Cosmic ray acceleration in a medium with allowance for losses and diffuse gamma-ray sources

Details Cosmic ray acceleration in a medium with allowance for losses and diffuse gamma-ray sources Cosmic ray acceleration in a medium with allowance for losses and diffuse gamma-ray sources

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981izssr..45.1122v&link_type=abstract

(Evropeiskii Simpozium po Kosmicheskim Lucham, 7th, Leningrad, USSR, Sept. 15-19, 1980.) Akademiia Nauk SSSR, Izvestiia, Seriia

Astronomy and Astrophysics

Astronomy

Cosmic Rays, Cosmology, Gamma Ray Astronomy, Milky Way Galaxy, Particle Acceleration, Shock Wave Interaction, Supernova Remnants, Energetic Particles, Energy Dissipation, Energy Transfer, Interstellar Gas, Molecular Clouds, Pitch (Inclination), Stellar Envelopes, Stellar Winds, Velocity Distribution

Scientific paper

The mechanisms of cosmic ray acceleration by shock waves are examined in light of the recent observational data on gamma-ray sources. The discussion focuses on general effects of particle energy loss on cosmic ray acceleration, characteristics of discrete hard gamma-ray sources, cosmic ray acceleration by stellar winds in clouds, and gamma-ray sources produced by supernova explosions within the clouds.

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