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Fig. 6


υsini versus Teff for our sample of stars. Symbols are the same as in Fig. 5. The theoretical predictions here are mean υsini  and correspond to the υeq values at 3.7 Gyr given in Table 5 multiplied by . The filled dot is for S1242, which has been identified as a peculiar Li-rich subgiant in a previous work of ours (Canto Martins et al. 2006).

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