Velocities and positions of the young and intermediate-age clusters within the LMC as a function of the radial distance from the galaxy’s centre, R. In each panel, the clusters with less robust isochrone fits are denoted with diamond symbols and grey error bars. Panel a presents the tangential velocity, V_ϕ. Theoretical 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. Panel b shows the radial velocity, V_R; the out-of-plane velocity, V_Z, is presented in panel c; and panel d shows the vertical distance from the plane, Z. In all panels, the clusters are colour-coded by the logarithm of their ages (in years).