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Crab-Like Supernova Remnants

Published online by Cambridge University Press:  04 August 2017

R.H. Becker*
Affiliation:
Physics Department, University of California, Davis, CA 95616 Institute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory

Abstract

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Crab-like SNR are markers for recently formed pulsars. The current catalog of 15 objects allows a direct measure of the space distribution of pulsars, the beaming factor of pulsars, and the energetics at young pulsars. The 15 Crab-like SNR are equally divided between those with surroundings shells and those without. No other properties appear to correlate with the presence or lack of a shell. The ratio of 10 to 1 between all remnants and Crab-like remnants has important implications for the formation of pulsars.

Type
I. Rotation-Powered Pulsars
Copyright
Copyright © Reidel 1987 

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