J/ApJ/870/1ivo://CDS.VizieR/J/ApJ/870/1doi:10.26093/cds/vizier.18700001CDSEbinger K.Curtis S.Frohlich C.Hempel M.Perego A.Liebendorfer M.,Thielemann F.-K.2021-01-05T12:55:46Z2020-03-03T16:23:36ZCDS support team

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

cds-question@unistra.frsupernovaestellar-massesastronomical-modelsIn a previously presented proof-of-principle study, we established a parameterized spherically symmetric explosion method (PUSH) that can reproduce many features of core-collapse supernovae (CCSN). The present paper goes beyond a specific application that is able to reproduce observational properties of SN1987A and performs a systematic study of an extensive set of nonrotating, solar metallicity stellar progenitor models in the mass range from 10.8 to 120M_{sun}_. This includes the transition from neutron stars to black holes as the final result of the collapse of massive stars, and the relation of the latter to supernovae, possibly faint supernovae, and failed supernovae. We discuss the explosion properties of all models and predict remnant mass distributions within this approach. The present paper provides the basis for extended nucleosynthesis predictions in a forthcoming paper to be employed in galactic evolution models.2019ApJ...870....1Ehttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/870/1CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/ApJ/608/405 : Explosive yields of massive star (Chieffi+, 2004)J/AJ/131/2245 : BATC photometry of SN2004dj (Zhang+, 2006)J/MNRAS/372/1315 : UBVRI photometry of SN 2004et (Sahu+, 2006)J/ApJ/724/341 : Nucleosynthesis of massive metal-free stars (Heger+, 2010)J/MNRAS/408/827 : Simulations of supernova explosions (Dessart+, 2010)J/ApJS/199/38 : Presupernova evolution (Limongi+, 2012)J/ApJ/764/21 : Stellar evolutionary models with 13-120Msun (Chieffi+, 2013)J/ApJ/769/99 : Nucleosynthetic yields for stars >12M{sun} (Brown+, 2013)J/MNRAS/433/1871 : UBVRI griz light curves of SN 2012aw (Bose+, 2013)J/ApJ/808/42 : CHemical Abundances of Spirals II. M51 (Croxall+, 2015)J/ApJ/824/6 : Obs. of precursor to SNHunt275 2015 May event (Ofek+, 2016)J/A+A/624/A66 : Massive runaway and walkaway stars models (Renzo+, 2019)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/870/1https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/870/1http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/870/1https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/870/1https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/870/1http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/870/1GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/ApJ/870/1/table5WHW02 and WH07 models (standard calibration)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintModelModel identifier; WHW02 or WH07 (1)meta.id;stat.param;meta.modelledcharMzams[10/120] Zero-age main sequence (ZAMS) masssolMassphys.massfloatMprog[6/17] Progenitor masssolMassphys.massfloatEexpl[0.5/1.7] Explosion energy; in 10^51^erg units1e+44Jphys.energyfloattexpl[0.26/0.56] Time of explosionstime.epochfloatMNi[0.02/0.16] Ejected mass of ^56^NisolMassphys.massdoubleMrem[1.3/2] Remnant masssolMassphys.massfloat