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Fig. 1
Dredge-up efficiency λ (top) and the abundances of carbon and barium (middle and bottom, respectively) computed at each thermal pulse with the binary˙c and Stromlo codes (solid and dotted lines, respectively) for single star of mass (from left to right) M∗ = 0.9, 1, 1.5 M⊙ and MPMZ = 2 × 10-3M⊙.
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