The cause of the type I intermittency for hydrodynamic pulsation models-Reference-Cited by-同舟云学术

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The cause of the type I intermittency for hydrodynamic pulsation models

Published:1988 Issue:1 Volume:149 Page:149-161
ISSN:0004-640X
Container-title:Astrophysics and Space Science
language:en
Short-container-title:Astrophys Space Sci

Author:

Aikawa Toshiki

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00640475.pdf

Reference28 articles.

1. Aikawa, T.: 1985,Astrophys. Space Sci. 116, 401.

2. Aikawa, T.: 1987,Astrophys. Space Sci. 139, 214.

3. Aikawa, T.: 1988,Sci. Rep., Tohoku Univ., 8th Ser. 8, 113.

4. B�hm-Vitense, E.: 1958,Z. Astrophys. 46, 108.

5. Buchler, J. R., Goupil, M.-J., and Kovacs, G.: 1987,Phys. Letters A 126, 177.

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1. Characterization of intermittent chaos and oscillating frequencies in some pulsating stars;Astrophysics and Space Science;1994

2. Bifurcation in hydrodynamic models of stellar pulsation;Astrophysics and Space Science;1993-12

3. A dynamical systems approach to nonlinear stellar pulsations;Astrophysics and Space Science;1993-12

4. A Dynamical Systems Approach to Nonlinear Stellar Pulsations;International Astronomical Union Colloquium;1993

5. Bifurcation in Hydrodynamic Models of Stellar Pulsation;International Astronomical Union Colloquium;1993

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