The soft gamma-ray burst GB790107

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Extraterrestrial Radiation, Gamma Ray Bursts, Energy Spectra, Spectral Energy Distribution, Temporal Distribution, Venera 11 Satellite, Venera 12 Satellite

Scientific paper

It is pointed out that nearly all of the known gamma-ray bursts (GRBs) have intensity spectra which can be described in terms of several-hundred-keV exponential functions, taking into account observations over the energy range from approximately 30 keV to 1 MeV. The results are provided of detections of GB790107, which according to Mazets et al. (1982) has a soft spectrum. The instrumentation employed in the investigation is better suited for the study of such bursts than most instruments. It is found that above 20 keV the spectrum is indeed much softer than any other cosmic event observed through the apertures of these experiments. In the 5-15-keV range the spectrum is very flat. On the basis of statistical arguments, it appears that soft-spectrum events might belong to a disk population.

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