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. 22

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¹⁶O/¹⁷O versus ¹⁶O/¹⁸O. Observations are from Harris & Lambert (1984), Harris et al. (1988) for stars in the 1–3 M_⊙ range. The line symbols are the same as in Fig. 17. The initial values assumed for ¹⁶O/¹⁷O and ¹⁶O/¹⁸O are 1490 and 445 respectively.

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