Magnetar-driven explosions as power source of Gamma-ray Bursts and Supernovae

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dc.contributor.authorOlivares, E.Felipe
dc.contributor.authorGreiner, Jochen
dc.date.accessioned2023-08-18T15:40:44Z
dc.date.available2023-08-18T15:40:44Z
dc.date.issued2015
dc.descriptionIndexación: Scopuses
dc.description.abstractWe present photometry and spectroscopy of SN 2011kl associated to GRB 111209A. Peculiarities arise from both the ultra-long GRB and the very luminous SN, brighter than any other GRB-associated SN observed to date. We present unequivocal evidence in favor of a scenario where a newly-formed magnetar powers both the GRB and the SN. © International Astronomical Union 2016.es
dc.description.urihttps://www-cambridge-org.recursosbiblioteca.unab.cl/core/journals/proceedings-of-the-international-astronomical-union/article/magnetardriven-explosions-as-power-source-of-gammaray-bursts-and-supernovae/02D1FB4F81510FFB4336DD80503FA22D
dc.identifier.citationProceedings of the International Astronomical Union Volume 11, Issue A29B, Pages 241 - 2422015es
dc.identifier.doi10.1017/S1743921316005135
dc.identifier.issn1743-9213
dc.identifier.urihttps://repositorio.unab.cl/xmlui/handle/ria/52615
dc.language.isoenes
dc.publisherCambridge University Presses
dc.rights.licenseAtribución-NoComercial-CompartirIgual 3.0 Chile (CC BY-NC-SA 3.0 CL)
dc.rights.urihttps://creativecommons.org/licenses/by-nc-sa/3.0/cl/
dc.subjectgamma rayses
dc.subjectburstses
dc.subjectsupernovaees
dc.subjectindividual (SN 2011kl)es
dc.titleMagnetar-driven explosions as power source of Gamma-ray Bursts and Supernovaees
dc.typeArtículoes
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