Table 4.
Best fitting solutions
| Ratios | Side contributions | logΦ(H) | log Ptot | Vturb | Z | log H |  |
 |
f |
| [cm−2 s−1] | [cm−3 K] | [km s−1] | [Z⊙] | [erg cm−3 s−1] | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
| Three | 50-50 | 19.25 | 14 | 40 | 20 | – | – | 3.81 | 0.24 |
| Three | 50-50 | 19.25 | 14 | 30 | 20 | – | 0.10 | 7.15 | 0.25 |
| Three | 20-80 | 19.75 | 15.50 | 100 | 20 | – | – | 1.98 | 0.33 |
| Three | 20-80 | 19.50 | 14.75 | 100 | 20 | – | 0.14 | 4.88 | 0.36 |
| Three | 20-80 | 18.25 | 14.75 | 100 | 1 | −7 | – | 1.44 | 0.08 |
| Three | 50-50 | 18.00 | 14.75 | 100 | 1 | −7 | – | 1.45 | 0.04 |
| All | 50-50 | 19.50 | 15.50 | 40 | 20 | – | – | 11.90 | 0.22 |
| All | 50-50 | 19.50 | 15.50 | 40 | 20 | – | 0.08 | 16.06 | 0.22 |
| All | 20-80 | 20 | 16 | 100 | 20 | – | – | 7.97 | 0.32 |
| All | 20-80 | 20 | 18 | 100 | 20 | – | 0.14 | 10.90 | 0.33 |
Notes. (1) Ratios used in the computation of the best solution with the minimum χ2. (2) Percentage contribution from illuminated and dark sides of the cloud, respectively. (3) Logarithm of the ionizing flux of the central engine associated with the minimum χ2 solution. (4) Logarithm of the total pressure of the cloud associated with the minimum χ2 solution. (5) Microturbulent velocity of the cloud associated with the minimum χ2 solution. (6) Metallicity of the cloud associated with the minimum χ2 solution. Solutions with Z = 50 Z⊙ are not included in the table. (7) Extra mechanical heating applied to the cloud, if present. (8) Best fitting covering factor. This parameter is provided only when equivalent width control was used in the computation of the χ2. (9) Minimum χ2 associated with the best fitting solution. (10) Covering factor necessary to match the whole Fe II emission intensity across the wavelength range of the observed spectrum of RM 102 with the selected CLOUDY simulation.
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