Fig. 6.
Li abundance vs. stellar metallicity in mass bins for the 397 pre-turn-off stars cooler than 6500 K. The dashed lines at the top represent an approximate representation of the Galactic evolution of Li from Prantzos (2012). The metallicity Z has been converted from [Fe/H] based on the relationship between [Fe/H] and Z in the MARCS model stellar atmospheres.
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