Hard X-ray emission from young supernova remnants

Details Hard X-ray emission from young supernova remnants Hard X-ray emission from young supernova remnants

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66.1030a&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, Sept.-Oct. 1989, p. 1030-1038. In Russian.

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Cassiopeia A, Emission Spectra, Supernova Remnants, X Ray Spectra, Bremsstrahlung, Computational Astrophysics, Electron Acceleration, Electron Distribution, Thermal Energy

Scientific paper

Hard X-ray emission (greater than 10 keV) from the supernova remnant Cassiopeia A can be explained by bremsstrahlung of electrons accelerated by the regular mechanism at the shock wave front. This may be the first confirmation of the fact that the process of acceleration in supernova remnants starts from thermal energies. The need for X-ray observations of young remnants in the hard X-ray energy range (greater than 20 keV) is emphasized. The coefficient of electron diffusion in the vicinity of supernova remnants is estimated.

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