Fig. 9
Yields of 3He as a function of stellar mass, at different metallicities. (Left) Predictions for standard models. (Right) Predictions including thermohaline mixing only (solid lines) and including both thermohaline and rotation-induced mixings (dashed lines, for models computed up to the AGB tip or to 3He exhaustion).
This figure is made of several images, please see below:
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