Fig. 16.
Comparison of 0.55-M⊙ models with 5 × 10−8 M⊙ yr−1 initial accretion rate for different stellar-wind strengths. Left panel: models with the normal wind strength used throughout this work. Middle panel: models with a stellar wind that is weaker by a factor of ten, while right panel: models with two orders of magnitude weaker wind.
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