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Physical Constraints from Broadband Afterglow Fits: GRB000926 as an Example

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Gamma-Ray Bursts in the Afterglow Era

Part of the book series: ESO ASTROPHYSICS SYMPOSIA ((ESO))

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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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Authors and Affiliations

  1. Caltech, Pasadena CA 91125, USA

    Sarah A. Yost, Re’em Sari, Fiona A. Harrison, Edo Berger, Alan Diercks, Titus Galama & Dan Reichart

  2. National Radio Astronomy Observatory, Socorro NM 87801, USA

    Dale Frail

  3. Research School of Astronomy & Astrophysics, Australian National University, ACT 2601, Australia

    Paul A. Price

Authors
  1. Sarah A. Yost
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  2. Re’em Sari
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  3. Fiona A. Harrison
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  4. Edo Berger
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  5. Alan Diercks
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  6. Titus Galama
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  7. Dan Reichart
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  8. Dale Frail
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  9. Paul A. Price
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Corresponding author

Correspondence to Sarah A. Yost .

Editor information

Enrico Costa Filippo Frontera Jens Hjorth

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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

  • Published:

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-42771-1

  • Online ISBN: 978-3-540-45505-9

  • eBook Packages: Springer Book Archive

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