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Convective Instability of Hydrogen-Burning Shells in β–Cephei Stars

Published online by Cambridge University Press:  25 April 2016

R. Van der Borght
R. Van der Borght*
Affiliation:
Department of Mathematics, Monash University, Clayton
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Extract

It appears that the relative number of β–Cephei variables among the early B stars is comparable to the fraction of the evolutionary lifetime spent in the secondary contraction and early shell-burning phases (Lesh and Aizenman 1973a) and it may therefore be of some interest to investigate possible instability mechanisms associated with hydrogen shell-burning in stars within the mass range of 10 to 15 M⊙ (Lesh and Aizenman 1973b).

Type
Stellar
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 5 , September 1974 , pp. 269 - 270
Copyright
Copyright © Astronomical Society of Australia 1974

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References

Davey, W. R., Astrophys. J., 179, 235 (1973).Google Scholar
Kato, S., Publ. Astron. Soc. Japan, 18, 374 (1966).Google Scholar
Lesh, J. R., and Aizenman, M. L., Astron. Astrophys., 26, 1 (1973a).Google Scholar
Lesh, J. R., and Aizenman, M. L., Astron. Astrophys., 22, 229 (1973b).Google Scholar
Sakashita, S., and Hayashi, C., Prog. Theor. Phys., 22, 830 (1958).Google Scholar
Sakashita, S., and Hayashi, C., Prog. Theor. Phys., 26, 942 (1961).Google Scholar
Schwarzschild, M., and Härm, R., Astrophys. J., 128, 348 (1958).CrossRefGoogle Scholar
Stothers, R., Astrophys. J., 141, 671 (1965).CrossRefGoogle Scholar
Veronis, G., J. Marine Res., 23, 1 (1965).Google Scholar