Fig. 8.
The extracted kinematic maps with the fractional light contribution fixed to correspond to the photometrically derived one for NGC 448. The bins are selected such that the fractional contribution of the counter-rotating component is greater than 15%. Top-left panel: velocity field of the counter-rotating kinematic component. Top-right panel: velocity dispersion map for the counter-rotating component. Bottom-left panel: velocity field of the main kinematic component. Top-right panel: velocity dispersion map for the main component.
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