Volume 371, Number 2, May IV 2001
|Page(s)||667 - 671|
|Section||Interstellar and circumstellar matter|
|Published online||15 May 2001|
Period-doubling behavior in very slow classical cepheid models
Tohoku Gakuin University, Izumi-ku, Sendai 981-31, Japan
Corresponding author: T. Aikawa, firstname.lastname@example.org
Accepted: 9 March 2001
In a search of nonlinear models for very long-period Cepheids, we found models with period-doubling behaviors. The feature is quite similar to that mentioned by Carson & Stothers (1984). Here, we report the main features of these models, and briefly discuss the origin of the period-doubling behavior.
Key words: stars: variables: Cepheids stars: variables: general-stars: oscillations
© ESO, 2001
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