Table 1.
Parameters describing the ambient medium in starburst galaxies across various cases studied in this paper.
| Cases | External medium profile | Magnetic field structure | Bz [Gauss] | B0 [Gauss] |
|---|---|---|---|---|
| A | Halo and thick disk | – | 0.0 | 0.0 |
| B | Halo and thin disk | – | 0.0 | 0.0 |
| C | Halo | Uniform | 10−5 | 0.0 |
| D | Halo | Uniform | 10−4 | 0.0 |
| E | Halo | Dipole | 0.0 | 10−5 |
| F | Halo | Dipole | 0.0 | 10−4 |
| G | Halo | Dipole | 0.0 | 10−2 |
| H | Halo | Dipole | 0.0 | 1 |
| I | Halo and thick disk | Dipole | 0.0 | 10−4 |
| J | Halo and thin disk | Dipole | 0.0 | 10−4 |
| K | Halo and thick disk | Dipole | 0.0 | 10−2 |
| L | Halo and thin disk | Dipole | 0.0 | 10−2 |
| M | Halo and thick disk | Dipole | 0.0 | 1 |
| N | Halo and thin disk | Dipole | 0.0 | 1 |
| P | Halo and thick disk | Dipole + Uniform Bz | 10−5 | 1 |
| Q | Halo and thin disk | Dipole + Uniform Bz | 10−5 | 1 |
Notes. For each case, the external medium’s density and pressure profile, magnetic field structure, and strength are provided. All cases share the same properties for the galactic wind: a mass-loss rate of Ṁw = 1 M⊙ yr−1, a speed of vw = 2000 km s−1, a Mach number of ℳ = 20, and a duration of t = 10 Myr.
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