The influence of the reverse shock wave on the evolution of young supernova remnants

Details The influence of the reverse shock wave on the evolution of young supernova remnants The influence of the reverse shock wave on the evolution of young supernova remnants

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980acasn..21..184c&link_type=abstract

Acta Astronomica Sinica, vol. 21, June 1980, p. 184-188. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

1

Early Stars, Shock Wave Propagation, Stellar Evolution, Supernova Remnants, Gas Temperature, Radio Emission, Stellar Luminosity, X Ray Astronomy

Scientific paper

McKee's formula (1974) for the propagation of the reverse shock wave in supernova systems is improved, and the influence of the reverse shock wave on the evolution of young supernova remnants is discussed. It is shown that the temperature of the shocked gas behind the reverse wave increases progressively, while the thermal X-ray luminosity of the gas decreases. The effect of the reverse wave on radio emission from young remnants is considered.

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