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Fig. 2.

image

Comparitive plots of stellar quantities over time. Top: luminosity of evolutionary models with varied amounts of mixing with reference to the luminosity and age of the model with the minimum amount of mixing at the TAMS. Bottom: convective core mass of evolutionary models with varied amounts of mixing with reference to the age of the model with the minimum amount of mixing at the TAMS and the core mass of the same model at the ZAMS.

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