The effect of convection in nonlinear one-zone stellar models

Details The effect of convection in nonlinear one-zone stellar models The effect of convection in nonlinear one-zone stellar models

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.210..355s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 210, no. 1-2, p. 355-358

Astronomy and Astrophysics

Astrophysics

2

Chaos, Convection, Nonlinearity, Stellar Models, Stellar Oscillations, Variable Stars, Astrophysics, Period Doubling, Temperature Effects

Scientific paper

We study the convective nonlinear one-zone models of the pulsating variable stars. In the small convective case, the solution shows chaotic behavior through the period doubling bifurcation as the temperature is lower although the temperature at which the chaos appears is lower than in the case of no convection. On the other hand, in the strong convective case, the solution only shows period-one limit cycle.

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