Nearby, Young Moving Groups : Spatial and Kinematic Models

Here we show the Spatial and Kinematic Models that were used to represent nearby, young moving groups in the spatial <em>XYZ </em>and dynamical<em> UVW </em>parameter spaces<em>.</em> The distribution of <em>bona fide</em> members in each parameter space are represented with gaussian ellipsoids that are free to rotate along any axes. Red dots are members, the blue dot is the Sun, the 3D orange ellipsoid and its three projections are the 1.5-sigma contour of the kinematic model, green lines and pale blue dots are projections of the positions of members (red dots). See Gagné et al. (2013, submitted to ApJ) for more details.