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Periods of β Cephei and SPB Stars from Hipparcos Photometry1

Published online by Cambridge University Press:  12 April 2016

J. Molenda-Żakowicz
J. Molenda-Żakowicz*
Affiliation:
Wroclaw University Observatory, ul. Kopernika 11, 51-622 Wroclaw, Poland

Abstract

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For the β Cephei variables, we compare the periods derived from ground-based observations with those given in the Hipparcos catalogue. For the SPB stars, of which most have been discovered by Hipparcos, we examine the question of multiperiodicity.

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. 434 - 435
Copyright
Copyright © Astronomical Society of the Pacific 2000

Footnotes

1

Based on data from the Hipparcos astrometry satellite.

References

Cousins, A.W.J. 1982, IBVS, No. 2158 Google Scholar
Heynderickx, D. 1992, A&AS, 96, 207 Google Scholar
Jerzykiewicz, M. & Pigulski, A. 1999, MNRAS, in pressGoogle Scholar
Lomb, N.R. & Shobbrook, R.R. 1975, MNRAS, 173, 709 CrossRefGoogle Scholar
Sterken, C. & Jerzykiewicz, M. 1993, Space Sci. Rev., 62, 95 CrossRefGoogle Scholar
Waelkens, C., Aerts, C., Kestens, E., Grenon, M., & Eyer, L. 1998, A&A, 330, 215 Google Scholar