Back to Search Start Over

High-energy gamma rays from the intense 1993 January 31 gamma-ray burst

Authors :
Sommer, M
Bertsch, D. L
Dingus, B. L
Fichtel, C. E
Fishman, G. J
Harding, A. K
Hartman, R. C
Hunter, S. D
Hurley, K
Kanbach, G
Source :
Astrophysical Journal, Part 2 - Letters. 422(2)
Publication Year :
1994
Publisher :
United States: NASA Center for Aerospace Information (CASI), 1994.

Abstract

The intense gamma-ray burst of 1993 January 31 was detected by the Energetic Gamma Ray Experiment Telescope (EGRET) on the Compton Observatory. Sixteen gamma rays above 30 MeV were imaged in the telescope when only 0.04 gamma rays were expected by chance. Two of these gamma rays have energies of approximately 1 GeV, and the five bin spectrum of the 16 events is fitted by a power law of photon spectral index -2.0 +/- 0.4. The high-energy emission extends for at least 25 s. The most probable direction for this burst is determined from the directions of the 16 gamma rays observed by Egret and also by requiring the position to lie on annulus derived by the Interplanetary Network.

Subjects

Subjects :
Astrophysics

Details

Language :
English
ISSN :
0004637X
Volume :
422
Issue :
2
Database :
NASA Technical Reports
Journal :
Astrophysical Journal, Part 2 - Letters
Notes :
NAG5-1605, , NAS5-31210, , NAG5-1742, , BMFT-50-QV-9095, , NAG5-1559, , JPL-958056
Publication Type :
Report
Accession number :
edsnas.19950036135
Document Type :
Report
Full Text :
https://doi.org/10.1086/187213