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Identification of two classes of gamma-ray bursts

Kouveliotou, Chryssa, Meegan, Charles A., Fishman, Gerald J., Bhat, Narayana P., Briggs, Michael S., Koshut, Thomas M., Paciesas, William S., Pendleton, Geoffrey N.·1993·The Astrophysical Journal

Abstract

We have studied the duration distribution of the gamma-ray bursts of the first BATSE catalog. We find a bimodality in the distribution, which separates GRBs into two classes: short events (less than 2 s) and longer ones (more than 2 s). Both sets are distributed isotropically and inhomogeneously in the sky. We find that their durations are anticorrelated with their spectral hardness ratios: short GRBs are predominantly harder, and longer ones tend to be softer. Our results provide a first GRB classification scheme based on a combination of the GRB temporal and spectral properties.

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Authors
Kouveliotou, C., Meegan, C. A., Fishman, G. J., Bhat, N. P., Briggs, M. S., Koshut, T. M., Paciesas, W. S., & Pendleton, G. N.
Venue
The Astrophysical Journal
Published
1993-08
Volume
413
Pages
L101
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1975498920
Cited by
2,028
References
0
FWCI
26.37
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Identification of two classes of gamma-ray bursts. https://app.cochat.ai/papers/10.1086/186969
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Kouveliotou, C., Meegan, C. A., Fishman, G. J., Bhat, N. P., Briggs, M. S., Koshut, T. M., Paciesas, W. S., & Pendleton, G. N. (1993). Identification of two classes of gamma-ray bursts. The Astrophysical Journal. https://doi.org/10.1086/186969

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