Titlebook: Nonlinear Phenomena in Stellar Variability; M. Takeuti,J.-R. Buchler Book 1993 Springer Science+Business Media Dordrecht 1993 Accretion.Va

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Predicting Variable Star Light Curvestion 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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the estimate of stability, the appearance and disappearance of possible modes can be studied in detail. While nonlinearity in stellar pulsations is not a very complicated concept, it generally requires extensive and sometimes so­ phisticated numerical studies. Therefore, the development of appropri

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