Fig. 3
Download original image
Comparison with Galactic chemical evolution models – when available – with the reported [Y/Fe], [Zr/Fe], [Ba/Fe], [La/Fe], [Ce/Fe], [Pr/Fe], [Nd/Fe], and [Eu/Fe]. The background, coloured in grey, scales with the logarithmic number of stars in each bin. The correspondent abundances of candidate stars of GSE (François et al. 2024; Lucertini et al. 2025), Sequoia (François et al. 2024; Lucertini et al. 2025), Ceres (Lombardo et al. 2021; Lombardo 2023), halo stars (Lucertini et al. 2025), the Gaia-ESO sample of disc stars, and thick disc stars (François et al. 2024; Lucertini et al. 2025) are shown as in blue diamonds, red triangles, black pluses, yellow dots, blue crosses, and black stars, respectively.
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.