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The Changing Blazhko Effect of XZ Cygni
Published online by Cambridge University Press: 12 April 2016
Abstract
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An analysis of new and old photometry of the RR Lyrae star XZ Cyg indicates that both its primary period and its Blazhko period have undergone significant changes.
- Type
- Part 3. Nonlinear Effects in Pulsating Stars
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2002
References
Shibahashi, H.
2000, in ASP Conf. Ser., Vol. 203, The Impact of Large-Scale Surveys on Pulsating Star Research, eds. Szabados, L. & Kurtz, D.W., (San Francisco ASP), 299
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