Spatially resolved stellar kinematics of the BGG in 11 Voronoi bins with sufficient S/N extracted over a 8″ × 8″ field of view. The maps show the line-of-sight velocities v (left), the projected velocity dispersions, σ (middle), and the second velocity moments, V_rms (right). The orientation of the figure differs from the previous figures. The x′ axis points to the north and is aligned with the major axis of the BGG, while the y′ axis points to the west. Note that the spectrum shown in Fig. 6 corresponds to the central resolution element.