J/MNRAS/408/827ivo://CDS.VizieR/J/MNRAS/408/827doi:10.26093/cds/vizier.74080827CDSDessart L.Livne E.Waldman R.2024-07-12T20:14:49Z2011-06-03T16:07:57ZCDS support team

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

cds-question@unistra.frsupernovaeastronomical-modelsstellar-atmospheresWe present radiation-hydrodynamic simulations of core-collapse supernova (SN) explosions, artificially generated by driving a piston at the base of the envelope of a rotating or non-rotating red-supergiant progenitor star. We search for trends in ejecta kinematics in the resulting Type II-Plateau (II-P) SN, exploring dependencies with explosion energy and pre-SN stellar-evolution model.2010MNRAS.408..827Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/408/827CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/408/827https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/408/827http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/408/827https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/408/827https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/408/827http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/408/827GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/MNRAS/408/827/table1Summary of the properties for a representative sample of pre-SN models employed in this studyrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintModelPre-SN model designation (1)meta.id;meta.maincharMiInitial mass (i.e. the main-sequence mass)solMassphys.massfloatMfFinal mass (i.e. the mass at core collapse)solMassphys.massfloatMcoreLagrangian mass delimiting outer edge of the coresolMassphys.massfloatMeOLagrangian mass delimiting outer edge of the oxygen (O) shellsolMassphys.massfloatMeHeLagrangian mass delimiting outer edge of the helium (He) shellsolMassphys.massfloatMiHLagrangian mass delimiting inner edge of the hydrogen (H) shellsolMassphys.massfloatMHenvMass of the hydrogen-rich envelopesolMassphys.massfloatDRSize of the hydrogen-rich envelope (in 10^13^cm)1e+08kmphys.size.radiusfloatR*surface radius (in 10^13^cm)1e+08kmphys.size.radiusfloatEgravGravitational energy of the progenitor envelope outside of Mcore (in 10^51^erg)1e+44Jphys.energyfloatEbindBinding energy of the progenitor envelope outside of Mcore (in 10^51^erg)1e+44Jphys.energyfloatJ/MNRAS/408/827/simulSummary of properties (tables 2-7 of the paper)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintCase[2/7] Model cases (1)meta.id;stat.fitintMiInitial masssolMassphys.massfloatEkinasymptotic ejecta kinetic energy1e+44Wphys.energyfloatMpPiston mass cutsolMassphys.massfloatVpPiston speedkm/sphys.velocintMfFinal masssolMassphys.massfloatMremMass of the remnant (2)solMassphys.massfloatMejMass of the ejectasolMassphys.massfloatVinnerMean velocity of the inner 0.1M_{sun}_ of the ejectakm/sphys.veloc;stat.meanintVeOVelocity at the outer edge of the oxygen shellkm/sphys.velocintViHVelocity at the inner edge of the hydrogen shellkm/sphys.velocintVp15dPhotospheric velocity at 15d after shock breakoutkm/sphys.velocintVp50dPhotospheric velocity at 50d after shock breakoutkm/sphys.velocintEejEffective asymptotic ejecta kinetic energy (in 10^51^erg)1e+44Wphys.energyfloatf(H)Fraction endowed by the hydrogen-rich part of the ejecta%phys.mass;arith.ratiointMOEjected oxygen masssolMassphys.massfloattSBODelay time between the piston trigger and shock breakoutdtime.intervalfloatdtPPlateau duration (3)dtime.intervalfloatSimSimulation Namemeta.id;stat.fitchar