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Table 1
Mean emission radius ρm/rin of the three BLR models for some representative values of the inclination of the line of sight, considering a rapidly decreasing emissivity ϵ(r) = ϵ0 (rin/r)3.
| i = | 22° | 34° | 44° | 62° | |
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| Keplerian disk | 2.47 | 2.35 | 2.23 | 1.96 | |
| Polar wind | 3.06 | 3.01 | 2.98 | 3.04 | |
| Equatorial wind | 3.73 | 3.54 | 3.37 | 2.97 | |
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