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Breaking the sound barrier in recombination fronts

We exploit a generic instability in the integration of steady, sonic, near-isothermal flows to find the complete transition diagram for recombination fronts (for a model system of equations). The instability requires the integration of the flow equations for speeds between the isothermal and adiabatic sound speeds to be performed with particular care. As a result of this, the previous work of Newman & Axford on the structure of recombination fronts neglected an important class of solution, that of transonic fronts; our method is readily extensible to a more complete treatment of the ionization structure. Future papers will apply these results in models of the structure of ultracompact HII regions.

preprint1995arXivOpen access
R. J. R. WilliamsJ. E. Dyson
astro-ph
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Open access2 authors1 topic
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R. J. R. WilliamsJ. E. Dyson

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