Abstract

Lyman-alpha line profiles are a powerful probe of ISM structure, outflow speed, and Lyman continuum escape fraction. In this paper, we present the Lyα\alpha line profiles of the COS Legacy Archive Spectroscopic SurveY, a sample rich in spectroscopic analogs of reionization-era galaxies. A large fraction of the spectra show a complex profile, consisting of a double-peaked Lyα\alpha emission profile in the bottom of a damped, Lyα\alpha absorption trough. Such profiles reveal an inhomogeneous interstellar medium (ISM). We successfully fit the damped Lyα\alpha absorption (DLA) and the Lyα\alpha emission profiles separately, but with complementary covering factors, a surprising result because this approach requires no Lyα\alpha exchange between high-NHIN_\mathrm{HI} and low-NHIN_\mathrm{HI} paths. The combined distribution of column densities is qualitatively similar to the bimodal distributions observed in numerical simulations. We find an inverse relation between Lyα\alpha peak separation and the [O III]/[O II] flux ratio, confirming that the covering fraction of Lyman-continuum-thin sightlines increases as the Lyα\alpha peak separation decreases. We combine measurements of Lyα\alpha peak separation and Lyα\alpha red peak asymmetry in a diagnostic diagram which identifies six Lyman continuum leakers in the CLASSY sample. We find a strong correlation between the Lyα\alpha trough velocity and the outflow velocity measured from interstellar absorption lines. We argue that greater vignetting of the blueshifted Lyα\alpha peak, relative to the redshifted peak, is the source of the well-known discrepancy between shell-model parameters and directly measured outflow properties. The CLASSY sample illustrates how scattering of Lyα\alpha photons outside the spectroscopic aperture reshapes Lyα\alpha profiles as the distances to these compact starbursts span a large range.Comment: 40 pages, 19 figures, 5 tables, submitted to ApJ, comments welcom

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