On particle acceleration in supernova remnants

Details On particle acceleration in supernova remnants On particle acceleration in supernova remnants

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ssrv...36...57d&link_type=abstract

(International Astronomical Union, Meeting on Galactic Astrophysics and Gamma-Ray Astronomy, Patras, Greece, Aug. 19, 1982) Spac

Astronomy and Astrophysics

Astronomy

48

Energetic Particles, Gamma Ray Astronomy, Particle Acceleration, Supernova Remnants, Radio Emission, Shock Waves, Synchrotron Radiation

Scientific paper

An examination is undertaken of the applicability of firstand second-order Fermi acceleration to electrons in SNRs, respectively differentiating the theories of Krymsky (1977) and Axford et al (1977), on the one hand, and Scott and Chevalier (1975), on the other. The observational evidence does not exclude one or the other theory, but suggests that while both processes may occur in the observed SNRs, diffusive shock acceleration is probably the more important.

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