Fig. 8
Li vs. age for HIP 100963 (red filled square) based on NLTE analysis and isochronal age. The Li abundance for other stars analyzed by our group in previous works (Ramírez et al. 2011; Meléndez et al. 2012, 2014a; Monroe et al. 2013) is shown with blue filled circles. The lithium abundance errors are smaller than the size of the circles. Li depletion models are also shown with different lines.
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