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Fig. 6.
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Evolution of stellar parameters as a function of the of the actual mass of the CS, for three models at Z = 8 × 10−3. Left: surface carbon mass fraction for the 2.5 M⊙ model (red), 2.0 M⊙ (yellow), and 1.5 M⊙ (cyan). Right: core mass variation for the same models reported in the left panel.
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