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Table 5

Model parameters and line predictions.

Quantity Model

CHII + CPDR Dl Dh Warm dust Totala

Energy source Starburst 3.7 Myr Star 35 000 K Star 35 000 K Starburst 3.7 Myr
nH [cm-3] 102.8 105.1 (103.4) 101.0 103.0 101.5
rin [cm] 1021.4 1021.4 1021.8 1021.8 1019.8

I([S iv] 10.5)/Iobsb 0.84 (0.29) 0.84
I([Ne ii] 12.8)/Iobs 0.20 (0.10) 0.53 0.89 0.73
I([Ne iii] 15.6)/Iobs 1.13 (0.61) 1.13
I([S iii] 18.7)/Iobs 1.03 (0.50) 0.26 0.16 1.29
I([S iii] 33.5)/Iobs 1.04 (0.63) 0.61 0.14 1.65
I([Si ii] 34.8)/Iobs 0.11 (0.07) 0.24 (0.37) 0.04 0.24 0.39
I(Hu α 12.4)/Iobs 1.28 (0.61) 0.37 0.63 1.65
I([Fe iii] 22.9)/Iobs 0.49 (0.27) 0.44 0.50 0.93
I([O iv] 25.9)/Iobs 1.18 (0.74) 0.10 1.28
I([Ar iii] 8.99)/Iobs 1.49 (0.51) 0.08 0.06 1.57
I([Ar ii] 6.99)/Iobs 0.12 (0.08) 0.75 1.49 0.87
I([C ii] 157)/Iobs 0.01 (0.01) 0.07 (0.49) 0.40 0.19 0.48
I([O iii] 88)/Iobs 0.59 (0.44) 0.02 0.61
I([O i] 63)/Iobs 0.03 (0.02) 1.11 (1.03) 0.08 1.14
I([O i] 145)/Iobs 0.03 (0.02) 0.95 (1.00) 0.07 0.98
I([N iii] 57)/Iobs 1.41 (0.99) 0.13 1.44
I([N ii] 122)/Iobs 0.29 (0.23) 1.46 0.46 1.75

Notes. 

(a)

The total is taken as the sum of models C, Dl and warm dust, which is what we consider for the final build-up in Sect. 7; although Dh and CB may also alter the line predictions.

(b)

Ratio of the predicted intensity of the model over the observed intensity (Iobs). Ratio values below 1% are not indicated.

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