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The ROSAT Observations of Classical Novae

  • M. Orio
  • H. Ögelman
  • S. Balman
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 208)

Abstract

We observed a number of classical and recurrent novae in the Galaxy and the LMC with the ROSAT X-ray telescope and searched the archival data for other serendipitous observations. Preliminary results show that only 9 out of 37 observed objects were bright enough in X-rays to be detected with ROSAT, either in outburst or at quiescence.

Keywords

Thin Shell Archival Data White Dwarf Thermal Plasma Related Object 
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. Krautter, J., Ögelman, H., Starrfield, S., et al., 1996, Ap. J., 456, 788ADSCrossRefGoogle Scholar
  2. O’Brien, T. J., Lloyd, H. M., Bode, M. F., 1994, MNRAS, 271, 155ADSGoogle Scholar
  3. Ögelman, H., Orio, M., Krautter, J., Starrfield, S., 1993, Nature, 361, 331ADSCrossRefGoogle Scholar
  4. Shanley, L. Ögelman, H., Gallagher, J., et al., 1995, Ap. J., 438, L95ADSCrossRefGoogle Scholar

Copyright information

© Kluwer Academic Publishers 1996

Authors and Affiliations

  • M. Orio
    • 1
    • 2
  • H. Ögelman
    • 1
  • S. Balman
    • 1
  1. 1.Department of PhysicsU WisconsinMadisonUSA
  2. 2.Osservatorio Astronomico di TorinoItaly

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