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Thermal stability of a weakly magnetized rotating plasma

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arxiv 1206.3890 v2 pith:6DLKPH3E submitted 2012-06-18 astro-ph.GA physics.plasm-ph

classification astro-ph.GAphysics.plasm-ph
keywords stabilitymagnetizedplasmarotatingthermalweaklyanalysisatmospheres
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The thermal stability of a weakly magnetized, rotating, stratified, optically thin plasma is studied by means of linear-perturbation analysis. We derive dispersion relations and criteria for stability against axisymmetric perturbations that generalize previous results on either non-rotating or unmagnetized fluids. The implications for the hot atmospheres of galaxies and galaxy clusters are discussed.

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