Cyg X-2: its Recurrent X-ray Behaviour

  • E. Kuulkers
  • M. Van Der Klis
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 208)

Abstract

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

Keywords

Basic Distinction Cataclysmic Variable Normal Branch Soft Colour Level Episode 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

References

  1. Hasinger, G., van der Klis, M., 1989, A&A, 225, 79ADSGoogle Scholar
  2. Hasinger, G., van der Klis, M., Ebisawa, K., et al., 1990, A&A, 235, 131ADSGoogle Scholar
  3. Hasinger, G., van der Klis, M., Ebisawa, K., et al., 1990, A&A, 235, 131ADSGoogle Scholar
  4. Vrtilek, S.D., Kahn, S.M., Grindlay, J.E., et al, 1986, Ap. J., 307, 698ADSCrossRefGoogle Scholar

Copyright information

© Kluwer Academic Publishers 1996

Authors and Affiliations

  • E. Kuulkers
    • 1
    • 2
  • M. Van Der Klis
    • 1
  1. 1.Astronomical Institute “Anton Pannekoek”University of Amsterdam & Center for High-Energy AstrophysicsAmsterdamThe Netherlands
  2. 2.Astrophysics Division (SA)ESA/ESTECNoordwijkThe Netherlands

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