Abstract
Almost all models of interstellar dynamics have been of a hydrodynamic nature. However, the magnetic and cosmic ray pressures are comparable to the thermal pressure throughout a sizable fraction of the volume of the interstellar medium (e.g. Ferrière 1998).
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Hartquist, T., Wagner, A., Falle, S. (2007). The Effects of Cosmic Rays on Interstellar Dynamics. In: HARTQUIST, T., PITTARD, J., FALLE, S. (eds) Diffuse Matter from Star Forming Regions to Active Galaxies. Astrophysics and Space Science Proceedings. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-5425-9_14
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