Fig. 13.

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Change of the C/N and N/O ratios on the surface of the models given at seven different times in the evolution; at the zero-age main sequence (ZAMS), half-way the main sequence (MMS), at the terminal-age main sequence (TAMS), on the Hertzsprung gap (HRG), and at the onset of helium burning (ZAHeB). The symbols are for the different values for αov while the colours indicate the different amounts of log(Denv/cm2 s−1) in the same way as in the previous figures.
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