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18 - Supernovae and Their Remnants: Pulsar Wind Nebulae

from Part IV - Environments and the Interstellar Medium

Published online by Cambridge University Press:  21 July 2022

Andrew Lyne ,
Francis Graham-Smith  and
Benjamin Stappers
Andrew Lyne
Affiliation:
University of Manchester
Francis Graham-Smith
Affiliation:
University of Manchester
Benjamin Stappers
Affiliation:
University of Manchester
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Summary

The remnant of a supernova explosion may be observed for some thousands of years in close relation to a pulsar. Radiation from a pulsar may excite radiation from the interstellar medium, causing a pulsar wind nebula, which may be asymmetric due to velocity of the pulsar

Keywords

Stellar evolutionStellar collapseAccretion induced collapseSupernova remnantsLuminosity decayThe Crab NebulaEnergy supplyPulsar and supernova associationsPulsar wind nebulae
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Chapter
Information
Pulsar Astronomy , pp. 299 - 321
Publisher: Cambridge University Press
Print publication year: 2022

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