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Fig. 11


A(Li), [C/H], [N/H], and 12C/13C as a function of temperature in wGb stars compared to different model predictions. The colours of the data points identify the stars as indicated in Table 1. The shaded areas correspond to the regions of these planes that should be populated with points according to the predictions of the different families of models computed here as labelled in Table 6. In the upper left plot, the MildRot (Paper I) label associated with the dark grey area indicates the predictions of rotating models with υZAMS = 50 km s-1 computed and presented in Palacios et al. (2012).

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