J/MNRAS/482/384ivo://CDS.VizieR/J/MNRAS/482/384doi:10.26093/cds/vizier.74820384CDSXiao L.Galbany L.Eldridge J.J.Stanway E.R.2024-08-19T20:15:01Z2022-08-01T12:49:09ZCDS support team

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

cds-question@unistra.frmultiple-starssupernovaeh-ii-regionsgalaxiesMassive stars are the main objects that illuminate HII regions and they evolve quickly to end their lives in core-collapse supernovae (CCSNe). Thus, it is important to investigate the association between CCSNe and HII regions. In this paper, we present emission-line diagnostics of the stellar populations around nearby CCSNe, which include their host HII regions, from the Potsdam Multi-Aperture Spectrophotometer (PMAS)/PPak integral-field supernova hosts compilation (PISCO). We then use bpass stellar population models to determine the age, metallicity and gas parameters for HII regions associated with CCSNe, contrasting models that either consider single-star evolution alone or incorporate interacting binaries. We find that binary-star models, which allow for ionizing photon loss, provide a more realistic fit to the observed CCSN hosts, with metallicities that are closer to those derived from the oxygen abundance in O3N2. We also find that Type II and Type Ibc SNe arise from progenitor stars of similar age, mostly from 7 to 45Myr, which corresponds to stars with masses =<20M_{sun}_. However, these two types of SNe have little variations in their host environment metallicity measured by oxygen abundance or in progenitor initial mass. We note that at lower metallicities the SNe are more likely to be Type II.2019MNRAS.482..384Xhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/482/384CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/482/384https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/482/384http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/482/384https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/482/384https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/482/384http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/482/384GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/482/384/tablea1 (Best-fitting parameters for the no-leakage case for each CCSN host HII region, from single-star and binary-star populations)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/482/384/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/482/384/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/482/384/tablea1?GETtext/xml+votable180.050000true0.7771667-1.91161110.0055555555555555566/43 471 552 738 908-909 995 1517 1596 1644 2372 2395 2408 3105 3217 3519 3929 4178 4472 4511 4704 4716 4806 5028 5148 5190 5399 5505 5593 5642 5715 5757 6000 6034 6261 6335 6366 6539 6637 6805 6970 6994 7214 7309 7458 7572 7599 7606 7735 7824 7849 7983 8045 8376 8391 8498 8700 8922 8973 9101 9220 9859 9891 9974 10189 10380-10381 10398 10566 10577 10595 10621 10629 10642 10727 10739 10782 11111 11164 11173 11247 11392 11544 11944 13316 13496 13780 13901 14560 14968 15593 16091 16120 17398 17571 17912 18300 18398 18854 19073 19108 19283 19661 19848 19954 19996 20040 20060 21916 21953 22353 22751 23051 23204 23356 23895 24027 24055 24186 25491 26068 27368 27373 27596 28112 28149 28213 28263 28606 32614 36793https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/482/384?format=asciidefaultJ/MNRAS/482/384/tablea1Best-fitting parameters for the no-leakage case for each CCSN host HII region, from single-star and binary-star populationsSimbadNameSimbad column added by the CDSmeta.idcharnullableTypeSupernova typesrc.classchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainNameSupernova namemeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogAgeSNLAge of the inner ionizing stellar population source from single-star model best fit for the no-leakage caselog(yr)time.agefloate_logAgeSNLError on logAgeSNLlog(yr)stat.errorfloatlognHSNLHydrogen density from single-star model best fit for the no-leakage caselog(cm**-3)phot.flux.densityfloate_lognHSNLError on lognHSNLlog(cm**-3)phot.flux.densityfloatlogUSNLIonization parameter from single-star model best fit for the no-leakage casephys.ionizParamfloate_log(O/H)SNLError on log(O/H)SNLphys.abundfloatlogAgeBNLAge of the inner ionizing stellar population source from binary-star model best fit for the no-leakage caselog(yr)time.agefloate_logAgeBNLError on logAgeBNLlog(yr)stat.errorfloate_logUSNLError on logUSNLstat.errorfloatlog(O/H)SNLOxygen abundance 12+log(O/H) from single-star model best fit for the no-leakage casephys.abundfloatlognHBNLHydrogen density from binary-star model best fit for the no-leakage caselog(cm**-3)phot.flux.densityfloate_lognHBNLError on lognHBNLlog(cm**-3)phot.flux.densityfloatlogUBNLIonization parameter from binary-star model best fit for the no-leakage casephys.ionizParamfloate_logUBNLError on logUBNLstat.errorfloatlog(O/H)BNLOxygen abundance 12+log(O/H) from binary-star model best fit for the no-leakage casephys.abundfloate_log(O/H)BNLError on log(O/H)BNLphys.abundfloatJ/MNRAS/482/384/tablea2Best-fitting parameters for the leakage case for each CCSN host HII region, from single-star and binary-star populationsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSupernova namemeta.id;meta.maincharTypeSupernova typesrc.classcharlogAgeSLAge of the inner ionizing stellar population source from single-star model best fit for the leakage caselog(yr)time.agefloate_logAgeSLError on logAgeSLlog(yr)stat.errorfloatlognHSLHydrogen density from single-star model best fit for the leakage caselog(cm**-3)phot.flux.densityfloate_lognHSLError on lognHSLlog(cm**-3)phot.flux.densityfloatlogUSLIonization parameter from single-star model best fit for the leakage casephys.ionizParamfloate_logUSLError on logUSLstat.errorfloatlog(O/H)SLOxygen abundance 12+log(O/H) from single-star model best fit for the leakage casephys.abundfloate_log(O/H)SLError on log(O/H)SLphys.abundfloatlogAgeBLAge of the inner ionizing stellar population source from binary-star model best fit for the leakage caselog(yr)time.agefloate_logAgeBLError on logAgeBLlog(yr)stat.errorfloatlognHBLHydrogen density from binary-star model best fit for the leakage caselog(cm**-3)phot.flux.densityfloate_lognHBLError on lognHBLlog(cm**-3)phot.flux.densityfloatlogUBLIonization parameter from binary-star model best fit for the leakage casephys.ionizParamfloate_logUBLError on logUBLstat.errorfloatlog(O/H)BLOxygen abundance 12+log(O/H) from binary-star model best fit for the leakage casephys.abundfloate_log(O/H)BLError on log(O/H)BLphys.abundfloat