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Table 5
Comparison between our model and the Bennert et al. (2006) nuclear optical spectrum.
| Line ratios to Hβ | Obs. | Calc. | ||
|
|
||||
| [O II] 3727+ | 2.63 | 3.1 | ||
| [Ne III] 3869+ | 1.7 | 1.3 | ||
| [O III] 4363 | 0.23 | 0.1 | ||
| He II 4686 | 0.24 | 0.2 | ||
| [O III] 5007+ | 12.06 | 12.02 | ||
| [Fe VII] 6087 | 0.04 | 0.02 | ||
| [O I] 6300 | 0.56 | 0.7 | ||
| [Fe X] 6375 | 0.03 | 0.001 | ||
| Hα | 2.87 | 2.9 | ||
| [N II] 6583 | 1.99 | 2.9 | ||
| [S II] 6716 | 0.56 | 0.3 | ||
| [S II] 6731 | 0.63 | 0.45 | ||
|
|
||||
| n0 (cm-3) | – | 190 | ||
| Vs (km s-1) | – | 370 | ||
| B0 (Gauss) | – | 10-4 | ||
| log F1 | – | 10.85 | ||
| D (cm) | – | 2 × 1017 | ||
| Hβ (erg cm-2 s-1) | – | 0.23 | ||
| n (cm-3) | – | 6330 | ||
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