On the morphology of supernova remnants with pulsars

Details On the morphology of supernova remnants with pulsars On the morphology of supernova remnants with pulsars

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990japa...11..125b&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 11, June 1990, p. 125-140.

Astronomy and Astrophysics

Astrophysics

35

Pulsars, Supernova Remnants, Brightness Distribution, Stellar Envelopes, Stellar Evolution, Stellar Magnetic Fields

Scientific paper

One of the intriguing aspects of supernova remnants is their morphology. While the majority of them look like hollow shells, a few, called plerions, are centrally filled like the Crab nebula, and some have a shell-plerion combination morphology. The centrally-filled component in these remnants is believed to be powered by a central pulsar. In this paper results of model calculations of the evolution of surface brightness and morphology of supernova remnants containing pulsars are presented. The paper discusses how the morphology of a supernova remnant will depend on the velocity of expansion, the density of the ambient medium into which it is expanding, and the initial period and magnetic field strength of the central pulsar.

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