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Fig. 20

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Left: evolution of 6Li/7Li ratio as a function of [Fe/H] (left) and of time (right). Data are taken from Asplund et al. (2006, As06), Garcia-Perez et al. (2009, GP09) and Kawanomoto et al. (2009, K09). Solid curves correspond to Model A and dotted curves to Model B, respectively, both starting with standard (low) pre-galactic 6Li; dashed curves correspond to Model A with high pre-galactic 6Li.

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