Table 7.
Molecular outflow properties for different types of AGN.
| Object | log Lbol | rout | vmax | Ṁout | Mout/Mtot | Refs |
|---|---|---|---|---|---|---|
| (erg s−1) | (kpc) | (km s−1) | (M⊙ yr−1) | |||
| Seyferts | 43.2–44.2 | 0.03–0.5 | 90–200 | 0.3–5 | 0.001–0.01 | 1,2,3 |
| Jetted Seyferts | 44.6–44.9 | 0.1–0.5 | 300–650 | 15–30 | 0.03–0.05 | 4,5 |
| QSO2s | 45.7–46.3 | 0.4–1.3 | 200–350 | 8–16 | 0.002–0.007 | 6 |
| AGN ULIRGs | 44.7–45.7 | 0.5–1.2 | 600–1200 | 60–400 | 0.02–0.27 | 7,8 |
| PDS 456 | 47.0 | 1.2–5 | 1000 | 290 | 0.12 | 9 |
Notes. Lbol corresponds to AGN bolometric luminosity. Outflow gas masses and corresponding rates have been recalculated when necessary assuming αCO = 0.8 M⊙(K km s−1 pc2) −1 and the outflow geometry corresponding to Eq. (1).
References. (1) Alonso-Herrero et al. (2019); (2) Domínguez-Fernández et al. (2020); (3) García-Bernete et al. (2021); (4) García-Burillo et al. (2014); (5) Morganti et al. (2015); (6) This work; (7) Feruglio et al. (2010); (8) Cicone et al. (2014); (9) Bischetti et al. (2019a).
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