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Fig. 1.


Chandra 0.5–8 keV cutout (left panel) and HST images with colours in log scale. In the Chandra image, blue contours represent F435W fluxes. In the F435W image, we labelled the two major tidal tails, T1 and T2, that extend over tens of kpc and possibly overlap on the right of the SE nucleus in the figure. A shell-like region (S) is also indicated. In the three-colour cutout, the white boxes show the GMOS FOV from which previous spatially resolved kinematic results have been obtained by Rupke & Veilleux (2013). The white contour represents the S/N = 40 level in the stellar continuum map at ∼5550 Å and is taken as a reference in the next figures. The MaNGA field of view is also shown with white dashed lines.

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