Fig. 3
Left: VRd/Rd versus SFR surface density ΣSFR. The dashed line shows a linear-fit to the data. The position of the post-starburst dwarf galaxy NGC 6789 is indicated. Right: ΣSFR versus Σgas/τorb, where Σgas considers the atomic gas only and τorb is the orbital time on the solid-body portion of the rotation curve. The dashed lines show a linear relation for different values of ϵ. Symbols are the same as in Fig. 1.
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