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Nonlinear models of first overtone mode Cepheids

E. Antonello, T. Aikawa

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Abstract

Nonlinear models of population I Cepheids pulsating in the first overtone mode have been constructed using augmented opacities and a nonstandard mass-luminosity relation. The properties of the Fourier parameters of their light curves are discussed and compared with those of observed stars. It is shown that the models reproduce in part the observed behavior of first overtone Cepheids, and confirm the importance of the resonance P 1 /P 4 =2 between the first and fourth overtone modes

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What this paper is about

Nonlinear models of population I Cepheids pulsating in the first overtone mode have been constructed using augmented opacities and a nonstandard mass-luminosity relation. The properties of the Fourier parameters of their light curves are discussed and compared with those of observed stars. It is shown that the models reproduce in part the observed behavior of first overtone Cepheids, and confirm the importance of the resonance P 1 /P 4 =2 between the first and fourth overtone modes

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Available abstract

Nonlinear models of population I Cepheids pulsating in the first overtone mode have been constructed using augmented opacities and a nonstandard mass-luminosity relation. The properties of the Fourier parameters of their light curves are discussed and compared with those of observed stars. It is shown that the models reproduce in part the observed behavior of first overtone Cepheids, and confirm the importance of the resonance P 1 /P 4 =2 between the first and fourth overtone modes

Key concepts: Cepheid variable, Overtone, Physics, Astrophysics, Light curve, Stars, Population, Nonlinear system

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