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3 keV to 2 MeV observations of four gamma-ray burstsSimultaneous X and gamma ray spectra were obtained for four gamma ray burst events using satellite instrumentation. The P78-1 satellite proportional counters recorded X-ray data in the 3-10 keV range, while Pioneer Venus Orbiter and ISEE 3 sensors had a 3 keV lower limit for events. The positively correlated data covered the events GB 790307, 790325, 790504, and 790731. The time histories of the X and gamma ray energies did not correlate well. The post-gamma ray phase of GB 790307 displayed features of simple cooling, and in conjunction with soft X-ray data suggested an origin in an optically thin fireball. However, the data were equally well-fitted by a model of an emitting hot spot on a neutron star. The data negated any concept that gamma ray bursts evolve similarly to classical X-ray bursts.
Document ID
19850039081
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Laros, J. G.
(Los Alamos Scientific Lab. NM, United States)
Evans, W. D.
(Los Alamos Scientific Lab. NM, United States)
Fenimore, E. E.
(Los Alamos Scientific Lab. NM, United States)
Klebesadel, R. W.
(Los Alamos National Laboratory Los Alamos, NM, United States)
Shulman, S.
(U.S. Navy, Naval Research Laboratory, Washington, DC; Sachs/Freeman Associates, Inc. Bowie, MD, United States)
Fritz, G.
(U.S. Navy, Naval Research Laboratory, Washington DC, United States)
Date Acquired
August 12, 2013
Publication Date
November 15, 1984
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 286
ISSN: 0004-637X
Subject Category
Space Radiation
Accession Number
85A21232
Funding Number(s)
CONTRACT_GRANT: NASA ORDER A-98331-A
CONTRACT_GRANT: NAS5-25980
Distribution Limits
Public
Copyright
Other

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