Fig. 10
Size distribution of the galaxies and star-forming knots from the isophotal analysis of the HST high spatial resolution F814W images. Circular symmetry is assumed to estimate the radius. Panel a), the distribution of both the total sample and Sknot galaxies is shown in light gray and gray, respectively. Panel b), the distribution of knots in Mknot galaxies, Sknot+diffuse galaxies, and Sknot galaxies is shown in light gray, gray, and empty histogram.
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