Fig. 10
Left panels: colour-coded Hertzsprung-Russell diagram for different stellar masses. The colour code represents the values of A(Li) at the stellar surface. Right panels: the evolution of surface lithium abundance (from the ZAMS to the end of the He-burning phase) as a function of effective temperature. Circles and diamonds denote, respectively, Li detections and upper limits for stars with [Fe/H] <−0.26 (top panels), −0.26 ≤ [Fe/H] <−0.125 (middle panels), and [Fe/H] ≥−0.125 (bottom panels). Error bars are shown for all stars.
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