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Quasi-Periodic Oscillations in Low-Mass X-ray Binaries

Published online by Cambridge University Press:  04 August 2017

M. van der Klis
M. van der Klis*
Affiliation:
Space Science Department of ESA, ESTEC, postbus 299, 2200 AG Noordwijk, The Netherlands

Abstract

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The properties of the rapid, persistent quasi-periodic oscillations (QPO) discovered with EXOSAT in the X-ray flux of at least 7 bright low-mass X-ray binaries are described. Particular attention is given to the various relations observed between QPO frequency and X-ray intensity, the link between QPO and the low-frequency noise in the X-ray intensity and the bimodal properties of in particular Sco X-1, GX 5-1 and Cyg X-2. The merits of the hypothesis that the QPO indicate the presence of a neutron star with a magnetosphere are considered.

Type
IV. Neutron Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 321 - 331
Copyright
Copyright © Reidel 1987 

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