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X-Ray and Optical Observations of by CAM

  • Gavin Ramsay
  • Paul A. Mason
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 208)

Abstract

We present preliminary results of an analysis of X-ray and optical data of the asynchronous AM Her star BY Cam [1]. We use X-ray data from EXOSAT (0.1… 50 keV), Ginga (1.5… 50 keV) and ROSAT (0.1… 2.0 keV) and optical data obtained during a 45-day campaign in 1994.

Keywords

Orbital Period Light Curf White Dwarf Optical Data Spin Period 
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. 1.
    Mason, P.A., Andronov, I.L., Kolesnikov, S.V.,1995, in “Magnetic Cataclysmic Variables”,D. Buckley, B. Warner, ASP Conf. Ser. 85, 493Google Scholar
  2. 2.
    Wynn G., King, A.R., 1992, MNRAS, 255, 83ADSGoogle Scholar

Copyright information

© Kluwer Academic Publishers 1996

Authors and Affiliations

  • Gavin Ramsay
    • 1
  • Paul A. Mason
    • 2
  1. 1.Astronomical InstituteThe University of UtrechtUtrechtThe Netherlands
  2. 2.Astronomy DepartmentCase Western Reserve UniversityClevelandUSA

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