Table 3.
Multiphase outflows properties
| QSO2 | Data | Emission | rout | vout |
 |
Mout | Ṁout | Ref. |
|---|---|---|---|---|---|---|---|---|
| line | kpc | km s−1 | Myr | 106 M⊙ | M⊙ yr−1 | |||
| J1430 | ALMA | CO(2-1) | 0.5 | −180|250 | 2.5 | 31 | 15.8 | a |
| ALMA | CO(2-1) ( * ) | 1.2 | 300 | 3.9 | 160 | 41.0 | b | |
| GTC/MEGARA | [O III] | 3.7|3.1 | −760|529 | 4.8|5.7 | 5 | 1.1 | c | |
| VLT/SINFONI | H2 | 1.9 | −470|430 | 4.0|4.3 | 2.6 × 10−3 | 6.2 × 10−4 | d | |
| J1356 | ALMA | CO(2-1) | 0.4 | 310 | 1.4 | 14 | 7.8 | a |
| ALMA | CO(2-1) ( * ) | 1.3 | 300 | 4.3 | 129 | 26.2 | b | |
| GTC/MEGARA | [O III] | 12.6|6.8 | −631|483 | 19.5|13.8 | 35 | 2.0 | c | |
| VLT/SINFONI | H2 | 2.0 | 370 | 5.3 | 1.5 × 10−3 | 2.9 × 10−4 | d | |
Notes. The table reports the multiphase outflows properties derived from this work and from literature for J1430 and J1356. Two values are reported when both the blue- and red-shifted sides of the outflows are detected. The [O III] masses are derived using the [S II]-based electron density (SP24) and the corresponding mass outflow rates are divided by 3 to match our outflow geometry. ( * )Outflow properties are computed following Scenario II from Audibert et al. (2023). Column 6 are the dynamical times of the outflows 
.
References: (a) RA22; (b) Audibert et al. (2024); (c) SP24; (d) this work.
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