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• W3104769791 startingPage "131" @default.
• W3104769791 abstract "In a thermally bistable medium, cold, dense gas is separated from warm, rarefied gas by thin phase transition layers, or fronts, in which heating, radiative cooling, thermal conduction, and convection of material are balanced. We calculate the steady-state structure of such fronts in the presence of magnetic fields, including the processes of ion–neutral drift and ion–neutral frictional heating. We find that ambipolar diffusion efficiently transports the magnetic field across the fronts, leading to a flat magnetic field strength profile. The thermal profiles of such fronts are not significantly different from those of unmagnetized fronts. The near uniformity of the magnetic field strength across a front is consistent with the flat field strength–gas density relation that is observed in diffuse interstellar gas." @default.
• W3104769791 created "2020-11-23" @default.
• W3104769791 creator A5062425188 @default.
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• W3104769791 date "2010-10-28" @default.
• W3104769791 modified "2023-09-27" @default.
• W3104769791 title "AMBIPOLAR DIFFUSION-MEDIATED THERMAL FRONTS IN THE NEUTRAL INTERSTELLAR MEDIUM" @default.
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• W3104769791 doi "https://doi.org/10.1088/0004-637x/724/1/131" @default.
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