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Fig. 10


MUSE field centered on UGC 6697 smoothed by 10 × 10 pixels fit with two sets of the Hα+[NII] lines with different velocities along the line of sight. After adopting a δv threshold of 75 km s-1 between gas and stars to distinguish the gas emission that is still bound to the galaxy and the stripped gas emission, we separate the onboard gas (left column) and the stripped gas (right column). The flux, velocity, and velocity dispersion maps are displayed from top to bottom, and the gray contours and the cross in each panel are the same as in previous figures.

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