Fig. 8.
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Velocity maps of region ID26. Left panel: velocity field near the hinge clump. This map was derived from a single Gaussian fit on the Hα emission line observed with Gemini/GMOS. Right panel: Hα velocity dispersion map of the same region as shown in the left panel. The top two panels show a white square that corresponds to a poor fiber in the IFU/GMOS.
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