Highlight
Free Access

Fig. 3

thumbnail

[Fe/H] ratios as a function of effective temperature for stars analysed in NGC 1851 (upper panel), M 4 (middle panel), and M 5 (lower panel), both from Carretta et al. (2009a,b). The filled red circles indicate stars with GIRAFFE spectra, the blue filled squares stars with UVES spectra. Error bars in the left and right side of the panels refer respectively to our GIRAFFE and UVES data and indicate star-to-star errors.

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.