A young stellar environment for the superluminous supernova PTF12dam

dc.contributor.authorThoene, C. C.
dc.contributor.authorPostigo, A. de Ugarte
dc.contributor.authorGarcia Benito, R.
dc.contributor.authorLeloudas, G.
dc.contributor.authorSchulze, S.
dc.contributor.authorAmorin, R.
dc.date.accessioned2024-01-10T13:46:18Z
dc.date.available2024-01-10T13:46:18Z
dc.date.issued2015
dc.description.abstractThe progenitors of superluminous supernovae (SLSNe) are still a mystery. Hydrogen-poor SLSN hosts are young, highly star-forming dwarf galaxies and the majority belongs to the class of 'extreme emission line galaxies'. Here we present a resolved long-slit study of the host of the hydrogen-poor SLSN PTF12dam probing the kiloparsec environment of the SN site to determine the age of the progenitor. The SN occurred in a star-forming region in the head of a 'tadpole' galaxy with largely uniform properties. The galaxy experienced a recent starburst superimposed on an underlying old stellar population (SP). We determine a very young SP at the SN site of similar to 3 Myr and a metallicity of 12+log(O/H)=8.0 but do not observe any Wolf-Rayet features. The progenitor of PTF12dam was likely a massive star of >60 M-circle dot and one of the first stars exploding as an SN in the most recent starburst episode.
dc.description.funderSpanish MINECO
dc.description.funderDNRF
dc.description.funderCONICYT-Chile
dc.description.funderFP7 SPACE project ASTRODEEP of the EC
dc.fechaingreso.objetodigital2024-04-29
dc.format.extent5 páginas
dc.fuente.origenWOS
dc.identifier.doi10.1093/mnrasl/slv051
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnrasl/slv051
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/79145
dc.identifier.wosidWOS:000361302000014
dc.information.autorucFísica;Schulze S;S/I;237742
dc.issue.numero1
dc.language.isoen
dc.nota.accesocontenido parcial
dc.publisherOXFORD UNIV PRESS
dc.revistaMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
dc.rightsacceso restringido
dc.subjectsupernovae: individual: PTF12dam
dc.subjectgalaxies: abundances
dc.subjectgalaxies starburst
dc.subjectSTAR-FORMING GALAXIES
dc.subjectMASS-METALLICITY RELATION
dc.subjectBURST HOST GALAXIES
dc.subjectGREEN PEA GALAXIES
dc.subjectDIGITAL SKY SURVEY
dc.subjectLUMINOUS SUPERNOVAE
dc.subjectPOPULATION SYNTHESIS
dc.subjectCHEMICAL ABUNDANCES
dc.subjectFORMATION HISTORY
dc.subjectSYNTHESIS MODELS
dc.subject.ods07 Affordable and Clean Energy
dc.subject.odspa07 Energía asequible y no contaminante
dc.titleA young stellar environment for the superluminous supernova PTF12dam
dc.typeartículo
dc.volumen451
sipa.codpersvinculados237742
sipa.indexWOS
sipa.indexScopus
sipa.trazabilidadCarga SIPA;09-01-2024
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