Fig. 8.
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Stellar mass properties at the end of core H burning (MTAMS) and the end of core He burning (final) for models calculated at ZSMC (green) and 10% Z⊙ (black) for a range of critical rotation rates (0% in solid lines, 40% in dashed lines, and 70% in dash-dotted lines). A 1:1 mass ratio has been plotted for each panel in grey dotted lines.
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