UVW galactocentric space velocities of young moving group members in Montes et al. (2001, Castor, Hyades Supercluster, IC 2391 Moving Group, Local Association, Ursa Major, AB Doradus) along with G 264–012 (in red) and Gl 393 (in blue). Crosses and ellipses correspond to the 1σ and 2σ values for each group, respectively. Over-plotted in grey are the typical UV W values and dispersion for AB Dor according to Gagné et al. (2018).