Table 2.
Simulations used for post-processing.
| Name | v* | ni | Nzones | Box size | Cell size (Δx) |
|---|---|---|---|---|---|
| 1a | 20 | 50 | 1536 × 1024 | 6.61 × 4.40 pc | 4.303 × 10−3 pc |
| 1b | 20 | 100 | 1536 × 1024 | 4.67 × 3.12 pc | 3.040 × 10−3 pc |
| 1c | 20 | 200 | 1536 × 1024 | 3.30 × 2.20 pc | 2.148 × 10−3 pc |
| 2a | 30 | 50 | 1536 × 1024 | 4.40 × 2.94 pc | 2.864 × 10−3 pc |
| 2b | 30 | 100 | 1536 × 1024 | 3.12 × 2.08 pc | 2.031 × 10−3 pc |
| 2c | 30 | 200 | 1536 × 1024 | 2.20 × 1.47 pc | 1.432 × 10−3 pc |
| 3a | 40 | 50 | 1536 × 1024 | 3.30 × 2.20 pc | 2.148 × 10−3 pc |
| 3b | 40 | 100 | 1536 × 1024 | 2.34 × 1.56 pc | 1.523 × 10−3 pc |
| 3c | 40 | 200 | 1536 × 1024 | 1.65 × 1.10 pc | 1.074 × 10−3 pc |
Notes. Simulations with a “1” in their name have a star velocity of v* = 20 km s−1, “2” have v* = 30 km s−1, and “3” have v* = 40 km s−1. Simulations with an “a” in their name have an ISM ion density of 50 cm−3, “b” have ni = 100 cm−3, and “c” have ni = 200 cm−3. v* is the velocity of the star in km s−1. Nzones shows the number of grid zones in the simulation.
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