Table 4: Emergent line luminosities predicted by the model for IRAS 14416-5937 - A.

Element and
Wavelength Luminosity $\frac{L({\rm line})}{L([{\rm C~II}])}$
ionisation stage ($\mu $m) ($L_\odot$)  
[C II] 157.78 17.91 1
[O I] 145.63 0.17 0.01
[N II] 121.84 1.57 0.09
[O III] 88.42 121.40 6.78
[O I] 63.23 2.64 0.15
[N III] 57.26 57.70 3.22
[O III] 51.85 271.54 15.16
[Ne III] 36.04 8.20 0.46
[Si II] 34.84 6.23 0.35
[S III] 33.50 116.71 6.52
[O IV] 25.91 1.12 0.06
[Ar III] 21.84 2.79 0.16
[S III] 18.69 111.75 6.24
[Ne III] 15.57 88.77 4.96
[Ne II] 12.82 23.81 1.33
[S IV] 10.52 50.65 2.83
[Ar III] 8.99 35.51 1.98
[Ar II] 7.00 2.23 0.12


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