The evolution of nonthermal supernova remnants. II - Can radio supernovae become plerions?

Details The evolution of nonthermal supernova remnants. II - Can radio supernovae become plerions? The evolution of nonthermal supernova remnants. II - Can radio supernovae become plerions?

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...285..134b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 285, Oct. 1, 1984, p. 134-140. Research supported by the Consiglio Nazional

Astronomy and Astrophysics

Astronomy

41

Nonthermal Radiation, Radio Sources (Astronomy), Stellar Evolution, Supernova Remnants, Brightness, Diameters, Light Curve, Pulsars, X Ray Sources

Scientific paper

The authors discuss the evolution of pulsar-driven supernova remnants. It is shown that the early stages closely resemble the phenomenon of radio supernovae and that one can establish a direct evolutionary link between the two classes of objects. Light curves are obtained in the radio and the X-ray ranges under simple assumptions about the injected spectrum. The derived relations between surface brightness and diameter, both at low and at high frequencies, are compared with the observational data.

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