Table 3: Observed and modelled forbidden line luminosities. For the observed values, we took the intensities given in Table 4 and assumed a distance of 2 kpc. The fifth column contains the ratio of observed over modelled line luminosity, and in the sixth column we describe in which part(s) of the wind the line is produced. The classifications of p, i, and d mean polar wind, intermediate wind, and disk, respectively. In the upper part we gathered the lines used to derive the mass fluxes and temperature distributions in each wind zone, while the lines in the lower part have been used to confirm the models and to derive the abundance, especially in the case of N.
Ion $\lambda $ (Å) $L_{\lambda}^{\rm obs}$ $L_{\lambda}^{\rm model}$ ratio region
O III 4363 $9.71\times 10^{33}$ $2.90\times 10^{34}$ 0.33 p,i
O III 4959 $3.58\times 10^{34}$ $3.91\times 10^{34}$ 0.92 p,i
O III 5007 $1.13\times 10^{35}$ $1.13\times 10^{35}$ 1.00 p,i
O II 7319 $7.23\times 10^{33}$ $7.70\times 10^{33}$ 0.94 i
O II 7330 $6.18\times 10^{33}$ $6.17\times 10^{33}$ 1.00 i
O I 5577 $1.12\times 10^{32}$ $2.33\times 10^{32}$ 0.48 d
O I 6300 $4.98\times 10^{32}$ $4.86\times 10^{32}$ 1.02 d
O I 6364 $1.49\times 10^{32}$ $1.60\times 10^{32}$ 0.93 d
S III 6312 $2.95\times 10^{33}$ $2.98\times 10^{33}$ 0.99 i
S II 4068 $1.15\times 10^{33}$ $4.57\times 10^{32}$ 2.52 i,d
S II 4076 $3.43\times 10^{32}$ $1.18\times 10^{32}$ 2.90 i,d
S II 6716 $9.05\times 10^{31}$ $1.05\times 10^{32}$ 0.86 i,d
S II 6731 $2.13\times 10^{32}$ $2.20\times 10^{32}$ 0.97 i,d
N II 5755 $4.56\times 10^{33}$ $4.57\times 10^{33}$ 1.00 i
N II 6548 $4.84\times 10^{33}$ $6.15\times 10^{33}$ 0.79 i
N II 6584 $2.08\times 10^{34}$ $1.81\times 10^{34}$ 1.15 i
Cl III 5517 $1.10\times 10^{32}$ $4.23\times 10^{31}$ 2.60 p,i
Cl III 5538 $1.74\times 10^{32}$ $1.74\times 10^{32}$ 1.00 p,i
Cl II 6153 $3.88\times 10^{31}$ $3.82\times 10^{31}$ 1.01 i
Ar III 5193 $1.16\times 10^{32}$ $6.44\times 10^{32}$ 0.18 p,i
Ar III 7136 $7.37\times 10^{33}$ $6.88\times 10^{33}$ 1.07 p,i
Ar III 7753 $1.49\times 10^{33}$ $1.68\times 10^{33}$ 0.89 p,i


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