J/ApJ/664/1033ivo://CDS.VizieR/J/ApJ/664/1033doi:10.26093/cds/vizier.16641033CDSYoung P.A.Fryer C.L.2017-06-01T08:52:41Z2009-11-05T21:45:23ZCDS support team

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

cds-question@unistra.frastronomical-modelssupernova-remnantssupernovaeTheoretical nucleosynthetic yields from supernovae are sensitive to both the details of the progenitor star and the explosion calculation. We attempt to comprehensively identify the sources of uncertainties in these yields. In this paper we concentrate on the variations in yields from a single progenitor arising from common 1D methods of approximating a supernova explosion. Subsequent papers will examine 3D effects in the explosion and the progenitor, and trends in mass and composition. For the 1D explosions we find that both elemental and isotopic yields for Si and heavier elements are a sensitive function of explosion energy. Also, piston-driven and thermal bomb-type explosions have different yields for the same explosion energy. Yields derived from 1D explosions are nonunique.2007ApJ...664.1033Yhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/664/1033CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/664/1033https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/664/1033http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/664/1033https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/664/1033https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/664/1033http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/664/1033GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/ApJ/664/1033/yieldsDetailed yields before radioactive decay for all simlationsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAIsotopic mass id elementphys.atmol.weightintElElement identificationmeta.id;phys.atmol.elementchar23e-0.8Yield for the 23e-0.8 model (1)solMassphys.composition.yielddouble23e-1.1Yield for the 23e-1.1 model (1)solMassphys.composition.yielddouble23e-1.2Yield for the 23e-1.2 model (1)solMassphys.composition.yielddouble23e-1.4Yield for the 23e-1.4 model (1)solMassphys.composition.yielddouble23e-1.5Yield for the 23e-1.5 model (1)solMassphys.composition.yielddouble23e-2.0Yield for the 23e-2.0 model (1)solMassphys.composition.yielddouble23p-0.9Yield for the 23p-0.9 model (2)solMassphys.composition.yielddouble23p-1.2Yield for the 23p-1.2 model (2)solMassphys.composition.yielddouble23p-1.6Yield for the 23p-1.6 model (2)solMassphys.composition.yielddoubled0.2s0.8Yield for the d0.2s0.8 model (3)solMassphys.composition.yielddoubled0.2s1.5Yield for the d0.2s1.5 model (3)solMassphys.composition.yielddoubled0.7s0.8Yield for the d0.7s0.8 model (3)solMassphys.composition.yielddoubled0.7s1.5Yield for the d0.7s1.5 model (3)solMassphys.composition.yielddouble