The effect of hot plasma in the envelopes of young supernova remnants on radio emission

Details The effect of hot plasma in the envelopes of young supernova remnants on radio emission The effect of hot plasma in the envelopes of young supernova remnants on radio emission

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..118s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Feb. 1987, p. 118-123. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

High Temperature Plasmas, Radio Emission, Stellar Envelopes, Supernova Remnants, Cassiopeia A, Plasma Radiation, Relativistic Particles, Synchrotron Radiation, X Ray Astronomy

Scientific paper

It is shown that plasma and Compton mechanisms of relativistic electron radiation may act together with synchrotron one in the envelopes of young supernova remnants giving an intense X-ray radiation. For Cassiopeia A the intensity of plasma radiation for the contemporary epoch increases. It has been obtained that the energy density of plasma turbulence in the source amounts 2×10-2 of the thermal one.

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