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Spatial distribution of gamma-ray bursts observed by BATSEAn analysis of 153 gamma-ray bursts detected by the Burst and Transient Source Experiment on the Compton Gamma Ray Observatory is reported. The number versus intensity distribution does not follow the -3/2 power law expected for a spatially extended homogeneous distribution of sources, but at the same time the angular distribution is isotropic within statistical limits. Taken together these results are consistent with the spatial distribution of any known population of galactic objects, but may be consistent with the bursts being at cosmological distances.
Document ID
19920037422
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Meegan, C. A.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Fishman, G. J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Wilson, R. B.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Horack, J. M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Brock, M. N.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Paciesas, W. S.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Pendleton, G. N.
(Alabama, University Huntsville, United States)
Kouveliotou, C.
(Universities Space Research Association Huntsville, AL, United States)
Date Acquired
August 15, 2013
Publication Date
January 9, 1992
Publication Information
Publication: Nature
Volume: 355
ISSN: 0028-0836
Subject Category
Space Radiation
Report/Patent Number
ISSN: 0028-0836
Accession Number
92A20046
Distribution Limits
Public
Copyright
Other

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