Fig. 5.

image

Epicyclic overdensities depicted in colour in different plots showing various phase-space coordinates for model M1. We used the X − Y phase-space to identify epicyclic overdensities. Stars belonging to the epyciclic overdensities are plotted in colour and appear in various Gaia parameter spaces.

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.