Table 4.
Outflow properties.
| Name | SνΔvCO(2 − 1),out | Mmol, out | fout | Vmol, out | Rmol, out | Ṁmol,out |
|---|---|---|---|---|---|---|
| Jy km s−1 | 107 M⊙ | % | km s−1 | kpc | M⊙ yr−1 | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
| NGC 6860 | 340 ± 6b | 0.06–0.5 | 0.7 | 140 | 0.56 | 0.1–1 |
| Mrk 915a | 184 ± 4c | 0.08–0.7 | 4 | 300 | 2.8 | 0.09–0.7 |
| MCG -01-24-012 | 9220 ± 10d | 3–20 | 30 | 40 | 3 | 0.4–3 |
Notes. (1) Galaxy name; (2) Disturbed/outflowing CO(2-1) flux; (3) Disturbed/outflowing cold molecular gas mass; (4) Fraction of molecular mass that is perturbed: fout = Mmol, out/Mmol, tot; (5) De-projected outflow velocity; (6) De-projected outflow radius; (7) Mass outflow rate. The inclinations used were 57.7°, 66.5° and 74° for NGC 6860, Mrk 915, and MCG -01-24-012, respectively. See Sects. 6.3, 7.2.2 and 8.2, and Appendix E.2, for additional information.
a: Assuming that the spiral arms of Mrk 915 are trailing (see Appendix C).
b: Flux integrated from the c2-component, inside a 0.6″ radius.
c: Flux integrated from the c2-component, inside a 2.3″ radius.
d: Integrated from both components in the double-peak region.
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