Synchrotron radiation of type I supernova remnants

Details Synchrotron radiation of type I supernova remnants Synchrotron radiation of type I supernova remnants

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993roizf..57...70a&link_type=abstract

Rossijskaya Akademiya Nauk, Izvestiya, Seriya Fizicheskaya (ISSN 0367-6765), vol. 57, no. 7, p. 70-72.

Physics

Electron Acceleration, Interstellar Magnetic Fields, Supernova Remnants, Synchrotron Radiation, Distribution Functions, Shock Wave Propagation

Scientific paper

A model of synchrotron radiation from electrons accelerated by an
external shock wave in the magnetic field of a supernova remnant is
examined that may describe the synchrotron radiation of supernova
remnants. Calculation results agree satisfactorily with data for SN 1006
and SN Tycho in the frequency range 10 exp 9 to 10 exp 18 Hz.

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