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Multiperiodicity in the Line-Profile Variations of the Spectroscopic Binary β Cep Star λ Scorpii

Published online by Cambridge University Press:  12 April 2016

K. Uytterhoeven
Affiliation:
Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Belgium
C. Aerts
Affiliation:
Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Belgium

Abstract

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A study of the rapid variations of the line profiles of λ Scorpii leads to the following new result: we find evidence for the presence of at least 5 periodicities in the intrinsic variations of λ Scorpii, which seem to be part of an equidistant multiplet. The modes associated to these periodicities are interpreted as non radial pulsation modes.

Type
Part 1.2. Pulsations in Close Binaries
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

De Mey, K., Aerts, C., Waelkens, C., Cramer, S.R., Schrijvers, C., Telting, J.H., Daems, K., & Meeus, G. 1997, A&A, 324, 1096 Google Scholar
Lomb, N.R., Shobbrook, R.R. 1975, MNRAS, 173, 709 Google Scholar
Uytterhoeven, K., Aerts, C., Ausseloos, M. 2002, in ASP Conf. Ser., Observational Aspects of Pulsating B and A stars, eds. Sterken, C. & Kurtz, D., (San Francisco ASP), in pressGoogle Scholar
Watson, R.D. 1988, Ap&SS, 140, 255 Google Scholar