The role of turbulence in the warm ionized medium

Published 16 Jul 2010 in astro-ph.GA | (1007.2767v1)

Abstract: We discuss the role of turbulence in establishing the observed emission measures and ionization of the warm ionized medium. A Monte Carlo radiative transfer code applied to a snapshot of a simulation of a supernova-driven, multi-temperature, stratified ISM reproduces the essential observed features of the WIM.

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