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On the evolution of the H i column density distribution in cosmological simulations | Synapse

February 9, 2013Open Access

On the evolution of the H i column density distribution in cosmological simulations

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Resumen

A substantial fraction of the interstellar medium (ISM) in galaxies consists of atomic hydrogen. This makes studying the distribution of neutral hydrogen (HI) and its evolution crucial for our understanding of various aspects of star formation.

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Cite This Study

Rahmati et al. (Sat,) studied this question.

synapsesocial.com/papers/6a0ed4b1950456576347cc02 https://doi.org/https://doi.org/10.1093/mnras/stt066

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