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Fig. 12


Time evolution of the mass fraction in the CNM, WNM and thermally unstable gas (top), the mean Mach number obs (middle), and the mean velocity dispersion σturb (bottom) for a decaying simulation with the following initial conditions: n0 = 1 cm-3, ζ = 1.0, vS = 7.0 km s-1. The turbulent driving was applied at first and shut down after 40 Myear.

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