Fig. 8.
Panels from top to bottom: EW(Li), log g, and γ as a function of Teff for the Li-rich giant (blue squares), (non-Li-rich) giant (fuchsia squares), and NG (green squares) outliers in the field of the young clusters, in all cases without taking into account the rest of field stars. Turquoise squares indicate potential NGs in the 1.01 > γ > 1.0 range.
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