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On the emission region of gamma ray burstsWithin the last few years the rapid accumulation of gamma ray burst spectral data, especially those of KONUS and solar maximum mission, has made the confrontation between theories of the gamma ray emission mechanisms and observations much more urgent and challenging. At present the most viable mode seems to be some combination of inverse Comptonization and synchrotron emission. Here, an attempt is made to limit the acceptable parameter space of the emission region by taking into account the maximum set of observational constraints. These are then applied to two specific scenarios: surface emission versus magnetospheric emission. Some observable predictions based on these scenarios are considered.
Document ID
19850025593
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Liang, E. P. (Lawrence Livermore National Lab. Livermore, CA, United States)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 1
Subject Category
Space Radiation
Report/Patent Number
OG-1.1-4
Accession Number
85N33906
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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