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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Yost, S.A. et al. Physical Constraints from Broadband Afterglow Fits: GRB000926 as an Example. In: Costa, E., Frontera, F., Hjorth, J. (eds) Gamma-Ray Bursts in the Afterglow Era. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10853853_56
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DOI: https://doi.org/10.1007/10853853_56
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Publisher Name: Springer, Berlin, Heidelberg
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