Table 2
Different combinations of the ionizing photons flux emitted by the primary source (Φ(H)) and electronic density in the BLR clouds (Ne), used as input for Cloudy Fe ii simulated templates for different physical condition of the BLR.
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8 | 10 | 10 | 12 | 12 | 12 | 14 | 14 | 14 | 14 |
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17 | 17 | 19 | 17 | 19 | 21 | 17 | 19 | 21 | 23 |
Notes. The two parameters define the space of possible values for the ionization parameter U, describing the physical condition in the ionized region. For every combination we considered the case a microturbulence velocity uturb = 100 km s-1 is present. The result is a set of 20 templates for the Fe ii emissions.
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