Disparate effects of circumgalactic medium angular momentum in IllustrisTNG and SIMBA

Open Access

Fig. A.1.

Same to Figs. 2 and 6, but also including the results for TNG100-2 and TNG50. Overall, the trends in TNG100-2 and TNG50 are very similar to that in TNG100, with weak dependence on resolution. The quenched galaxies in TNG100-2 and TNG50 still show a higher λ_CGM than their star-forming counterparts.

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