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- W2059897458 abstract "We investigate the column density distribution function of neutral hydrogen at redshift z = 3 using a cosmological simulation of galaxy formation from the OverWhelmingly Large Simulations project. The base simulation includes gravity, hydrodynamics, star formation, supernovae feedback, stellar winds, chemodynamics, and element-by-element cooling in the presence of a uniform UV background. Self-shielding and formation of molecular hydrogen are treated in post-processing, without introducing any free parameters, using an accurate reverse ray-tracing algorithm and an empirical relation between gas pressure and molecular mass fraction. The simulation reproduces the observed z = 3 abundance of Lyα forest, Lyman limit, and damped Lyα H i absorption systems probed by quasar sight lines over 10 orders of magnitude in column density. Self-shielding flattens the column density distribution for NH i > 1018 cm−2, while the transition to fully neutral gas and conversion of H i to H2 steepen it around column densities of NH i = 1020.3 cm−2 and NH i = 1021.5 cm−2, respectively." @default.
- W2059897458 created "2016-06-24" @default.
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- W2059897458 date "2011-08-02" @default.
- W2059897458 modified "2023-09-25" @default.
- W2059897458 title "THROUGH THICK AND THIN—H I ABSORPTION IN COSMOLOGICAL SIMULATIONS" @default.
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- W2059897458 doi "https://doi.org/10.1088/2041-8205/737/2/l37" @default.
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