Table 6
BLR gas velocities (in km s-1), central black hole masses (in units of 108M⊙), and apparent Eddington ratios for the 14 broad line AGNs discussed in this paper.
| Object | v BLR | M BH | LX/LEdd |
|
|
|||
| IGR J02447+7046 | 4000 | 1.4 | 0.2 |
| IGR J02574−0303 | 3900 | 0.42 | ~0.5 |
| IGR J06293−1359 | 5700 | 0.87 | <1.6 |
| IGR J14488−4008 | 5300 | 3.8 | <0.007 |
| IGR J17476−2253 | 11 100 | 3.6 | 0.002 |
| IGR J17488−2338 | 8200 | 13 | <0.006 |
| 2E 1923.7+5037 | 9700 | 5.8 | ~0.002 |
| IGR J21565+5948 | 5700 | 5.6 | 0.02 |
|
|
|||
| IGR J02115−4407 | 6100 | 8.9 | <3.3 |
| IGR J03564+6242 | 11 300 | 63 | 0.2 |
| IGR J09034+5329 | 11 000 | 20 | <1.8 |
| IGR J21319+3619 | 10 700 | 19 | <0.6 |
| IGR J23558−1047 | 8200 | 11 | 3.5 |
|
|
|||
| IGR J16388+3557 | 23000 | 160 | 0.4 |
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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