Characterisation of the Dynamics of a Variable Star



Tentatives to detect chaos in variable stars are presented. Constraints on the accuracy on individual measurements and length of the records, necessary to obtain de-fenitive conclusions, are discussed. Some directions for future improvements are sketched.


Fourier Spectrum Chaotic Attractor White Dwarf Physical Review Letter Variable Star 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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© Springer Science+Business Media Dordrecht 1993

Authors and Affiliations

  1. 1.Observatoire de Paris-MeudonDASAL. URA CNRSMeudonFrance

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