Table 1
Parameters used for the 16 spherically symmetric radiation-hydrodynamics simulations.
| ID | v∞ (km s-1) | Ṁ (M⊙ yr-1) | Fγ (cm-2 s-1) | |
|
|
||||
| M5V15W | 15 | 2 × 10-5 | 7.87 × 1010 | |
| M5V20W | 20 | 2 × 10-5 | 1.29 × 1011 | |
| M5V25W | 25 | 2 × 10-5 | 8.29 × 1010 | |
| M5V30W | 30 | 2 × 10-5 | 5.83 × 1010 | |
|
|
||||
| M4V15W | 15 | 1 × 10-4 | 1.70 × 1012 | |
| M4V20W | 20 | 1 × 10-4 | 2.34 × 1012 | |
| M4V25W | 25 | 1 × 10-4 | 1.44 × 1012 | |
| M4V30W | 30 | 1 × 10-4 | 9.95 × 1011 | |
|
|
||||
| M5V15E | 15 | 2 × 10-5 | 1.70 × 1010 | |
| M5V20E | 20 | 2 × 10-5 | 2.78 × 1010 | |
| M5V25E | 25 | 2 × 10-5 | 1.79 × 1010 | |
| M5V30E | 30 | 2 × 10-5 | 1.26 × 1010 | |
|
|
||||
| M4V15E | 15 | 1 × 10-4 | 3.67 × 1011 | |
| M4V20E | 20 | 1 × 10-4 | 5.05 × 1011 | |
| M4V25E | 25 | 1 × 10-4 | 3.10 × 1011 | |
| M4V30E | 30 | 1 × 10-4 | 2.15 × 1011 | |
Notes. In the identifier (ID), M5/M4 refer to the mass-loss rates, V15/V20/V25/V30 refers to the wind velocity, and W/E denote WNW side or ESE side of W26 (i.e. when the ionization front is closer to or further from W26). The ionizing fluxes have been set to give ionization fronts that match the observations as closely as possible in terms of Hα brightness as a function of distance from the star.
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