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Nonlinear oscillations in the convective zone

  • Wasaburo Unno
  • Da-run Xiong
Part III Excitation Mechanism of Oscillations
Part of the Lecture Notes in Physics book series (LNP, volume 367)

Abstract

Radiation-hydrodynamics for stellar oscillations in convective zone (Xiong 1989 is reformulated into a form suitable for non-linear dynamical interpretation of semi-regular and irregular variability of red super-giant stars.

Keywords

Nonlinear Oscillation Eddy Viscosity Convective Zone Convective Flux Molecular Viscosity 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Kamijo, F. 1963, Publ. Astron. Soc. Japan, 15, 1.Google Scholar
  2. Nakano, T., Fukushima, T., Unno, W., and Kondo, M. 1979, Publ. Astron. Soc. Japan, 31, 713.Google Scholar
  3. Saitou, M., Takeuti, M., and Tanaka, Y. 1989, Publ. Astron. Soc. Japan, 41, 297.Google Scholar
  4. Yuasa, M., Unno, W., and Chikawa, M. 1989, Science and Technology (Kinki University), 1, 35.Google Scholar
  5. Xiong, D.-R. 1989, Astron. Astrophys., 209, 126.Google Scholar

Copyright information

© Springer-Verlag 1990

Authors and Affiliations

  • Wasaburo Unno
    • 1
  • Da-run Xiong
    • 2
  1. 1.Res. Inst. Sci. Tech.Kinki UniversityOsakaJapan
  2. 2.Purple Mountain ObservatoryNanjingChina

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