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The Supernova/GRB Connection

Published online by Cambridge University Press:  19 September 2016

P. Höflich ,
D. Baade ,
A. Khokhlov ,
L. Wang  and
J.C. Wheeler
P. Höflich
Affiliation:
Dept. of Astronomy, University of Texas, Austin, TX 78681, USA; pah@astro.as.utexas.edu&, wheel@hej3.as.utexas.edu
D. Baade
Affiliation:
ESO, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany; pdbaade@eso.org
A. Khokhlov
Affiliation:
Naval Research Lab, Washington DC, USA; ajk@lcp.nrl.navy.mil
L. Wang
Affiliation:
Lawrence Berkeley Lab, CA 94720, USA; lifan@panisse.lbl.gov
J.C. Wheeler
Affiliation:
Dept. of Astronomy, University of Texas, Austin, TX 78681, USA; pah@astro.as.utexas.edu&, wheel@hej3.as.utexas.edu

Summary

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We discuss the possible connection between supernova explosions (SN) and gamma-ray bursters (GRB) from the perspective of our current understanding of SN physics. Core collapse supernovae (SN) are the final stages of stellar evolution in massive stars during which the central region collapses, forms a neutron star (NS) or black hole, and the outer layers are ejected. Recent explosion scenarios assumed that the ejection is due to energy deposition by neutrinos into the envelope but detailed models do not produce powerful explosions. There is new and mounting evidence for an asphericity and, in particular, for axial symmetry in several supernovae which may be hard to reconcile within the spherical picture. The 3-D signatures are a key to understand core collapse supernovae and the GRB/SN connection. In this paper we study the effects and observational consequences of asymmetric explosions.

Type
Part VI Supernova and Gamma-Ray Burst Connections
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 403 - 410
Copyright
Copyright © Springer-Verlag 2005

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