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Fig. 6

image

Observed Lyα spectra of LyC leakers from our Lyα criteria. Top: HST/COS Lyα profile of the known LyC leaking galaxy Haro 11 Bergvall et al. (2006), with a narrow P Cygni profile with vpeak ≤ 150 km s-1, typical of Lyα transfer through low optical depth medium. Bottom: GHRS Lyα spectrum of a low-metallicity blue compact dwarf galaxy Tol 1214277, highly suggestive of Lyman-continuum leakage from a riddled ISM (Sect. 2.3). The systemic redshifts and their errors (grey shaded area in each plot) were adopted from the 6dF survey for Haro 11 and from Pustilnik & Martin (2007) for Tol 1214277. The blue horizontal line denotes the continuum level.

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