J/ApJ/608/405ivo://CDS.VizieR/J/ApJ/608/405doi:10.26093/cds/vizier.16080405CDSChieffi A.Limongi M.2017-10-06T09:39:16Z2005-09-02T23:53:34ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelssupernovaechemical-abundancesWe present a new and homogeneous set of explosive yields for masses 13, 15, 20, 25, 30, and 35M_{sun}_ and metallicities Z=0, 10^-6^, 10^-4^, 10^-3^, 6x10^-3^, and 2x10^-2^. A wide network extending up to Mo has been used in all computations. We show that at low metallicities (Z<=10^-4^), the final yields do not depend significantly on the initial chemical composition of the models, so a scaled solar distribution may be safely assumed at all metallicities. Moreover, no elements above Zn are produced by any mass in the grid up to a metallicity ~10-3. These yields are available for any choice of the mass cut on request.2004ApJ...608..405Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/608/405CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/608/405https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/608/405http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/608/405https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/608/405https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/608/405http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/608/405GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/ApJ/608/405/yieldsExplosive yields (from table1)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZMetallicity of the modelphys.abund.Z;meta.modelledfloattDate after explosion (0 or 2.510^4^s)stime.agedoubleAAtomic mass of the element (1)phys.atmol.elementintElElement name or parameter (1)meta.id;phys.atmol.elementcharM13ElMass of element (A, El) if Mini=13solMasssolMassstat.paramdoubleM15ElMass of element (A, El) if Mini=15solMasssolMassstat.paramdoubleM20ElMass of element (A, El) if Mini=20solMasssolMassstat.paramdoubleM25ElMass of element (A, El) if Mini=25solMasssolMassstat.paramdoubleM30ElMass of element (A, El) if Mini=30solMasssolMassstat.paramdoubleM35ElMass of element (A, El) if Mini=35solMasssolMassstat.paramdouble