Fig. 8.
Kinematic information derived from a Gaussian fit to the Hα emission with the Hα velocity field (left panel). The black contours are the contours of the I-band image reconstructed from the MUSE cube. Right panel: FWHM map of the Hα line. The instrumental FWHM is quadratically subtracted. Over-plotted in blue and red contours are the blue (−50, −30, −15 km s−1) and red (15, 25, 35 km s−1) shifted velocity respectively.
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