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The Coupling Coefficients of Radial Pulsation in Third Order

Published online by Cambridge University Press:  12 April 2016

T. Ishida ,
R. Takano ,
F. Yamakawa  and
M. Takeuti
T. Ishida
Affiliation:
Nishi-Harima Astronomical Observatory, Ohnadesan, Sayo-cho, Hyogo 679-53, Japan
R. Takano
Affiliation:
Astronomical Institute, Tóhoku University, Sendai 980, Japan
F. Yamakawa
Affiliation:
Space System Dept., Fujitsu Ltd., Nakase 1-chome, Mihama-ku, Chiba 261, Japan
M. Takeuti
Affiliation:
Astronomical Institute, Tóhoku University, Sendai 980, Japan

Abstract

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The third order theory of coupling is discussed regarding the radial pulsation of stellar models.

Type
III. Models
Information
International Astronomical Union Colloquium , Volume 134: Nonlinear Phenomena in Stellar Variability , 1993 , pp. 349
Copyright
Copyright © Kluwer 1993

References

Buchler, J.-R. and Goupil, M.-J.: 1984, Astrophysical Journal 279, 394.Google Scholar
Schwarzschild, M. and Savedoff, M.P.: 1949, Astrophysical Journal 109, 298.Google Scholar
Takeuti, M. and Aikawa, T.: 1981, Sci. Reports Tôhoku Univ., Eighth Ser. 2, 106.Google Scholar
Takeuti, M. Yamakawa, F., and Ishida, T.M.: 1992, Publications of the ASJ to be published.Google Scholar