Unifying the dynamical classification of early-type galaxies: Kinematic deficits in IllustrisTNG versus observations

Open Access

Fig. 9.

κ_rot(all), f_spheroid(all) of the selected ETGs samples in TNG simulation, plotted as a function of $\bar{k_{5}} (R_{e})$ $Mathematical equation: $ \overline{k_{5}}(R_{\mathrm{e}}) $$ . No clear correlation appears between κ_rot(all) and f_spheroid(all) of the selected ETGs samples in the TNG simulations. The red and blue dots represent the TNG50 and TNG100 samples, respectively.

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