Fig. 5.

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Stellar kinematic maps of NGC 7733. Left panel: stellar velocity (V), velocity dispersion (σ), V/σ, and h3 as indicated. The isophotes, equally spaced in 0.15 mag steps, are derived from MUSE intensity maps. Colour bars beside each map indicate the parameter ranges. The black circle on the velocity map marks the bulge, with a radius equal to the bulge effective radius from photometric decomposition using the Ks band NIR image, as detailed in Table 1. Here, 1 arcsec = 737 pc. North is up, and east is to the left. Right panel: h3 vs. V/σ plot for each Voronoi bin. Red circles denote bins within the bulge effective radius (inside the black circle on the velocity map), while grey points represent bins for the entire galaxy.
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