Free Access

Fig. 8


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:

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.