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On some problems of gamma-astronomyGamma ray emissions from young supernova remnants are discussed and calculated. The positron annihilation line is also calculated. Decay of charged pions in remnants cause generation of high energy neutrinos. This emission of neutrinos is reviewed. The CR origin and gamma emission from Magellanic clouds help to establish the intensity gradient in the galaxy. This gamma astronomical data is briefly discussed.
Document ID
19850025675
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Berezinsky, V. S.
(Academy of Sciences (USSR) Moscow, Ussr)
Ginzburg, V. L.
(Academy of Sciences (USSR) Moscow, Ussr)
Ptuskin, V. S.
(Academy of Sciences (USSR) Moscow, Ussr)
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-2.7-15
Report Number: OG-2.7-15
Accession Number
85N33988
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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