Abstract
I present a new method to test determinism, in particular the nonlinear behavior, in observed time series of pulsating stars, based on a recent prediction method which exploits the dynamical system theory. A method for filling gaps in data has thereby been constructed. Estimated bounds to the necessary embedding dimension can be obtained and chaotic divergences can be estimated.
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© 1993 Springer Science+Business Media Dordrecht
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Serre, T. (1993). Predicting Variable Star Light Curves. In: Takeuti, M., Buchler, JR. (eds) Nonlinear Phenomena in Stellar Variability. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1062-4_17
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DOI: https://doi.org/10.1007/978-94-011-1062-4_17
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