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Fig. 5


Left: pixel values within rhm of h3 (upper panel), h4 (bottom panel) versus V/σ extracted from the simulated kinematic maps for all the simulated remnants M0–M3. Different colors correspond to the different B/T ratios of their progenitors. Right: same as the left panel for one of the CALIFA prolate-rotating galaxies, LSBCF560-04, that shows weak evidence for an h3-V/σ correlation.

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