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Philos Trans A Math Phys Eng Sci. 2007 May 15;365(1854):1277-80.

Gamma-ray burst models.

Author information

1
Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH, UK. ark@astro.le.ac.uk

Abstract

I consider various possibilities for making gamma-ray bursts, particularly from close binaries. In addition to the much-studied neutron star+neutron star and black hole+neutron star cases usually considered good candidates for short-duration bursts, there are also other possibilities. In particular, neutron star+massive white dwarf has several desirable features. These systems are likely to produce long-duration gamma-ray bursts (GRBs), in some cases definitely without an accompanying supernova, as observed recently. This class of burst would have a strong correlation with star formation and occur close to the host galaxy. However, rare members of the class need not be near star-forming regions and could have any type of host galaxy. Thus, a long-duration burst far from any star-forming region would also be a signature of this class. Estimates based on the existence of a known progenitor suggest that this type of GRB may be quite common, in agreement with the fact that the absence of a supernova can only be established in nearby bursts.

PMID:
17293332
DOI:
10.1098/rsta.2006.1978

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