Two-mode model of the chaotic stellar pulsation

Details Two-mode model of the chaotic stellar pulsation Two-mode model of the chaotic stellar pulsation

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aipc..285..553v&link_type=abstract

Noise in physical systems and 1/f fluctuations. AIP Conference Proceedings, Volume 285, pp. 553-556 (1993).

Physics

Pulsations, Oscillations, And Stellar Seismology, Hydrodynamics

Scientific paper

The interacting modes model describing the W Vir variables behavior is considered. It is demonstrated, that nonisochronism plays an essential role in appearance of multifrequency regimes and stochastization processes. The model considered supposedly is the simplest one which describes such an interesting phenomenon, as multistability. Thus, it seems reasonable to say, that nonisochronism has to be taken into account in investigation of the stellar eigenmodes interaction.

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