J/ApJS/237/13ivo://CDS.VizieR/J/ApJS/237/13doi:10.26093/cds/vizier.22370013CDSLimongi M.Chieffi A.2019-01-07T09:40:46Z2018-10-22T13:31:22ZCDS support team

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

cds-question@unistra.frastronomical-modelssupernovaestellar-massesmetallicityWe present a new grid of presupernova models of massive stars extending in mass between 13 and 120M_{sun}_, covering four metallicities (i.e., [Fe/H]=0, -1, -2, and -3) and three initial rotation velocities (i.e., 0, 150, and 300km/s). The explosion has been simulated following three different assumptions in order to show how the yields depend on the remnant mass-initial mass relation. An extended network from H to Bi is fully coupled to the physical evolution of the models. The main results can be summarized as follows. (a) At solar metallicity, the maximum mass exploding as a red supergiant (RSG) is of the order of 17M_{sun}_ in the nonrotating case, with the more massive stars exploding as Wolf-Rayet (WR) stars. All rotating models, conversely, explode as WR stars. (b) The interplay between the core He-burning and the H-burning shell, triggered by the rotation-induced instabilities, drives the synthesis of a large primary amount of all the products of CNO, not just ^14^N. A fraction of them greatly enriches the radiative part of the He core (and is responsible for the large production of F), and a fraction enters the convective core, leading therefore to an important primary neutron flux able to synthesize heavy nuclei up to Pb. (c) In our scenario, remnant masses of the order of those inferred from the first detections of gravitational waves (GW 150914, GW 151226, GW 170104, GW 170814) are predicted at all metallicities for none or moderate initial rotation velocities.2018ApJS..237...13Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/237/13CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/416/1117 : Abundances in the early Galaxy (Cayrel+, 2004)J/ApJ/608/405 : Explosive yields of massive star (Chieffi+, 2004)J/A+A/479/541 : VLT-FLAMES survey of massive stars (Hunter+, 2008)J/A+A/496/841 : VLT-FLAMES survey of massive stars (Hunter+, 2009)J/MNRAS/408/827 : Simulations of supernova explosions (Dessart+, 2010)J/ApJ/724/341 : Nucleosynthesis of massive metal-free stars (Heger+, 2010)J/A+A/530/A115 : Rotating massive MS stars evolutionary models (Brott+, 2011)J/AJ/144/130 : Rotational velocities of nearby HIP B stars (Braganca+, 2012)J/A+A/537/A146 : Stellar models with rotation. 0.8<M<120 (Ekstrom+, 2012)J/ApJS/199/38 : Presupernova evolution (Limongi+, 2012)J/ApJ/764/21 : Stellar evolutionary models with 13-120Msun (Chieffi+, 2013)J/A+A/558/A131 : Model spectra of hot stars at the pre-SN stage (Groh+, 2013)J/A+A/600/A81 : VLTS. 30Dor O giants and supergiants (Ramirez-Agudelo+, 2017)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/237/13https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/237/13http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/237/13https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/237/13https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/237/13http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/237/13GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/ApJS/237/13/table7Properties of the presupernova modelsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintVel[0/300] Velocitykm/sphys.veloc;meta.modelledint[Fe/H][-3/0] Metallicitylog(Sun)phys.abund.ZintMass[13/120] Initial masssolMassphys.massintH[0/24.2] Hydrogen present in the envelopesolMassphys.abund.XfloatHe[0.4/26.5] Helium present in the envelopesolMassphys.abund.YfloatFe[1/2.8] Iron core mass (1)solMassphys.massfloatEbind[0.6/47.6] Binding energy; 1e+51erg (2)1e+44Jphys.energyfloatxi2.5[0.02/0.6] Compactness parametermeta.code;phys.sizefloatJFe[0/0.2] Angular momentum within iron core (3)1e+44J.sphys.angMomentumfloatJCO[0/11.4] Angular momentum within CO core (3)1e+44J.sphys.angMomentumfloatJHe[0/19.1] Angular momentum within He core (3)1e+44J.sphys.angMomentumfloatJ1.5[0/0.06] Angular momentum within inner 1.5M_{sun}_ (3)1e+44J.sphys.angMomentumfloatJ2.0[0/0.2] Angular momentum within inner 2.0M_{sun}_ (3)1e+44J.sphys.angMomentumfloatSNTypeExpected supernova type (SNIIP: 50 occurrences; or SNIb) (4)src.classcharJ/ApJS/237/13/table8Isotopic yields - Recommended setIsoIsotope identifiermeta.id;phys.molcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintVel[0/300] Velocitykm/sphys.veloc;meta.modelledint[Fe/H][-3/0] Metallicitylog(Sun)phys.abund.Zint13M[2.8e-60/6.3] The 13M_{sun}_ model yield of Isotopephys.composition.yielddouble15M[3.9e-60/7.1] The 15M_{sun}_ model yield of Isotopephys.composition.yielddouble20M[4.7e-60/9] The 20M_{sun}_ model yield of Isotopephys.composition.yielddouble25M[6.4e-60/10.5] 25M_{sun}_ model yield of Isotopephys.composition.yielddouble30M[0/11.6] The 30M_{sun}_ model yield of Isotopephys.composition.yielddouble40M[0/15.6] The 40M_{sun}_ model yield of Isotopephys.composition.yielddouble60M[0/29] The 60M_{sun}_ model yield of Isotopephys.composition.yielddouble80M[0/42.1] The 80M_{sun}_ model yield of Isotopephys.composition.yielddouble120M[0/68] The 120M_{sun}_ model yield of Isotopephys.composition.yielddoubleJ/ApJS/237/13/table9Isotopic yields in the wind - Recommended setrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintVel[0/300] Velocitykm/sphys.veloc;meta.modelledint[Fe/H][-3/0] Metallicitylog(Sun)phys.abund.ZintIsoIsotope identifiermeta.id;phys.molchar13M[0/4.8] The 13M_{sun}_ model yield of Isotopephys.composition.yielddouble15M[0/5.2] The 15M_{sun}_ model yield of Isotopephys.composition.yielddouble20M[0/8.5] The 20M_{sun}_ model yield of Isotopephys.composition.yielddouble25M[0/10.2] The 25M_{sun}_ model yield of Isotopephys.composition.yielddoubleJ/ApJS/237/13/table3Network reference matrixrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIsoIsotope identifiermeta.id;phys.molcharf_IsoFlag on Iso (1)meta.codecharp.alpThe (p,{alpha}) reference code (2)meta.notecharp.nThe (p,n) reference code (2)meta.notecharp.gamThe (p,{gamma}) reference code (2)meta.notecharalp.pThe ({alpha},p) reference code (2)meta.notecharalp.nThe ({alpha},n) reference code (2)meta.notecharalp.gamThe ({alpha},{gamma}) reference code (2)meta.notecharn.pThe (n,p) reference code (2)meta.notecharn.alpThe (n,{alpha}) reference code (2)meta.notecharn.gamThe (n,{gamma}) reference code (2)meta.notechargam.pThe ({gamma},p) reference code (2)meta.notechargam.alpThe ({gamma},{alpha}) reference code (2)meta.notechargam.nThe ({gamma},n) reference code (2)meta.notecharbetaPThe (beta^+^) reference code (2)meta.notecharbetaMThe (beta^-^) reference code (2)meta.notecharJ/ApJS/237/13/table5Main evolutionary properties of the modelsN/C[6.3e-08/156] Nitrogen to Carbon abundance ratiophys.abund;arith.ratiodoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintVel[0/300] Velocitykm/sphys.veloc;meta.modelledint[Fe/H][-3/0] Metallicitylog(Sun)phys.abund.ZintIMass[13/120] Initial masssolMassphys.massintPhaseEvolutionary phase (1)meta.notecharTime[1e-05/21500000] Lifetimeyrtime.lifetimedoubleMCC[0/95.5] Maximum mass of convective coresolMassphys.massfloatlogT[3.5/5.4] log effective temperaturelog(K)phys.temperature.effectivefloatlogL[4/6.7] log luminositylog(solLum)phys.luminosityfloatTMass[5/120] Total masssolMassphys.massfloatMHe[0/81] Helium core masssolMassphys.massfloatMCO[0/59] CarbonOxygen core masssolMassphys.massfloatvEqua[0/645] Equatorial velocitykm/sphys.veloc;pos.eqdoubleomega[0/0.0007] Surface angular velocitys**-1phys.veloc.angdoubleRatio[0/1] Ratio of omega to critical angular velocityphys.veloc;arith.ratiodoubleJtot[0/6.2] Total angular momentum1e+53g.cm**-2.s**-1phys.angMomentumdoubleH[0/0.8] Surface Hydrogen mass fractionphys.abund.XdoubleHe[0.2/1] Surface Helium mass fractionphys.abund.YdoubleN[2.7e-08/2.3] Surface Nitrogen mass fractionphys.abunddoubleN/O[1.4e-09/165] Nitrogen to Oxygen abundance ratiophys.abund;arith.ratiodoubleJ/ApJS/237/13/table6Wolf-Rayet lifetimes of the modelstO[11400/17800000]? Lifetime during the O-type phaseyrtime.lifetimedoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintVel[0/300] Velocitykm/sphys.veloc;meta.modelledint[Fe/H][-3/0] Metallicitylog(Sun)phys.abund.ZintMass[13/120] Initial masssolMassphys.massinttWR[307/1160000]? Lifetime during the WNR phaseyrtime.lifetimedoublenullabletWNL[307/851000]? Lifetime during the WNL phaseyrtime.lifetimedoublenullableWNL? Central mass fraction at WNL stage start (1)phys.masschartWNE[812/156000]? Lifetime during the WNE phaseyrtime.lifetimedoublenullableWNE? Central mass fraction at WNE stage start (1)phys.masschartWNC[0.003/134000]? Lifetime during the WNC phaseyrtime.lifetimedoublenullableWNC? Central mass fraction at WNC stage start (1)phys.masschartWC[3220/295000]? Lifetime during the WC phaseyrtime.lifetimedoublenullableWC? Central mass fraction at WC stage start (1)phys.mass;arith.ratiochar