Open Access

Fig. 4

image

Download original image

3D velocity components of NGC 104 with respect to the mean cluster velocity, as a function of the position angle θi . The combined sample of RGB, AGB, HB, and MSTO stars in each velocity catalogue are shown as black points with errorbars. Top panel: the radial component of the proper motion, with the mean value shown in green. Middle panel: the same as the top panel, but for the tangential component of the proper motion. Bottom panel: the LOS velocity as a function of θi, with the sinusoidal fit to the distribution shown in green and the position angle of the rotation axis θ0 shown as a white star with errorbars.

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.