Free Access

Fig. 13.


Stars within Gaia DR2 with δϖ/ϖ < 0.10. These stars have been identified as accreted by our neural network using 5D kinematics alone. While the HR diagram is shown, photometric information is not used in these selections. As expected for an accreted population, these stars are nearly uniformly distributed in the l, b plane. See Fig. A.1 for the analogous figure for the stars classified as in situ.

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.