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Cyg X-2: Its Recurrent X-Ray Behaviour

Published online by Cambridge University Press:  12 April 2016

E. Kuulkers  and
M. van Der Klis
E. Kuulkers
Affiliation:
Astronomical Institute “Anton Pannekoek”, University of Amsterdam & Center for High-Energy Astrophysics, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands ESA/ESTEC, Astrophysics Division (SA), P.O. Box 299, 2200 AG Noordwijk, The Netherlands
M. van Der Klis
Affiliation:
Astronomical Institute “Anton Pannekoek”, University of Amsterdam & Center for High-Energy Astrophysics, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands

Abstract

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We find evidence for the occurrence of three different types of behaviour which as their basic distinction have different X-ray brightness levels. They are found to be recurrent.

Type
X-Ray Binaries
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 363 - 364
Copyright
Copyright © Kluwer 1996

References

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