A discrete-dynamic study of pulsating stars

Details A discrete-dynamic study of pulsating stars A discrete-dynamic study of pulsating stars

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.136..129t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 136, no. 1, Aug. 1987, p. 129-132.

Statistics

Computation

11

Computational Astrophysics, Kinetic Energy, Stellar Oscillations, Variable Stars, Astronomical Models, Chaos, Maxima

Scientific paper

A sequence of successive kinetic energy maxima at the expanding phases of pulsating stars is used as a discrete-dynamic expression of stellar pulsation. It is shown that the transition from the periodic pulsation to the irregular one can be explained by the rate of dissipation. Thus, the semiirregular and irregular stellar pulsation may be produced by the stong dissipation of large-amplitude pulsations.

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