Table 4: Mean core abundance variations during MS of the 60 $M_\odot $ models. $\delta {\rm {X}}$ refers to the amplitude (in dex) of variation of element X. For NGC 6752 it refers to the amplitude variation observed between polluted and unpolluted stars.
Model $\delta{\rm {C}}$ $\delta{\rm {N}}$ $\delta{\rm {O}}$ $\delta{\rm {Na}}$ $\delta{\rm {Mg}}$ $\delta{\rm {Al}}$
NGC 6752 -0.7 1.7 -1.0 0.9 -0.3 1.4
60rA -0.9 1.5 -1.8 1.6 0.5 0.7
60rB -0.9 1.5 -1.8 1.6 0.0 0.7
60rC -0.9 1.5 -1.8 1.0 -0.1 0.7
60rD -0.9 1.5 -1.8 1.0 -0.4 1.3

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