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| Paper: |
Line-Driven Disk Wind Model for BALQSOs |
| Volume: |
460, AGN Winds in Charleston |
| Page: |
224 |
| Authors: |
Nomura, M.; Ohsuga, K.; Wada, K.; Susa, H.; Misawa, T. |
| Abstract: |
We investigate the conditions for which the line-driven disk wind model
reproduces broad absorption line (BAL) features. We research the
structure of the disk wind using non-hydrodynamic calculations for a
wide range of the parameters. We compare the resulting wind structure
with the wind properties of X-ray observations of BAL quasars. We
find that the probability that the BAL is observed is large for large
black hole mass and large Eddington ratio. When the density of gas at
the wind-base is the same as that of the broad emission-line region
(BELR), the disk wind model can reproduce BAL features. Our results
support the new hypothesis that the wind-base is the BELR. |
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