Fig. 7.

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Projected sAM as a function of stellar mass for the ePN.S galaxies. Lenticulars, fast, and slow rotators ellipticals are shown with different colors and symbols as in the legend. We show with progressively decreasing sizes jp, light vs. M*, jp, mass vs. M*, and jp, mass + IMF vs. M*, var IMF. Arrows connect different measures for the same galaxies. Dashed lines show the power-law fit to jp, light vs. M*; solid lines show the fit to jp, mass vs. M*; dotted lines show the fit to jp, mass + IMF vs. M*, var IMF. Purple lines show the fits to the elliptical galaxies (E-FRs+SRs), while green lines show the fits to the lenticulars.
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