Free Access
Fig. 1
Kinematics of the Milky Way BHB stars. From top to bottom: radial velocity of the stars in kms-1, radial velocity dispersion calculated in a given bin with s3 and s4 parameters, which describe symmetric and asymmetric departures from the Gaussian, respectively.
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.