What drives the corpulence of galaxies? - I. The formation of central compact dwarf galaxies in TNG50

Open Access

Fig. 13.

Same as Fig. 3, but for the angular momentum of the current accreting gas (negative radial velocity, v_r < 0 km s⁻¹) measured in the region above two times the half-gas-mass radius (r > 2 r_1/2, gas). Only the 30 galaxies considered in Fig. 10 are shown here, for 13 epochs.

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