Fig. 6.
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Velocity difference maps of the stellar and gaseous velocity fields. The left panel is the (υHα–υstar) map at the original spatial resolution of MUSE data, and the other three panels to the right are respectively the (υHα–υstar), (υH I–υstar) and (υHα–υH i) maps, where the MUSE data have been smoothed to match the spatial resolution (FWHM ∼ 18″) of H I data.
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