Abstract
Methods for analyzing time series of long-period variable stars from observational data bases of variable stars are discussed. These methods are compared to obtain the best accuracy for the characteristics of individual variability cycles.
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Translated from Astrofizika, Vol. 49, No. 3, pp. 433–451 (August 2006).
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Andronov, I.L., Marsakova, V.I. Variability of long-period pulsating stars. I. Methods for analyzing observations. Astrophysics 49, 370–385 (2006). https://doi.org/10.1007/s10511-006-0037-8
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DOI: https://doi.org/10.1007/s10511-006-0037-8