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Neutron Stars in Twelve Supernova Remnants

Published online by Cambridge University Press:  04 August 2017

Frederick D. Seward
Frederick D. Seward*
Affiliation:
Harvard Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge MA 02138

Abstract

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X-ray observations of selected SNR are summarized. Five contain internal spinning neutron stars–four isolated and one in a binary system. Another seven contain central unresolved sources or bright nebulae. Observations of these nebulae, probably due to synchrotron emission, are used to estimate characteristics of the unseen pulsars.

Type
I. Rotation-Powered Pulsars
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 99 - 108
Copyright
Copyright © Reidel 1987 

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