Published 2001
| public
Book Section - Chapter
Physical Constraints from Broadband Afterglow Fits: GRB000926 as an Example
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.
Additional Information
© 2001 Springer-Verlag Berlin Heidelberg. First Online: 14 October 2003.Additional details
- Eprint ID
- 99172
- DOI
- 10.1007/10853853_56
- Resolver ID
- CaltechAUTHORS:20191009-073118337
- Created
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2019-10-09Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Series Name
- ESO Astrophysics Symposia