Thermohaline instability and rotation-induced mixing - I. Low- and intermediate-mass solar metallicity stars up to the end of the AGB

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201118331e]

Fig. 10

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Evolution of the surface abundance of ⁷Li in the 1.25 M_⊙ star up to the RGB tip when considering thermohaline transport but no rotation-induced mixing. The black solid and red dashed curves correspond to computations performed with C_t = 10³ and 10⁴ respectively.

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