Fig. 3.
SINFONI stellar kinematics (derived from CO band-head spectroscopy) of our target galaxies (from top to bottom) NGC 584, NGC 2784, NGC 3640, NGC 4281, NGC 4570, and NGC 7049. From left to right: maps of signal-to-residual noise (S/rN), mean velocity (V), velocity dispersion (σ), and the Gauss-Hermite moments h3 and h4. The black contours indicate the galaxy surface brightness from the collapsed data cube. North is up and east to the left.
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