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Monthly Notices of the Royal Astronomical Society: Letters
We analyze the evaporation and condensation of spherical and cylindrical HI clouds of the cold neutral medium surrounded by the warm neutral medium. Because the interstellar medium including those two phases is well described as a thermally bistable fluid, it is useful to apply pattern formation theories to the dynamics of the interface between the two phases. Assuming isobaric evolution of fluids and a simple cubic form of the heat-loss function, we show the curvature effects of the interface.doi:10.1111/j.1745-3933.2005.00057.x fatcat:cniwtturwnf4lkpg352oinigdi