Table 1.
Parameters for the models used in this study as well as the injected power obtained by matching the calculated flux with the observed one.
| Model | L (kpc) | D0 (kpc2 Myr−1) | δ | Vwind (km s−1) | vA(km s−1) | α | 𝒫inj |
|---|---|---|---|---|---|---|---|
| MIN2.4 | 1.0 | 0.0016 | 0.85 | 13.5 | 22.4 | 2.4 | 2.9 × 1045 |
| MED2.2 | 4.0 | 0.012 | 0.7 | 12.0 | 52.9 | 2.2 | 3.2 × 1041 |
| MED2.3 | 2.3 | 4.3 × 1041 | |||||
| MED2.4 | 2.4 | 6.5 × 1041 | |||||
| MAX2.2 | 15.0 | 0.0765 | 0.46 | 5.0 | 117.6 | 2.2 | 6.9 × 1040 |
| MAX2.3 | 2.3 | 9.2 × 1040 | |||||
| MAX2.4 | 2.4 | 1.4 × 1041 | |||||
| *Kr2.4 | 10 | 0.09 | 0.5 | 10.0 | 28.0 | 2.4 | 2.8 × 1041 |
| *Kol2.55 | 10 | 0.23 | 1/3 | 12.0 | 30.0 | 2.55 | 6 × 1041 |
Notes. The number appearing in the name of the model corresponds to the value of the logarithmic exponent α in the source term. (*)Models with a star are described in Sect. 4.2 and reproduce the observed primary fluxes.
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