Table 2: Line emission fluxes for the knots D and F.
    D1 F1 IRS 40+F0

$\lambda$ ($\mu $m)
Ident. $F \pm\Delta F$ (10-15 erg s-1 cm-2)
1.644 [FeII]a4D7/2-a4F9/2     0.8 $\pm$ 0.3a
1.686 (1, 0)S9 0.7 $\pm$ 0.2 - -
1.714 (1, 0)S8 0.5 $\pm$ 0.2a - -
1.748 (1, 0)S7 1.5 $\pm$ 0.1 0.3 $\pm$ 0.1 0.4 $\pm$ 0.1
1.788 (1, 0)S6 1.4 $\pm$ 0.1 0.6 $\pm$ 0.1 -
1.958 (1, 0)S3 38.1 $\pm$ 0.6 4.2 $\pm$ 0.4 5.4 $\pm$ 0.2
2.004 (2, 1)S4 1.4 $\pm$ 0.1 - -
2.034 (1, 0)S2 8.2 $\pm$ 0.2 2.0 $\pm$ 0.3 -
2.073 (2, 1)S3 1.8 $\pm$ 0.2 0.9 $\pm$ 0.3 -
2.122 (1, 0)S1 27.8 $\pm$ 0.2 7.9 $\pm$ 0.1 6.1 $\pm$ 0.2
2.154 (2, 1)S2 1.1 $\pm$ 0.1 - -
2.224 (1, 0)S0 9.4 $\pm$ 0.4 2.1 $\pm$ 0.2 1.7 $\pm$ 0.4
2.247 (2, 1)S1 3.5 $\pm$ 0.4 1.1 $\pm$ 0.2 1.0 $\pm$ 0.2
2.407 (1, 0)Q1 54.2 $\pm$ 0.4 11.8 $\pm$ 0.2 8.2 $\pm$ 0.4
2.414 (1, 0)Q2 20.3 $\pm$ 0.5 3.9 $\pm$ 0.2 4.1 $\pm$ 0.4
2.424 (1, 0)Q3 48.7 $\pm$ 0.5 10.6 $\pm$ 0.2 6.6 $\pm$ 0.4
2.438 (1, 0)Q4 21.4 $\pm$ 0.5 6.6 $\pm$ 0.2 4.5 $\pm$ 0.5
2.455 (1, 0)Q5 11.2 $\pm$ 0.5 12.9 $\pm$ 0.2 6.5 $\pm$ 0.4
2.476 (1, 0)Q6 16.3 $\pm$ 0.6 - 1.8 $\pm$ 0.4
2.501 (1, 0)Q7 29.0 $\pm$ 0.6 - -
$\textstyle \parbox{9cm}{
Note: $^a$\space Signal-to-noise ratio less than three}$.


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