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Spectral evolution of gamma-rays from adiabatically expanding sources in dense cloudsThe excess of antiprotons (P) observed in cosmic ray was attributed to their production in supernova (SN) envelopes expanding in dense clouds. While creating P, gamma rays are also produced and these clouds would shine as gamma-ray sources. The evolution of the gamma-ray spectrum is calculated for clouds of r sub H = 10.000 and 100.000/cu cm.
Document ID
19850025646
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Stephens, S. A. (Tata Inst. of Fundamental Research Bombay, India)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 1
Subject Category
Space Radiation
Report/Patent Number
OG-2.5-2
Report Number: OG-2.5-2
Accession Number
85N33959
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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