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The Fast Evolution of SN 2010bh associated with GRB 100316D

Published online by Cambridge University Press:  05 September 2012

E. Felipe Olivares ,
Jochen Greiner ,
Patricia Schady ,
Arne Rau ,
Sylvio Klose  and
Thomas Krühler
E. Felipe Olivares
Affiliation:
Max-Planck-Institute für extraterrestrische Physik, Giessenbachstraße 1, 85748, Garching, Germany, email: foe@mpe.mpg.de
Jochen Greiner
Affiliation:
Max-Planck-Institute für extraterrestrische Physik, Giessenbachstraße 1, 85748, Garching, Germany, email: foe@mpe.mpg.de
Patricia Schady
Affiliation:
Max-Planck-Institute für extraterrestrische Physik, Giessenbachstraße 1, 85748, Garching, Germany, email: foe@mpe.mpg.de
Arne Rau
Affiliation:
Max-Planck-Institute für extraterrestrische Physik, Giessenbachstraße 1, 85748, Garching, Germany, email: foe@mpe.mpg.de
Sylvio Klose
Affiliation:
Thüringer Landessternwarte Tautenburg, Sternwarte 5, 07778, Tautenburg, Germany
Thomas Krühler
Affiliation:
Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100, Copenhagen, Denmark
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Abstract

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We report on the type-Ic SN 2010bh associated with XRF 100316D at z = 0.059, which is among the latest spectroscopically confirmed GRB-SNe (Bufano et al. 2012). This supernova proves to be the most rapidly evolving GRB-SN to date.

Keywords

supernovae: individual (SN 2010bh)gamma-rays: burts
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S279: Death of Massive Stars: Supernovae and Gamma-Ray Bursts , April 2011 , pp. 375 - 376
Copyright
Copyright © International Astronomical Union 2012

References

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