Merger Models of Gamma-Ray Bursts: A Comparison

dc.contributor.author	Sivaram, C
dc.date.accessioned	2009-01-02T11:17:18Z
dc.date.available	2009-01-02T11:17:18Z
dc.date.issued	1995
dc.identifier.citation	N. Iucci and E. Lamanna. ed., 24th International Cosmic Ray Conference, Vol. 2, held August 28 - September 8, 1995 in Rome, Italy.	en
dc.identifier.uri	http://hdl.handle.net/2248/4231
dc.description.abstract	Two possible merger modes of gamma ray bursts are considered. The merger of two white dwarfs leading to a neutrino bursts accompanying the gamma ray burst. However the merger of two neutron stars should give rise to only a gamma ray burst with a much smaller neutrino flux. Observable signatures to discriminate between these pictures is clarified.	en
dc.language.iso	en	en
dc.publisher	International Union of Pure and Applied Physics	en
dc.relation.ispartofseries	International Union of Pure and Applied Physics;
dc.relation.uri	http://adsabs.harvard.edu/abs/1995ICRC....2..164S	en
dc.title	Merger Models of Gamma-Ray Bursts: A Comparison	en
dc.type	Article	en