Table 5
BLR gas velocities (in km s-1), central black hole masses (in units of 107 M⊙) and apparent Eddington ratios for 13 broad line AGNs belonging to the sample presented in this paper.
| Object | vBLR | MBH | LX/LEdd |
|
|
|||
| IGR J05255−0711 | 3000 | 15 | <4.6 |
| IGR J06523+5334 | 2000 | 3.6 | <3.5 |
| IGR J13466+1921 | 3800 | 4.6 | ~0.05 |
| IGR J14385+8553 | 3000 | 1.7 | <0.15 |
| IGR J16443+0131 | 3700 | 4.3 | <1.4 |
| 1RXS J175252.0−053210 | 3900 | 40 | 0.011 |
| IGR J19491−1035 | 3400 | 3.2 | ~0.005 |
| IGR J20450+7530 | 2700 | 2.4 | <0.32 |
|
|
|||
| IGR J06073−0024 | 5300 | 50 | <3.5 |
| IGR J08262+4051 | 4200 | 15 | <9.3 |
| IGR J12562+2554 | 8400 | 90 | 1.1 |
| IGR J16388+3557 | 23 000 | 270 | 0.15 |
|
|
|||
| IGR J12319−0749 | 5600 | 280 | <2.5 |
Notes. The final uncertainties on the black hole mass estimates are about 50% of their values. The velocities were determined using Hβ, Mg ii, or C iv emissions (upper, central and lower part of the table, respectively), whereas the apparent Eddington ratios were computed using the (observed or rescaled, see text) 20–100 keV luminosities.
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