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The Fast Evolution of SN 2010bh associated with GRB 100316D
Published online by Cambridge University Press: 05 September 2012
Abstract
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.
- 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