Distributions of eccentricity for stars between a range of metallicity −1.0 < [Fe/H] < 0.5 as a function of [Mg/Fe]. The lower [Mg/Fe] stars have a thin disk eccentricity distribution with the bulk of the stars on roughly circular orbits. The higher [Mg/Fe] stars have a more thick disk-like distribution with the bulk of the stars having non-circular orbits.
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.