X-ray variability of the O star ζ Puppis

  • Thomas W. Berghöfer
Variable Winds
First Online:
Part of the Lecture Notes in Physics book series (LNP, volume 523)

Keywords

Stellar Wind Sinusoidal Model Star Wind ROSAT PSPC Einstein Observatory 
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.
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References

  1. Berghöfer, T. W., Schmitt, J. H. M. M. 1994a, A&A 290, 435ADSGoogle Scholar
  2. Berghöfer, T. W., Schmitt, J. H. M. M. 1994b, ROSAT X-ray light curves of early-type stars, In: Astrophys. Space Sci. 221, 309Google Scholar
  3. Berghöfer, T. W., Schmitt, J. H. M. M. 1994c, Science 265, 1689CrossRefADSGoogle Scholar
  4. Berghöfer, T. W., Schmitt, J. H. M. M. 1995, Long term X-ray variability studies of OB-type stars, In: Adv. Space Res. Vol. 16, No. 3, p. 163Google Scholar
  5. Berghöfer, T. W., Schmitt, J. H. M. M., Cassinelli, J. P. 1996, A&AS 118, 481ADSCrossRefGoogle Scholar
  6. Berghöfer, T. W., Baade, D., Schmitt, J. H. M. M., et al. 1996, A&A, 306, 899ADSGoogle Scholar
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Copyright information

© Springer-Verlag 1999

Authors and Affiliations

  • Thomas W. Berghöfer
    • 1
    • 2
  1. 1.Space Sciences LaboratoryUniversity of CaliforniaBerkeleyUSA
  2. 2.Hamburger SternwarteHamburgGermany

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