Panels from top to bottom: mean azimuthal velocity, radial, vertical and azimuthal velocity dispersion of stars, as a function of their [Fe/H] abundance. In each panel, the relations are for various bins in [Mg/Fe], as indicated in the legend in the top panel. The black curves in each panel show the relation for the total sample. The 1σ uncertainty in each relation (coloured region around each relation) is estimated using 1000 bootstrapped realizations. In all panels, only bins containing more than 10 stars are shown.