Fig. 15.
Comparison of 0.55-M⊙ models with 1.5 × 10−7 M⊙ yr−1 initial accretion rate for different assumptions on the depth of mixing. Left panel: models where accreted gas is only mixed with the outermost convective zone. Middle panel: mixing down to the He II convective zone. Right panel: mixing down to the deep convective regions (at T ∼ 200 000 K).
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