Titlebook: Jets From Young Stars III; Numerical MHD and In S. Massaglia,G. Bodo,P. Rossi Book 2008 Springer-Verlag Berlin Heidelberg 2008 Computationa

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Thermal Instabilitiesrst give a derivation of the instability conditions by using a simple physical analysis and then I will give a more formal derivation. I will finally briefly discuss the effects of cooling-heating processes on the Kelvin-Helmholtz instability.

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Jets From Young Stars III978-3-540-76967-5Series ISSN 0075-8450 Series E-ISSN 1616-6361

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STERN

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The Kelvin–Helmholtz Instabilityntexts: 2-D and 3-D geometries, magnetic fields, relativistic regimes. The formation of shocks and the turbulent mixing are the most important effects of the onset of the KHI that can affect the jets propagation and dynamics on galactic and extragalactic scales.

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