Abstract
The Models of solar type stars are unstable to non-radial oscillations driven by burning 3He. These oscillations modify the distribution of 3He leading to finite amplitude oscillations with typical temperature perturbations ST/T ~ 0.1.
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References
Christensen Dalsaard J, Dilke F WW and Gough D 0, 1974 Mon. Not. Roy. Ast. Soc., 169, 429.
Christensen Dalsgaard J, Duvall T L, Gough D O, Harvey J W and Rhodes E J, 1985, Nature, 315, 378.
Dilke FWW and Gough D O, 1972, Nature 240, 262.
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© 1986 D. Reidel Publishing Company, Dordrecht, Holland
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Roxburgh, I.W. (1986). Finite Amplitude Limit of the 3He Instability. In: Gough, D.O. (eds) Seismology of the Sun and the Distant Stars. NATO ASI Series, vol 169. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4608-8_28
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DOI: https://doi.org/10.1007/978-94-009-4608-8_28
Publisher Name: Springer, Dordrecht
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