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The Origin and Interpretation of Line Profile Variations of Pulsating B Stars

Published online by Cambridge University Press:  12 April 2016

J. De Bidder  and
C. Aerts
J. De Bidder
Affiliation:
Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, B-3001 Heverlee, Belgium
C. Aerts
Affiliation:
Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, B-3001 Heverlee, Belgium

Abstract

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We report on an ongoing study on the importance of the contributions of different photospheric variations to the line profile variations of hot pulsating stars.

Type
Part 6. Variables Close to the Main Sequence
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 432 - 433
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Becker, S.R. & Butler, K. 1990, A&AS, 84, 95 Google Scholar
Osaki, Y. 1971, PASJ, 23, 485 Google Scholar