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Accreting Neutron Stars
Published online by Cambridge University Press: 04 August 2017
Abstract
This paper reviews accreting neutron stars in X-ray binaries, with particular emphasis on how variations in magnetic field strength may be responsible for explaining the spectral and temporal properties observed from the various systems. This includes a review of X-ray pulsars in both low and high mass systems, and a discussion of the spectral properties of the low mass X-ray binaries.
- Type
- II. Accretion Powered Pulsars
- Information
- Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 135 - 148
- Copyright
- Copyright © Reidel 1987
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