Fig. 14.
Distribution of orbital weights along long axis of the mean of the five best-fitting models. The dotted lines show the effective radius of the NSC (Reff, NSC = 0.7″, Turner et al. 2012) and FCC 47 (Reff, FCC 47 = 30″, Ferguson 1989). The shaded area shows the region where we lack coverage with the MUSE data along the short axis.
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