Three-mode Cepheid pulsation |
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| Authors: | T Ishida M Saitou |
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| Institution: | (1) Astronomical Institute, Faculty of Science, Tohoku University, Sendai, Japan;(2) Present address: Hitachi System Engineering, Ltd., Shinagawa-ku, Tokyo, Japan |
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| Abstract: | We simulated two models of classical Cepheids with the same effective temperature and luminosity but different masses. Neither model has significant resonance among linear nonadiabatic periods of the fundamental, the first overtone, and the second overtone radial modes. The higher mass model found to approach to the second overtone-only state. The lower mass model shows a complicated three-mode interaction and none of the amplitudes of three modes is negligible. The relation of the higher mass model to the shortest period Cepheid HR 7308, and that of the lower mass model to the double-mode Cepheids are discussed. It appears that three-mode nonresonant coupling should be considered to explain the behaviours of both models. |
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