Chaotic pulsations in stellar models
- Florida Univ., Gainesville (USA)
The irregular behavior of large-amplitude pulsating stars undergoing radial oscillations is examined theoretically, with a focus on hydrodynamic simulations of the W Virginis population II Cepheids (stars which show both regular and RV Tau characteristics). Sequences of models are constructed as one-parameter families (with luminosity, mass, and composition fixed and Teff as the control parameter) and analyzed to derive a systematic map of the bifurcation set; i.e., of the possible types of pulsations. The results are presented graphically, and it is shown that both cascades of period doubling (via destabilization of an overtone through a half-integer-type resonance) and tangent bifurcation are possible routes to chaos in these systems, depending on the stellar parameters. The general robustness of the chaotic behavior and the existence of a 'chaotic blue edge' in stellar-parameter space are demonstrated. 55 refs.
- OSTI ID:
- 5760019
- Report Number(s):
- CONF-8910308-; CODEN: ANYAA
- Journal Information:
- Annals of the New York Academy of Sciences; (USA), Vol. 617; Conference: 5. Florida workshop in nonlinear astronomy, Gainesville, FL (USA), 5-7 Oct 1989; ISSN 0077-8923
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
GENERAL PHYSICS
PULSATING VARIABLE STARS
STAR MODELS
ASTROPHYSICS
CEPHEIDS
CHEMICAL COMPOSITION
LUMINOSITY
MASS
MATHEMATICS
OSCILLATIONS
PULSATIONS
MATHEMATICAL MODELS
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
STARS
VARIABLE STARS
640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar
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