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Neutron Stars in Supernova Remnants

Published online by Cambridge University Press:  25 May 2016

F. Pacini
F. Pacini*
Affiliation:
Arcetri Astrophysical Obs. and Dept. of Astronomy & Space Sciences, University of Florence, Largo E. Fermi 5, I-50125, Firenze, Italy

Abstract

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In the following, we shall briefly summarize some facts and ideas concerning the presence of neutron stars in supernova remnants. While sources similar to the Crab Nebula require the presence of a central energetic object, shell-type remnants such as Cas A are compatible with the presence of neutron stars releasing a weak relativistic wind.

Type
Part I: Talks
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 91 - 93
Copyright
Copyright © Astronomical Society of the Pacific 2000 

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