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Fig. 19

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Evolution of total Li (solid curves), 6Li (dashed curves) and 7Li from GCR (dotted curves) in the standard case (low 6Li from SBBN, thick curves) and in the case of high pre-galactic 6Li and 7Li (thin curves). In the latter case, a minimum amount of depletion of 6Li within stars (equal to that of 7Li) has been conservatively assumed. 7Li data for halo stars are as in Fig. 16, while 6Li data are from Asplund et al. (2006, As09, open squares) and Garcia-Perez et al. (2009, GP09, filled circles).

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