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Fig. 12.
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Evolution of stellar mass (top), radius (middle), and envelope compactness (bottom) as a function of the stellar age for Z = 0.0025 and Ω/Ωc = 0.6. Black dotted lines: V01 case. Red lines: S23 case. Dotted lines are for optically thin winds, solid lines for optically thick winds, and dashed lines for WR-type winds.
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