Fig. 2.
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v/σ ratio as function of stellar mass for subhalos in (a) EAGLE-50, (b) EAGLE-eAGN-dT, (c) EAGLE-eAGN-Visc, (d) EAGLE-wAGN, and (e) EAGLE-NoAGN. Black circles display the median v/σ as a function of stellar mass for subhalos in each simulation. Horizontal dashed lines indicate v/σ = 0.5, where the rotation-dominated (v/σ ≥ 0.5) and pressure-dominated (v/σ < 0.5) galaxies are separated.
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