Chile | Artículo

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

dc.creatorOlivares, E.Felipe
dc.creatorGreiner, Jochen
dc.date.accessioned2023-08-18T15:40:44Z
dc.date.accessioned2024-05-02T15:01:35Z
dc.date.available2023-08-18T15:40:44Z
dc.date.available2024-05-02T15:01:35Z
dc.date.created2023-08-18T15:40:44Z
dc.date.issued2015
dc.identifierProceedings of the International Astronomical Union Volume 11, Issue A29B, Pages 241 - 2422015
dc.identifier1743-9213
dc.identifierhttps://repositorio.unab.cl/xmlui/handle/ria/52615
dc.identifier10.1017/S1743921316005135
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/9261259
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.
dc.languageen
dc.publisherCambridge University Press
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/3.0/cl/
dc.rightsAtribución-NoComercial-CompartirIgual 3.0 Chile (CC BY-NC-SA 3.0 CL)
dc.subjectgamma rays
dc.subjectbursts
dc.subjectsupernovae
dc.subjectindividual (SN 2011kl)
dc.titleMagnetar-driven explosions as power source of Gamma-ray Bursts and Supernovae
dc.typeArtículo


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