Fig. 8.
Download original image
Comparison of velocity profiles as a function of cylindrical radius R of the AGAMA-04 galaxy disk with those identified using the six different methods of dynamical decomposition. Top panel: Comparison of rotational velocity vϕ. Middle panel: Comparison of the radial velocity profile vR. Bottom panel: Comparison of the vertical velocity profile vz. In all cases, the solid black line corresponds to the velocity profile of the original stellar disk. These profiles are calculated with bins with an equal number of particles.
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.