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Low-Mass X-ray Binaries—Recent Developments

Published online by Cambridge University Press:  25 May 2016

M. Van Der Klis*
Affiliation:
Astronomical Institute “Anton Pannekoek”, and Center for High-Energy Astrophysics, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands

Abstract

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Recent developments in the field of low-mass X-ray binaries are briefly reviewed, with particular emphasis on a comparison between the systems that contain accreting low magnetic-field neutron stars and those that contain black-hole candidates. The possibility that inclination effects play a role in black-hole candidate phenomenology is explored.

Type
5 X-ray Binaries
Copyright
Copyright © Kluwer 1996 

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