Fig. 14
NLTE Li abundance as a function of [Ba/Fe] in each [Fe/H] bin for our sample stars with Li measurements. The range of [Fe/H] is specified in each plot. The [Fe/H] bin size is 0.26 dex. In each bin we label the mean correlation coefficient (R0 (P)) between ALi and [Ba/Fe], the mean correlation significance level (P0), the possibility of ALi – [Ba/Fe] correlation (β > 0) if considering the abundance uncertainties, and the possibility of P < 0.05 for the anticorrelation.
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