Magnetic ionization fronts II: Jump conditions for oblique magnetization
arXiv:astro-ph/0001116 · doi:10.1046/j.1365-8711.2000.03296.x
Abstract
We present the jump conditions for ionization fronts with oblique magnetic fields. The standard nomenclature of R- and D-type fronts can still be applied, but in the case of oblique magnetization there are fronts of each type about each of the fast- and slow-mode speeds. As an ionization front slows, it will drive first a fast- and then a slow-mode shock into the surrounding medium. Even for rather weak upstream magnetic fields, the effect of magnetization on ionization front evolution can be important. [Includes numerical MHD models and an application to observations of S106.]
9 pages, 10 figures, Latex, to be published in MNRAS
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Cited by in corpus (15)
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