Frequency of fast, narrow gamma-ray bursts

Details Frequency of fast, narrow gamma-ray bursts Frequency of fast, narrow gamma-ray bursts

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.308..434n&link_type=abstract

Nature (ISSN 0028-0836), vol. 308, March 29, 1984, p. 434, 435.

Astronomy and Astrophysics

Astronomy

64

Gamma Ray Bursts, Spaceborne Astronomy, Temporal Distribution, Astronomical Spectroscopy, International Sun Earth Explorer 3, Venera Satellites

Scientific paper

Early studies of the time histories of the γ-ray burst events reported by the Vela satellites led to the suggestion that very brief, ≡0.1 s, bursts formed a class distinct from the longer, highly structured bursts. Results of the KONUS experiments on Veneras 11, 12, 13 and 14 argue for the existence of a separate class of short-duration γ-ray bursts, revealing that many of the short bursts exhibit much softer spectra (≡30 keV) than the more familiar complex bursts. Here the authors point out that the results of the Goddard ISEE-3 γ-ray burst spectrometer actually enhance the appearance of two burst populations suggested in the Venera data.

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