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Variations of Light Curve Parameters in Miras with Progressive Period Changes

Published online by Cambridge University Press:  12 April 2016

Vladislava I. Marsakova
Vladislava I. Marsakova*
Affiliation:
Department of Astronomy, Odessa State University, T. G. Shevchenko Park, Odessa 270014, Ukraine

Abstract

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Variations of light curve parameters in Mira variables with progressive period changes have been studied. They lead to a consistent sequence of the stars which is related to the helium flash model.

Type
Part 2. Variability of High-Luminosity Stars
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 130
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Gál, J. & Szatmáry, K. 1995, A&A, 297, 461 Google Scholar
Marsakova, V.I. & Andronov, I.L. 1998, Ap&SS, 257, 49 Google Scholar
Wood, P.R. & Zarro, D.M. 1981, ApJ, 247, 247 CrossRefGoogle Scholar