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Cosmic gamma-ray bursts

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Abstract

The observational characteristics of gamma-ray bursts are reviewed, concerning their spectra as well as their temporal structure and spatial distribution. From this data, it is suggested that the sources belong to a thick halo population (scale height > 3 kpc), and that the mean recurrence time for one source is greater than 5 yr. The implications of these results are discussed, concerning the future experimental perspectives of detection of gamma-ray bursts, and also the constraints on theoretical models.

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Authors and Affiliations

  1. Centre d'Etude Spatiale des Rayonnements, B. P. 4346-31029, Toulouse, Cedex, France

    G. Vedrenne & G. Chambon

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  1. G. Vedrenne
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  2. G. Chambon
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Proceedings of the XVIII General Assemly of the IAU: Galactic Astrophysics and Gamma-Ray Astronomy, held at Patras, Greece, 19 August 1982.

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Vedrenne, G., Chambon, G. Cosmic gamma-ray bursts. Space Sci Rev 36, 319–335 (1983). https://doi.org/10.1007/BF00247096

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