Fig. 3.

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Intrinsic and pressure-support-corrected rotation-to-dispersion ratio (V/σ), plotted on the y- and x-axes, respectively. The solid black line represents the one-to-one relation between the two quantities. The vertical and horizontal dashed lines indicate the V/σ > 1 limit for intrinsic and pressure-support-corrected rotation-to-dispersion ratios, respectively. This figure indicates that, after pressure support corrections, none of the GS23 galaxies exhibit dispersion-dominated characteristics. Therefore, we utilize the entire GS23 sample for the TFR study.
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