Table 5
Outflow properties derived from the line fits and the formulas mentioned in Sect. 6.
| Object ID | f[O iii] | log(L[O iii]) |
|
|
|
P SFR | |||
| (10-16 erg/s/cm-2) | (erg/s) | (107M⊙) | (M⊙/yr) | (1041 erg/s) | (1043 erg/s) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | |||
|
|
|||||||||
| 178 | 2.33 ± 0.16 | 42.35 ± 0.02 | 1.13 | 2.00–2.96 | 1.53–4.98 | 9.4 | |||
| 5330* | 1.29 ± 0.04 | 42.68 ± 0.01 | – | – | – | 7.0 | |||
| 5627 | 1.65 ± 0.15 | 42.27 ± 0.02 | 0.94 | 0.83–1.74 | 0.16–1.46 | 11.0 | |||
| 54204 | 1.54 ± 0.84 | 42.26 ± 0.05 | 0.91 | 3.91–7.63 | 11.44–84.95 | 30.7 | |||
| 2028† | 2.64 ± 0.09 | 42.66 ± 0.01 | 2.32 | 8.24 | 58.44 | 17.5 | |||
Notes. Column (1) the X-ray ID of the sample; (2) flux of the broad Gaussian component in the [O iii] λ5007 profile; (3) luminosity corresponding to the flux in (2); (4) outflow mass traced by the [O iii] λ5007 line; (5) and (6) range of mass outflow rates and the kinetic energy associated with the ionized component corresponding to the velocity values in Table 3, keeping the rest of the assumptions constant; (7) power due to the star formation in the host galaxy.
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