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A search for gamma rays of 1.5-20.0 MeV from Centaurus AA search for a gamma-ray continuum and lines from Centaurus A is reported. No measurable gamma rays are found in the 1.5-20.0 MeV and 3 sigma upper limits are reported for various energies which are about a factor of two lower than the results reported by von Ballmoos et al. (1987). These upper limits, along with those of SAS 2 and COS B, suggest that the energy distribution turns over in the energy range of 500 keV to a few MeV. A high source temperature of 5 MeV or synchrotron self-Compton models for producing an excess of gamma rays of a few MeV do not appear necessary.
Document ID
19890048861
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
O'Neill, Terrence
(California Univ. Riverside, CA, United States)
Tumer, O. Tumay
(California Univ. Riverside, CA, United States)
Zych, Allen
(California Univ. Riverside, CA, United States)
White, R. Stephen
(California, University Riverside, United States)
Date Acquired
August 14, 2013
Publication Date
April 1, 1989
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 339
ISSN: 0004-637X
Subject Category
Space Radiation
Accession Number
89A36232
Funding Number(s)
CONTRACT_GRANT: NGR-05-008-022
Distribution Limits
Public
Copyright
Other

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