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Primary gamma-rays with E gamma or = to 10(15) eV: Evidence for ultrahigh energy particle acceleration in galactic sourcesThe recently observed primary ultra high energy gamma-rays (UHEGR) testify to the cosmic ray (CR) acceleration in the Galaxy. The available data may be interpreted as gamma-ray production due to photomeson production in CR sources.
Document ID
19850025661
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Aharonian, F. A. (Academy of Sciences of the Armenian SSR Erivan, Armenia)
Mamidjanian, E. A. (Academy of Sciences of the Armenian SSR Erivan, Armenia)
Nikolsky, S. I. (Academy of Sciences USSR, Moscow, United States)
Tukish, E. I. (Academy of Sciences USSR, Moscow, United States)
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-2.6-13
Report Number: OG-2.6-13
Accession Number
85N33974
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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