flag on Tau1meta.code.errorcharTau1Stellar lifetime for Z=1.00Z_{sun}_Gyrtime.agedoubleTau2Stellar lifetime for Z=0.05Z_{sun}_Gyrtime.agedoubleJ/A+A/341/709/table8SNII remnants of various progenitor masses, five different initial metallicities Z and three explosion models (A, B and C) from Table3 in Woosley & Weaver (1995ApJS..101..181W)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMassStellar masssolMassphys.massintn_Mass[** ] Note on model (1)meta.notecharR1SN II remnant for Z=1.0000Z_{sun}_solMassphys.massfloatR2SN II remnant for Z=0.1000Z_{sun}_solMassphys.massfloatR3SN II remnant for Z=0.0100Z_{sun}_solMassphys.massfloatR4SN II remnant for Z=0.0001Z_{sun}_solMassphys.massfloatR5SN II remnant for Z=0.0000Z_{sun}_solMassphys.massfloatJ/A+A/341/709/table9Remnants for different stellar masses and initial metallicities (Z=1, 0.2 and 0.05Z_{sun}_) from van den Hoek & Groenewegen (1997, Cat. <J/A+AS/123/305>)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMassMasssolMassphys.massfloatR1Remnant for Z=1.0Z_{sun}_solMassphys.massfloatR2? Remnant for Z=0.2Z_{sun}_solMassphys.massfloatnullableR3? Remnant for Z=0.05Z_{sun}_solMassphys.massfloatnullable