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Fig. 3.

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Escape fraction traced by FλLyC/Fλ1100 (left), (middle), and (right) vs. intrinsic velocity dispersion of the Hα broad component (top) and line asymmetry of [O III] 5007 (bottom). The dotted lines (A = 0) indicate a symmetric Gaussian profile. The stars identify the five galaxies from Izotov et al. (2016b, 2018a).

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