On some problems of gamma-astronomy

Details On some problems of gamma-astronomy On some problems of gamma-astronomy

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..305b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 305-308 (SEE N85-33902 22-93)

Astronomy and Astrophysics

Astronomy

Energy Spectra, Gamma Rays, Particle Emission, Particle Energy, Positron Annihilation, Pulsars, Supernova Remnants, Electrons, High Energy Interactions, Kinetic Energy, Magellanic Clouds, Neutrinos, Pions, Positrons, Protons

Scientific paper

Gamma 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.

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