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Cold accretion flows and the nature of high column density H i absorption at redshift 3

Monthly Notices of the Royal Astronomical Society, no. 4 (2012): 2809-2819

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Simulations predict that galaxies grow primarily through the accretion of gas that has not gone through an accretion shock near the virial radius and that this cold gas flows towards the central galaxy along dense filaments and streams. There is, however, little observational evidence for the existence of these cold flows. We use a large,...更多

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