Fig. 15

Relation between the central stellar velocity dispersion (σLOS,0 to the left and σz,0 to the right) and the circular speed of the disks at 2.2hR. The black solid line in each panel indicates the error-weighted fit, and the black dashed lines are the error-weighted RMS scatter in the ratio. The grey lines show the relation determined by Bottema (1993).
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.