Table B.1.
Main physical properties for the QSOs studied in Sect. 5.3, and for their pc-scale and galaxy-scale winds.
AGN properties |
X-ray wind |
Galaxy-scale wind |
||||||
---|---|---|---|---|---|---|---|---|
Parameter | log(LBOL/L⊙) | log(MBH/M⊙) | vUFO | NH, UFO | ṗUFO | Ekin | ṗout | Tracer |
Units | c | (1024 cm−2) | (LBOL/c) | (1056 erg) | (LBOL/c) | |||
IRAS 05189+2524 | 12.22 |
![]() |
0.11 ± 0.01 |
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6.35 ± 1.03 | OH+Na |
I Zw 1 | 12.01 |
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0.26 ± 0.01 | 0.60 ± 0.15 |
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Na |
PDS 456 | 13.61 ± 0.10 | 9.24 ± 0.17 | 0.25 ± 0.01 | 0.69 ± 0.09 |
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CO |
Mrk 231 | 12.60 ± 0.10 | 8.38 ± 0.09 | 0.067 ± 0.008 |
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12.8 |
![]() |
CO,OH |
IRAS F11119+3257 | 12.67 ± 0.10 | 8.29 ± 0.15 | 0.25 ± 0.01 |
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CO,OH |
IRAS 17020+4544 | [11.13, 11.79] | 7.59 ± 0.08 | 0.09 | (a)![]() |
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51.0 |
![]() |
CO |
MCG-03-58-007 | [11.62, 11.95] | 8.34 ± 0.05 | 0.075 ± 0.01 | 0.78 ± 0.32 |
![]() |
0.57 ± 0.03 |
![]() |
CO |
(b)APM 08279+5255 | 14.24 | 10.1 ± 0.4 | 0.18 ± 0.04 |
![]() |
![]() |
179 | 2.82 | CO |
Notes. The UFO mass rates are computed using Eq. (8) with (Ω/4π) in the range [0.1, 0.2], with the exceptions of I Zw 1 and PDS 456, for which covering fractions of 0.5 are directly measured.
The original entry from Longinotti et al. (2015) is , which we interpret as a truncated Gaussian distribution.
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