Fig. 17
Same as Fig. 11 for a thick disc stellar particle evolution in the orbits integration (first row and thin lines ofthird row) and in the simulation (second row and thick lines of third row) in which the stellar particle is an extreme migrator. The lack dash-dotted line shows time evolution of the corotation radius (bottom left panel) and of Ωp (bottom right panel) in the simulations.
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.