Radio-emitting supernovae as young plerions

Details Radio-emitting supernovae as young plerions Radio-emitting supernovae as young plerions

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pazh....7..479s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 7, Aug. 1981, p. 479-481.) Soviet Astronomy Letters, vol. 7, July-Aug. 1981, p. 263, 26

Astronomy and Astrophysics

Astronomy

8

Radio Emission, Radio Sources (Astronomy), Stellar Envelopes, Stellar Evolution, Stellar Radiation, Supernovae, Radio Bursts, Relativistic Particles, Stellar Magnetic Fields, Synchrotron Radiation

Scientific paper

It is suggested that young plerions formed immediately after supernova
outbursts generate the radio emission observed, and that the power of
these radio emissions will decay approximately as the inverse of R. It
is further suggested that radio waves will be emitted only by type II
supernovae.

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