Fig. 5.
Stellar light kinematic maps for FCC 47 acquired from the Voronoi-binned MUSE cube. Top left: mean relative velocity of the integrated light with respect to a systemic velocity of 1444 km s−1. Top right: velocity dispersion σ. Bottom left: h3 and bottom right: h4. The inset shows a zoom to the central region to highlight the inner structure. We show the same isophotes as used in Fig. 1. The effective radius of the NSC (0.7″) corresponds to the radius of the innermost isophote contour.
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