Table 6
Properties of the outflows discovered in the five WISSH quasars.
| SDSS | Δv a | v max b |
|
Ṁ | Ė kin | Ė kin / L Bol | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | |
|
|
|||||||
| J0745+4734 | −510±150 | 1890±170 | 6.9 | 5700 | 6.7 | 0.007 | |
| J0900+4215 | −480±160 | 2380±180 | 3.2 | 3300 | 6.3 | 0.008 | |
| J1201+1206 | (I)c | − | 1420±160 | 3.1 | 2500 | 2.8 | 0.005 |
| (II)c | −1060±120 | 1850±180 | 0.9 | 740 | 0.9 | 0.001 | |
| (III)c | −1990±200 | 3270±230 | 1.3 | 1890 | 6.7 | 0.012 | |
| J1326−0005 | −580±100 | 2160±170 | 8.2 | 7740 | 12.0 | 0.031 | |
| J1549+1245 | +330±130 | 1380±220 | 2.9 | 1740 | 1.1 | 0.002 | |
Notes. Columns give the following information: (1) SDSS ID; (2) velocity shift (in units of km s-1); (3) maximum outflow velocity (in units of km s-1); (4) ionised outflowing gas mass (in units of 109M⊙); (5) mass outflow rate (in units of M⊙ yr-1); (6) kinetic power (in units of 1045 erg s-1) of the outflow; and (7) ratio between the kinetic power of the outflow and the bolometric luminosity of the quasar. See Sect. 6.2 for a detailed description of the assumptions made to derive , Ṁ, and Ėkin.
The velocity shift Δv of the broad [OIII] component was derived from the shift in wavelength (− sign indicates a blueshift, + sign indicates a redshift) between broad/shifted and narrow/systemic [OIII] centroids.
Values derived (I) for the broad component centred at 5007 Å (see Sect. 5.1); (II) for the broad blueshifted component centred at λ ~ 4990 Å; (III) for the additional broad blueshifted component centred at λ ~ 4970 Å.
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