Table 1.
Properties of the ionized outflow in NGC 1365 traced by [Ne V] λ14 μm and [O III] λ5007 Å emission lines.
| Line | Method | Mout | Ṁout | Eout | Ėout |
|---|---|---|---|---|---|
| [104 M⊙] | [10−1 M⊙ yr−1] | [1053 erg] | [1039 erg s−1] | ||
| [Ne V] λ14 μm | standard | 0.26 ± 0.10 | 0.041 ± 0.020 | 0.04 ± 0.02 | 0.20 ± 0.13 |
| HOMERUN | 10.9 ± 0.2 | 1.7 ± 0.2 | 1.6 ± 0.3 | 8 ± 3 | |
| [O III] λ5007 Å | standard | 20 ± 7 | 3.8 ± 0.18 | 4 ± 2 | 26 ± 17 |
| HOMERUN | 8.8 ± 0.9 | 1.7 ± 0.3 | 1.9 ± 0.5 | 12 ± 4 |
Notes. From left to right: Emission line, method used to compute the energetics, outflow mass, mass outflow rate, kinetic energy, and power of the ionized outflow. These values are derived from the spatially resolved outflow properties in the FoV of MIRI Ch3, using the MOKA3D tool (see details in Section 3.6).
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