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Fig. 3.

image

Relation between optical radius R25 and stellar mass Msp. Panel a: R25 as a function of Msp for individual galaxies with R distribution (blue circles) and B distribution (red squares) of the gas velocity dispersion. Panel b: median values of R25 for galaxies in bins of 0.3 dex in Msp for galaxies with R distribution, shown with blue circles. The solid line is the linear best fit to those data. Red squares denote the binned median values for galaxies with B distribution. The dashed line is the linear best fit to those data.

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