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Fig. 5
Comparison between the lithium abundances and stellar effective temperatures obtained in this work with those obtained by Lebzelter et al. (2012), Gonzalez et al. (2009), and Brown et al. (1989). For consistency, our A(Li)LTE determinations are presented for 92 stars (5 dwarfs, 2 subgiants and 85 giants) with detected Li.
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