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Table 6
Comparison between our model and the Ramos Almeida et al. (2009) IR spectrum.
| Line ratios to [S iii] 0.9 | Obs. | Calc. | ||
|
|
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| [C I] 0.98 | 0.02 | 0.02 | ||
| [S VIII]0.99 | 0.012 | 0.01 | ||
| [S II] 1.03 | 0.054 | 0.045 | ||
| He I 1.08 | 0.35 | 0.36 | ||
| [S IX] 1.25 | 0.0057 | 0.06 | ||
| [S IX] 1.43 | 0.011 | 0.012 | ||
| Pα 1.96 | 0.158 | 0.2 | ||
| [S XI] 1.9 | 0.003 | 0.01 | ||
| [Si VI] 1.96 | 0.028 | 0.045 | ||
|
|
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| n0 (cm-3) | – | 200 | ||
| Vs (km s-1) | – | 500 | ||
| B0 (Gauss) | – | 10-4 | ||
| log F1 | – | 10. | ||
| D (cm) | – | 3 × 1015 | ||
| Hβ (erg cm-2 s-1) | – | 6.3 × 10-3 | ||
| Hβ/[S III] | – | 1.96 | ||
| n (cm-3) | – | 1300 | ||
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