Fig. 12
Upper panel: behaviour of the surface luminosity as a function of time for two HB models with the same mass (see labels). The solid line corresponds to our computations, while the dashed line displays results by Cassisi et al. (1997). Lower panel: as in the upper panel, but for 0.8 M⊙ calculations from the zero age MS to the RGB tip, also including a YY model.
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