Fig. 6
Hess diagram of the VPD for all the stars with PM CSE lower than 10 mas yr-1. Stars belonging to NGC 6544 cluster in the lower right corner, while field stars are the cloud around zero. This cloud is significantly elongated along the longitude axis, because of the presence of two populations, disk and bulge, with the disk having a significant rotation.
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.