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Paper: On the Structure of the Interstellar Atomic Gas
Volume: 365, SINS — Small Ionized and Neutral Structures in the Diffuse Interstellar Medium
Page: 133
Authors: Hennebelle, P.; Audit, E.
Abstract: The interstellar atomic hydrogen is known to be a 2-phase medium in which turbulence plays an important role. Here we present high resolution numerical simulations describing the gas from tens of parsec down to hundreds of AU. This high resolution allows to probe numerically, the small scale structures which naturally arises from the turbulence and the 2-phase physics.
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