Table 1
Summary of the different runs performed in the paper.
| Label | Physics | Scheme | Feedback | Resolution |
|
|
||||
| NF1 | MHD (2.5 μG) | − | − | 2563 |
| NF2 | hydro | − | − | 2563 |
| A | MHD (2.5 μG) | A | thermal+kinetic | 2563 |
| %hline B | MHD (2.5 μG) | B | thermal+kinetic | 2563 |
| C1 | MHD (2.5 μG) | C | thermal+kinetic | 2563 |
| C1b | MHD (2.5 μG) | C | thermal+kinetic | 5123 |
| C2 | hydro | C | thermal+kinetic | 2563 |
| C3 | MHD (0.5 μG) | C | thermal+kinetic | 2563 |
|
|
||||
| C4 | MHD (2.5 μG) | C | thermal | 2563 |
| D | MHD (2.5 μG) | D | thermal+kinetic | 2563 |
Notes. The scheme refers to the way supernovae are being introduced in the simulations. Schemes A and B assume a constant supernova rates and are not correlated with sink particles. With schemes C and D, the supernovae are correlated spatially and temporally with sink particles (see text).
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