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Table 1.
Kinetic luminosity carried away by the molecular gas wind in ESO 420-G13, compared to different possible launching mechanisms, i.e. AGN radiation, jet power, and star formation.
| Component | Luminosity |
|---|---|
| (erg s−1) | |
| Outflow | 1.1 × 1041 |
| AGN | 0.5–1 × 1044 |
| Jet | 0.001–4 × 1042 |
| Starburst | 7.7 × 1042 |
Notes.
The latter correspond to the knots identified in the ALMA 1.2 mm continuum located close to the outflow wind.
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