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Blazhko Cycles of ω Centauri RRab Stars

Published online by Cambridge University Press:  12 April 2016

Johanna Jurcsik
Johanna Jurcsik*
Affiliation:
Konkoly Observatory of the Hungarian Academy of Sciences

Abstract

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The present observational strategy of globular cluster variables does not favour long observational runs, which are needed to study the modulation properties of Blazhko type RR Lyrae stars. The only globular cluster for which we have enough data (both photographic and CCD) to determine modulation cycles of RRab stars is ω Centauri. Any connection between the modulation periods and other stellar or cluster parameters may serve as a new clue to the explanation of the Blazhko phenomenon.

Type
V. Variability Study
Information
International Astronomical Union Colloquium , Volume 183: Small-Telescope Astronomy on Global Scales , 2001 , pp. 217 - 218
Copyright
Copyright © Astronomical Society of the Pacific 2001

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