Synchrotron self-absorption of the radio emission of supernova 1983.51

Details Synchrotron self-absorption of the radio emission of supernova 1983.51 Synchrotron self-absorption of the radio emission of supernova 1983.51

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..261s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Apr. 1985, p. 261-264) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, Mar.-Apr

Astronomy and Astrophysics

Astronomy

3

Radio Emission, Radio Sources (Astronomy), Self Absorption, Stellar Radiation, Supernovae, Synchrotron Radiation, Plasma Density, Pulsars

Scientific paper

The radio light-curve of the type I supernova 1983n in M83 is attributable to synchrotron self-absorption, thereby setting a lower limit on the angular size of the radio emission zone. If the customary distance estimates (r is equal to approximately 6 Mpc) are correct, the radio source should have a radius at least three times that of the supernova photosphere; the radio-emitting envelope would be expanding faster than 60,000 km/sec. The origin of supernova radio emission is discussed.

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