Outline of the clusters’ velocities and positions within the LMC. In each panel, NGC 1841 is highlighted with triangle symbol. Panel (a) shows the tangential velocity, V_φ, as a function of the radial distance from the LMC centre R. Model circular velocities resulting from a pure NFW profile (orange solid line) and a model composed of a dark matter halo and a stellar disc and bar (green dashed line) are also shown. The size of the stellar bar is indicated by the vertical dashed line. The radial velocity V_R as a function of R is presented in panel (b). Panel (c) illustrates the out-of-plane velocity V_Z as a function of R and panel (d) shows the vertical distance from the plane Z as a function of R.