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Recent Observations of GRB-Supernovae

Published online by Cambridge University Press:  05 September 2012

Bethany Elisa Cobb
Bethany Elisa Cobb*
Affiliation:
George Washington UniversityDepartment of Physics725 21st St, NW, Corcoran 105 Washington DC, 20052, USA email: bcobb@gwu.edu
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Abstract

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The GRB-SNe connection has been strengthened since 2008 by the detection of 6 additional GRB-SNe at both local and cosmological redshifts. This review summarizes the recent observations of SNe associated with GRBs 081007, 090618, 091127, 100316D, 101219B and 111211A, as well as the observations of SN 2008D, which was associated with a bright X-ray flash (XRF 080109) and may represent a link between “plain” SN and GRB-SNe. It is now clear that most – if not all – long-duration GRBs are produced by the core collapse of massive stars.

Keywords

gamma rays: burstssupernovae: generalsupernovae: individual (2008D, 2008hw, 2009nz, 2010bh, 2010ma)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S279: Death of Massive Stars: Supernovae and Gamma-Ray Bursts , April 2011 , pp. 83 - 90
Copyright
Copyright © International Astronomical Union 2012

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