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Published 2001 | Version public
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Physical Constraints from Broadband Afterglow Fits: GRB000926 as an Example

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Abstract

We develop a model to fit the broadband afterglows of GRBs from the intrinsic parameters of the fireball's synchrotron emission, and apply it to a few wellstudied events, with the goal of constraining the intrinsic variability of GRB parameters. We give an example here of fitting to the recent bright event GRB000926.

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© 2001 Springer-Verlag Berlin Heidelberg. First Online: 14 October 2003.

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Eprint ID
99172
DOI
10.1007/10853853_56
Resolver ID
CaltechAUTHORS:20191009-073118337

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10.1007/10853853_56 (DOI)

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Created
2019-10-09
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Updated
2021-11-16
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Space Radiation Laboratory
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ESO Astrophysics Symposia