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Fig. 4.

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Light-weighted aperture sAM profiles for fast and slow rotators (left panels): ellipticals and S0s are distinguished by solid and dashed lines, respectively. The two mergers, NGC1316 and NGC5128, are shown with dotted gray lines. The right panels show the median jp(≤R)/jp(≤6Re) (top) and the median cumulative angular momentum Jp(≤R)/Jp(≤6Re) profiles (bottom) for galaxies divided into elliptical FRs, S0s, and SRs. The two recent major mergers NGC1316 and NGC5128 are highlighted with gray lines.

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