Table 3.
Positions, fluxes and masses of the galaxies and outflows.
| Tracer | Mass | v | Radius | dM/dt | c × v × dM/dt | 1/2 × v2dM/dt | Reference |
|---|---|---|---|---|---|---|---|
| (M⊙) | (km s−1) | (kpc) | (M⊙ yr−1) | 1012 × L⊙ | 1043 (erg s−1) | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| Hα | 8.5 × 106 | 1524 | ≤2 | 7.6 | 0.69 | 1.3 | (a) |
| Na I D | 7.6 × 107 | 403 | ≤2 | 24.5 | 0.89 | 0.63 | (a) |
| OH | 1.2 × 108 | 500−950 | 0.11 | 650 | 22 | 10 | (b) |
| H2 | 5.2 × 104 | 1000 | 0.4 | 0.13 | 0.006 | 0.004 | (c) |
| [CII] | 1.4 × 108 | 800 | ... | ... | ... | ... | (d) |
| CO(1-0)CD | 4.1 × 108 | 800 | 0.82 | 1210 | 47.8 | 24.5 | (e) |
| CO(1-0)ABCD | 2.7 × 108 | 1200 | 0.95 | 350 | 21 | 16 | This work |
Notes. Outflow properties of different ISM phases. As a comparison, the SFR is 69 M⊙/year (González-Alfonso et al. 2017). Columns: (1) tracer, (2) total gas mass in the outflow, (3) average or typical outflow velocity, (4) radius in kpc, (5) Outflow mass loss rate, (6) outflow momentum rate, (7) kinetic power in the outflow. The differences between the newest CO observations (CO(1-0)ABCD) and those presented earlier (CO(1-0)CD) are mostly caused by new insights in the outflow geometry. See Sects. 4.2 and 5.1 for details.
References. (a) Rupke & Veilleux (2013a), (b) González-Alfonso et al. (2017), (c) Rupke & Veilleux (2013b), (d) Janssen et al. (2016), (e) Cicone et al. (2014).
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