Astrophysics and Space Science

, Volume 136, Issue 1, pp 129–132 | Cite as

A discrete-dynamic study of pulsating stars

  • Mine Takeuti


A sequence of successive kinetic energy maxima at expanding phases of a pulsating star is considered. Transition from strictly periodic stellar pulsation to irregular one can be explained by the change in the rate of dissipation.


Kinetic Energy Energy Maximum Kinetic Energy Maximum Stellar Pulsation Pulsate Star 
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  1. Aikawa, T., Uji-iye, K., Okuda, T., and Takeuti, M.: 1982,Science Reports Tohoku Univ., Ser. 8 3, 82.Google Scholar
  2. Bier, M. and Bountis, T. C.: 1984,Phys. Letters 104A, 239.Google Scholar
  3. Cox, J. P.: 1974,Rep. Prog. Phys. 37, 563.Google Scholar
  4. Fadeyev, Yu. A.: 1982,Astrophys. Space Sci. 86, 143.Google Scholar
  5. Fadeyev, Yu. A.: 1984,Astrophys. Space Sci. 100, 329.Google Scholar
  6. Fadeyev, Yu. A. and Tutukov, V. A.: 1981,Monthly Notices Roy. Astron. Soc. 195, 811.Google Scholar
  7. Li, T. Y. and Yorke, J. A.: 1975,Am. Math. Monthly 82, 985.Google Scholar
  8. Nakata, M.: 1987,Astrophys. Space Sci., in press.Google Scholar
  9. Takeuti, M., Nakawa, M., and Aikawa, T.: 1985,Sci. Report Tohoku Univ. 8th Ser. 5, 180.Google Scholar
  10. Tuchman, Y., Sach, N., and Barkatt, Z.: 1979,Astrophys. J. 234, 217.Google Scholar

Copyright information

© D. Reidel Publishing Company 1987

Authors and Affiliations

  • Mine Takeuti
    • 1
  1. 1.Astronomical Institute, Faculty of ScienceTohoku UniversitySendaiJapan

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