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Clumpy ultracompact HII regions -- II. Cores, spheres and shells from subsonic flows

M. P. Redman·R. J. R. Williams·J. E. Dyson
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Abstract

We have modelled ultracompact HII regions (UCHIIR) in terms of steady subsonic ionized flows in a clumpy medium. Mass loss from neutral clumps allows the regions to be long-lived. We examine the form of global flows for different dependences of the volume mass injection rate, $\dot{q}$, on radius and Mach number, and describe the solutions in detail. We find that three observed UCHIIR morphologies are reproduced with these models. Mach number independent flows that include a radial variation can give centre- brightened core--halo morphologies. Mach number dependent flows reproduce naturally the uniform UCHIIR morphology. In a hybrid model, including subsonic and supersonic flows, we allow a supersonic wind to shock in the ionized region. The ionized subsonic gas has a high density and so dominates the emission. The shell produced has a velocity structure very different from that of fully supersonic models. Several morphologies of spherical UCHIIR can be understood in terms of these various models; however, kinematic data are crucial as a discriminant between them.

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M. P. Redman, R. J. R. Williams, J. E. Dyson. 1996-03-01. Clumpy ultracompact HII regions -- II. Cores, spheres and shells from subsonic flows. https://doi.org/10.1093/mnras%2F280.3.661

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