Abstract
It is shown that the coincidence between the pulsation periods and the critical frequencies found by Fadeyev (1982) results from strong effects of non-adiabaticity on the linear pulsation periods in low surface gravity models. If we apply the boundary condition of running waves for super-critical pulsations, it is found that the linear growth-rates are considerably affected by the boundary condition.
References
Aikawa, T.: 1984,Astrophys. Space Sci. (to be submitted).
Castor, J. I.: 1971,Astrophys. J. 166, 109.
Fadeyev, Yu. A.: 1982,Astrophys. Space Sci. 86, 143.
Fadeyev, Yu. A.: 1983, private communication to Dr M. Takeuti.
Rosseland, S.: 1949,The Pulsation Theory of Variable Stars, Clarendon Press, Oxford.
Schatzman, E.: 1956,Ann. Astrophys. 19, 51.
Simon, R. L.: 1957, Université de Liège, Institut d'Astrophysique Collection in 8-vo, No. 389.
Takeuti, M.: 1969,Astrophys. Space Sci. 3, 219.
Takeuti, M.: 1980,Space Sci. Rev. 27, 413.
Unno, W.: 1965,Publ. Astron. Soc. Japan 17, 205.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Aikawa, T. Pulsation periods and critical frequencies in low gravity yellow supergiant models. Astrophys Space Sci 104, 405–408 (1984). https://doi.org/10.1007/BF00650313
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00650313