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Pulsar Wind Nebulae and Their Supernovae

Published online by Cambridge University Press:  19 July 2016

Roger A. Chevalier
Roger A. Chevalier*
Affiliation:
Department of Astronomy, University of Virginia, P.O. Box 3818, Charlottesville, VA 22903, USA

Abstract

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Young supernova remnants that contain pulsar wind nebulae provide diagnostics for both the inner part of the supernova and the interaction with the surrounding medium, providing an opportunity to relate these objects to supernova types. Among observed young nebulae, there is evidence for a range of supernova types, including Type IIP (Crab Nebula and SN 1054) and Type IIb/IIn/IIL (G292.0+1.8).

Type
Part 4: Pulsar Wind Nebulae and Their Environments
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 159 - 162
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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