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The Birth of Neutron Stars

Published online by Cambridge University Press:  04 August 2017

S. E. Woosley
S. E. Woosley*
Affiliation:
Board of Studies in Astronomy and Astrophysics Lick Observatory, University of California at Santa Cruz Santa Cruz CA 95064 Special Studies Group, Lawrence Livermore National Laboratory Livermore CA 94550

Abstract

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Presupernova models of massive stars are discussed and their explosion by either the “core bounce” or neutrino energy transport mechanism briefly reviewed. Special consideration is given to those attributes of the stellar evolution and explosion that might influence the properties of the neutron star remnant: its mass, rotation rate, magnetic field, and “kick” velocity.

Type
III. Neutron Star Formation in Theoretical Supernovae
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 255 - 272
Copyright
Copyright © Reidel 1987 

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