Fig. A.1.
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Luminosity during the RSG phase as a function of the initial mass of the star. The points are distributed in 100 equal timesteps that span the whole time range of each model during its RSG phase, colored by the central helium mass fraction. For reference, we also show the luminosity at TAMS and various fittings from this or previous works, of the form of Eq. A.1.
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