Fig. 4
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Duration of the phase during which the stars evolve into the RGB (black squares and lines) and the AGB (red dots and lines) boxes introduced by H23 as a function of the initial mass (left) and the formation epoch (right). Dotted lines and green triangles refer to the results obtained by assuming 0.2 M⊙ mass loss during the RGB evolution of M < 1.5 M⊙ stars.
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