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Magnetic Reconnection and Extraplanar Diffuse Ionized Gas
Authors:Guido T Birk  Harald Lesch  Thomas Neukirch
Institution:1. Institute for Astronomy and Astrophysics, University of Munich, Germany
3. School of Mathematics and Statistics, University of St. Andrews, Scotland, UK
2. Centre of Interdisciplinary Plasma Science, Garching, Germany
Abstract:Photoionization by stars cannot be the only cause for the diffuseionized gas component in the distant halos of galaxies.Quasistationary localized magnetic reconnection can efficientlycontribute to the ionization of the extraplanar halo gas. The gas isheated and re-ionized in numerous current filaments fast enough tocompensate recombination. The necessary magnetic energy is provided bythe disk activity.
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