Table 1
Axisymmetric simulations that model the H ii region and wind bubble simultaneously.
| ID | v ∗ | Nz × Nr | ([ z ] × [ R ]) | τc (Myr) | Tmin (K) |
|
|
|||||
| V04 | 4 | 1280 × 512 | 5.0 × 2.0 | 1.22 | 300 |
| V06 | 6 | 1280 × 512 | 3.75 × 1.5 | 0.611 | 500 |
| V08 | 8 | 1280 × 512 | 2.5 × 1.0 | 0.306 | 500 |
| V16 | 16 | 640 × 256 | 1.25 × 0.5 | 0.076 | 500 |
Notes. All simulations use the same wind properites and ionizing photon luminosity; see text for details. v⋆ is the stellar space velocity in km s-1; Nz and Nr are the number of grid zones in the ẑ and 
directions, respectively; [ z ] and [ R ] are the simulation domain sizes in pc; τc is the time it takes for the star to cross the simulation domain (most relevant timescales are substantially shorter than this); and Tmin is the minimum temperature (in K) allowed in each simulation.
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