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Analysis of the BATSE GRB Light Curves

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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.

Different progenitors and physicalpro cesses could be at the origin of GRBs. New information about the properties of the gamma-ray emission can help to select among the different proposed models and possibly to identify different classes with different origins. We have tried to study the gamma light-curve behaviour in relation to other physicalparameters of the event as duration, peak counting rate, energy spectra hardness, et etc. There are hints that some of the mentioned correlations are present.

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Authors and Affiliations

  1. Istituto di Astrofisica Spaziale, CNR, Via del Fosso del Cavaliere, 00131, Roma, Italy

    B. M. Belli

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  1. B. M. Belli
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Enrico Costa Filippo Frontera Jens Hjorth

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Belli, B.M. Analysis of the BATSE GRB Light Curves. 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_12

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  • DOI: https://doi.org/10.1007/10853853_12

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  • 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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