Fig. 10.

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Post-MS mass loss by the end of core carbon burning of the models at solar metallicity (large markers) and LMC metallicity (small markers). The labeled regions denote which phase of mass loss is the dominant contributor to the total mass lost after the MS. The division of models into RSG/YSG and WR dominant post-MS mass loss corresponds exactly to the division into the low and high MS mass-loss regime, respectively.
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