Fig. 7
Detail of Fig. 4 with focus on the late-type stars with log (L/L⊙) > 3.4 that might be Quintuplet RSG candidates. Tracks show stellar evolution models from Meynet & Maeder (2003) with and without rotation (solid and dashed lines, respectively) and from Bressan et al. (1993, solid line with circles for Mini = 6 and 7 M⊙.
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