Fig. 8
Envelope mass and abundance evolution in metal-poor 0.8 M⊙ (left panels) and 0.85 M⊙ (right panels) models with different Reimers-type mass-loss rates. The values in the parentheses are the mass-loss rates at log L ≈ 0; the average mass-loss rate during the main sequence is about 50% higher as a result of the mass, radius, and luminosity scaling in Reimers’ law.
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