Fig. 4
Non-LTE Li abundance corrections for the 6707 Å resonance line using the model atom as Lind et al. (2009) and replacing the e + Li collisions from Park (1971) (dashed line) with the new calculations (solid line). The dotted line shows the zero value. In the lower left corner of each plot are the stellar parameters of the model used: Teff/log g/[Fe/H].
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