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Neutron Stars in Twelve Supernova Remnants
Published online by Cambridge University Press: 04 August 2017
Abstract
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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