Fig. 13.
Relative proper motion of the spectroscopic targets, according to our classification: dwarf stars and non-members (filled and empty blue dots), cluster members and probable cluster members (full and empty black dots). The large and small ellipses are centred on the cluster and field mean value, respectively, with semi-axis equal to the standard deviation of the distributions.
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.