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


Fig. 13

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Chemical structure at the turnoff of the 4.0 M star computed without rotation and with rotation for an initial rotation velocity of 300 km s-1 (top and bottom panels respectively). The mass fractions are multiplied by 600 for 3He, by 100 for 12C and 14N, by 2500 for 13C, by 50, 5000, and 6 × 104 for 16O, 17O, and 18O respectively, and by 1500 for 23Na. The vertical arrows show, in both cases, the maximum depth reached by the convective envelope at its maximum extent during the first dredge-up.

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