The Fast Evolution of SN 2010bh associated with GRB 100316D
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.
- Publication:
-
Death of Massive Stars: Supernovae and Gamma-Ray Bursts
- Pub Date:
- September 2012
- DOI:
- 10.1017/S1743921312013427
- Bibcode:
- 2012IAUS..279..375O
- Keywords:
-
- supernovae: individual (SN 2010bh);
- gamma-rays: burts