Magnetar-driven explosions as power source of Gamma-ray Bursts and Supernovae
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Archivos
Fecha
2015
Autores
Profesor/a Guía
Facultad/escuela
Idioma
en
Título de la revista
ISSN de la revista
Título del volumen
Editor
Cambridge University Press
Nombre de Curso
Licencia CC
Atribución-NoComercial-CompartirIgual 3.0 Chile (CC BY-NC-SA 3.0 CL)
Licencia CC
https://creativecommons.org/licenses/by-nc-sa/3.0/cl/
Resumen
We 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.
Notas
Indexación: Scopus
Palabras clave
gamma rays, bursts, supernovae, individual (SN 2011kl)
Citación
Proceedings of the International Astronomical Union Volume 11, Issue A29B, Pages 241 - 2422015
DOI
10.1017/S1743921316005135