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Fig. 8

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Upper panel: as in Fig. 7, but for a CMD region centred on the RC position and for stars inside 5′. The blue triangles are the UVES candidate members. The open triangle is the outlier in chemical abundance (see Table 4). Lower panel: the UVES target candidate members in the theoretical log g vs. Teff plane (only the 13 stars with complete analysis).

This figure is made of several images, please see below:

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