Theory of high-energy gamma-ray emission of supernova remnants

Details Theory of high-energy gamma-ray emission of supernova remnants Theory of high-energy gamma-ray emission of supernova remnants

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..558...88b&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: International Symposium. AIP Conference Proceedings, Volume 558, pp. 88-99 (2001).

Astronomy and Astrophysics

Astronomy

Radiation Mechanisms, Polarization, Cosmic Rays, Supernova Remnants, Supernova Remnants

Scientific paper

A brief review of the modern theory of cosmic ray and associated high-energy γ-ray production in supernova remnants is presented. Examples typical for supernovae type Ia, Ib and II are analyzed. The correspondence between observed properties of the emission produced by accelerated cosmic rays in SN 1006 and SN 1987A, and theoretical predictions is discussed. .

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