Fig. 3.

Li abundances vs. Teff for the microlensed dwarf sample. Triangles represent those stars for which we could only determine upper limits on the abundances. The grey circles and triangles in the background represent the 714 stars from Bensby et al. (2014) for which Li abundances are determined in Bensby & Lind (2018) in the exact same way as for the microlensed bulge dwarfs. The sizes of the markers are scaled with the estimated ages, and the bulge stars are also colour coded based on their surface gravities according to the colour bar on the right-hand side.
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.