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Fig. 15.

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Lyα escape fraction, f esc Lyα $ {f^\mathrm{Ly\alpha}_\mathrm{esc}} $, vs. intrinsic velocity dispersion σ0. Solid, dashed, and dotted lines indicate the analytically derived approximate solution, our Eq. (12), for monochromatic Lyα radiation escaping a plane parallel slab of NH = 1018 cm−2 (solid lines), 1019 cm−2 (dashed lines), and 1020 cm−2 (dotted line), respectively. For NH = 1018 cm−2 we show curves with E(B − V) = {0.1, 0.4, 0.7}, for NH = 1019 cm−2 curves with E(B − V) = {0.1, 0.4}, and for NH = 1020 cm−2 the curve for E(B − V) = 0.1. We also show the f esc Lyα $ {f^\mathrm{Ly\alpha}_\mathrm{esc}} $ vs. σ 0 obs $ \sigma_0^\mathrm{obs} $ pairings of the discussed sample. Scatter points and curves are colour coded by E(B − V) as indicated by the colour bar on the right. As in Fig. 11 we highlight points by red outlines that show LLyα/LHα ratios above the maximum dust screen expectation from Eq. (6).

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