The interpretation of the radio emission from supernova 1987A in the Large Magellanic Cloud

Details The interpretation of the radio emission from supernova 1987A in the Large Magellanic Cloud The interpretation of the radio emission from supernova 1987A in the Large Magellanic Cloud

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..109f&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Feb. 1989, p. 109-117. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Magellanic Clouds, Radio Emission, Supernova 1987A, Electronic Spectra, Gas Density, Magnetohydrodynamic Turbulence, Shock Waves, Stellar Envelopes, Stellar Winds, Synchrotron Radiation

Scientific paper

A model is proposed which explains the basic features of the radio emission from SN 1987A which was observed over several days after the maximum of optical light. The observations were carried out at four frequencies in the centimeter range. The variation of the gas plane in the region of the interaction of the supernova envelope with stellar wind is studied.

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