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Fig. 1.

Fig. 1. Refer to the following caption and surrounding text.

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Maps of B★, vlos, and stellar sAMSD for UGC9969. Left panel: SB in the 3.4 μm WISE W1 band. The transparent pixels correspond to the regions where the SB profile was used to fill the map after the foreground star removal process. Middle panel: Hα velocity map (solid colour vlos) on top of the Hα + H I RC projected on the sky (transparent vlos). Right panel: Stellar sAMSD per pixel computed using Eq. (5).

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