Relation between the gaseous disk thickness and the gas velocity dispersion for the unbarred galaxy simulation (RA) and the barred galaxy model (RB). This relation is shown for values within the inner 5 kpc of the disk and at 1.2 Gyr in each simulation (left and center panels). Right panel: the distribution functions of the thickness of the gaseous disk for the two models shown in the left and center panels.
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