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Fig. 2.

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Tracks across HR diagram for evolution models adopting Msc (solid lines), compared with tracks adopting MVink from Georgy et al. (2013; dashed lines). New wind prescription gives values for around ∼2 − 6 times lower than the mass-loss adopted for old models, as visualised in Fig. 3. Black stars mark the end of the H-core burning stage, whereas magenta stars mark the end of the He-core burning stage.

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