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

E. Felipe Olivares, Jochen Greiner

Resultado de la investigación: Article

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.

Idioma originalEnglish
Páginas (desde-hasta)241-242
Número de páginas2
PublicaciónProceedings of the International Astronomical Union
Volumen11
N.ºA29B
DOI
EstadoPublished - 1 ene 2015
Publicado de forma externa

Huella dactilar

magnetars
gamma ray bursts
photometry
supernovae
explosions
explosion
spectroscopy

ASJC Scopus subject areas

  • Astronomy and Astrophysics

Citar esto

Olivares, E. Felipe ; Greiner, Jochen. / Magnetar-driven explosions as power source of Gamma-ray Bursts and Supernovae. En: Proceedings of the International Astronomical Union. 2015 ; Vol. 11, N.º A29B. pp. 241-242.
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Magnetar-driven explosions as power source of Gamma-ray Bursts and Supernovae. / Olivares, E. Felipe; Greiner, Jochen.

En: Proceedings of the International Astronomical Union, Vol. 11, N.º A29B, 01.01.2015, p. 241-242.

Resultado de la investigación: Article

TY - JOUR

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AU - Greiner, Jochen

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N2 - 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.

AB - 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.

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