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Fig. 1
The Hertzprung-Russel diagram, as well as the evolution of Teff, log g, the temperature at the base of the SCZ (TBSCZ), the outer mass at the base of the SCZ (ΔMBSCZ), and the mass fraction of hydrogen in the core (Xc) for stars of 0.6 − 0.8 M⊙ with Z0 = 0.00017 and Ṁ = 10-12 M⊙ yr-1.
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