Fig. 5.
Velocity map (left) and associated error (right) of the ionised gas derived from MUSE for emission lines with an S/N > 5. The velocity of the gas is given relative to the systemic velocity of the galaxy of −170 km s−1 derived from HI observations. The white cross, star, and filled circle show the position of the photometric, stellar, and gas kinematical centres.
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