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 H II regions.
CITATION STYLE
Williams, R. J. R., & Dyson, J. E. (1996). Breaking the sound barrier in recombination fronts. Monthly Notices of the Royal Astronomical Society, 279(3), 987–992. https://doi.org/10.1093/mnras/279.3.987
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