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Fig. 9.

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Lithium abundance as a function of Teff. The upper envelopes of A(Li) for IC 2602 (age ≈ 30 Ma), the Pleiades (≈100 Ma), NGC 6475 (≈300 Ma), and the Hyades (≈600 Ma) clusters adapted from Sestito & Randich (2005) are overplotted.

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