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Fig. 6.

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Map of the stellar velocities derived from the pPXF fitting. The black square denotes the extent of the 7 × 7 arcsec2 zoom-in region shown in the insert. The position of the CON is marked with a black cross and dashed lines mark the positions of the major and minor axes. Pixels have been binned to achieve a signal-to-noise ratio of 20. An initial signal-to-noise ratio cut of 2 has been applied, with pixels below this threshold omitted from the binning.

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