Abstract
We have modelled ultracompact H II 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, 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.
Original language | English |
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Pages (from-to) | 651-660 |
Number of pages | 10 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 280 |
Issue number | 2 |
Publication status | Published - 1996 |
Externally published | Yes |
Keywords
- H II regions
- Hydrodynamics
- ISM: Structure
- Radio lines: ISM
- Shock waves
- Stars: Mass-loss