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dc.contributor.authorValenti, S.
dc.contributor.authorFraser, M.;
dc.contributor.authorBenetti, S.
dc.contributor.authorPignata, G.
dc.contributor.authorSollerman, J.
dc.contributor.authorInserra, C.
dc.contributor.authorCappellaro, E.
dc.contributor.authorPastorello, A.
dc.contributor.authorSmartt, S. J.
dc.contributor.authorErgon, M.
dc.contributor.authorBotticella, M. T.
dc.contributor.authorBrimacombe, J.
dc.contributor.authorBufano, F.
dc.contributor.authorCrockett, M.
dc.contributor.authorEder, I.
dc.contributor.authorFugazza, D.
dc.contributor.authorHaislip, J. B.
dc.contributor.authorHamuy, M.
dc.contributor.authorIvarsen, K. M.
dc.contributor.authorKankare, E.
dc.contributor.authorKotak, R.
dc.contributor.authorLaCluyze, A. P.
dc.contributor.authorMagill, L.
dc.contributor.authorMattila, S.
dc.contributor.authorMaza, J.
dc.contributor.authorMazzali, P. A.
dc.contributor.authorReichart, D. E.
dc.contributor.authorTaubenberger, S.
dc.contributor.authorTuratto, M.
dc.contributor.authorZampieri, L.
dc.contributor.authorHarutyunyan, K.M.
dc.date.accessioned2013-10-22T18:50:33Z
dc.date.accessioned2016-05-24T20:13:48Z
dc.date.available2013-10-22T18:50:33Z
dc.date.available2016-05-24T20:13:48Z
dc.date.issued2011
dc.identifier.urihttp://repositorio.unab.cl/xmlui/handle/ria/1916
dc.description.abstractWe present an extensive set of photometric and spectroscopic data for SN 2009jf, a nearby Type Ib supernova, spanning from 20 days before B-band maximum to one year after maximum. We show that SN 2009jf is a slowly evolving and energetic stripped-envelope SN and is likely from a massive progenitor (25-30 solar masses). The large progenitor’s mass allows us to explain the complete hydrogen plus helium strip- ping without invoking the presence of a binary companion. The supernova occurred close to a young cluster, in a crowded environment with ongoing star-formation. The specroscopic similarity with the He-poor Type Ic SN 2007gr suggests a common pro- genitor for some supernovae Ib and Ic. The nebular spectra of SN 2009jf are consistent with an asymmetric explosion, with an off-center dense core. We also find evidence that He-rich Ib supernovae have a rise time longer than other stripped-envelope su- pernovae, however confirmation of this result and further observations are needed.en
dc.language.isoen
dc.subjectSupernovae: general
dc.subjectSupernovae: SN 2009jf
dc.subjectGalaxies: NGC 7479
dc.titleSN 2009jf: a slow-evolving stripped-envelope core-collapse supernova
dc.typeArtículo de revista


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