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Analysis of line profile variations in pulsating B stars

  • C. Waelkens
  • C. Aerts
IV. Non-classical Phenomena in Early-Type Stars
Part of the Lecture Notes in Physics book series (LNP, volume 401)

Keywords

Line Profile Mode Identification Moment Method Pulsation Parameter Radial Mode 
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. Baade, D., 1988, IA U Symposium 132: The Impact of Very High SIN Spectroscopy on Stellar Physics, G. Cayrel de Strobel and M.Spite,edrs., 217Google Scholar
  2. Baade, D., 1990, edr., ESO Workshop on Rapid variability of OB-stars: nature and diagnostic value Google Scholar
  3. Gies, D.R., Kullavanijaya, A., 1988, Astrophys. J. 326, 813Google Scholar
  4. Heynderickx, D., 1991, Ph D Thesis KU LeuvenGoogle Scholar
  5. Lee, U., Saio, H., 1987, Mon. Not. R. astr. Soc. 224, 513Google Scholar
  6. Penrod, G.D., 1986, Publ. Astron. Soc. Pacific 98, 35Google Scholar
  7. Waelkens, C., 1991, Astron. Astrophys. 246, 453Google Scholar
  8. Waelkens, C., Cuypers, J., 1985, Asiron. Astrophys. 152, 15Google Scholar
  9. Watson, R.D., 1988, Astrophys. Space Sci. 140, 255Google Scholar

Copyright information

© Springer-Verlag 1992

Authors and Affiliations

  • C. Waelkens
    • 1
  • C. Aerts
    • 1
  1. 1.Astronomisch InstituutLeuvenBelgium

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