Fig. 4.
Convective core mass (top row) and age (bottom row) changes due to the inclusion of extra near-core mixing in the models (cf. Table 3, column CBM solution). Left and right columns: comparisons against the RM solution (cf. Sect. 4.3 and Table 3, column RM solution) and the IM solution (cf. Sect. 4.3 and Table 3, column IM solution), respectively.
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