Table 2: Infrared line intensities for BD+30 3639. All fluxes are in units of 10-12 erg cm-2 s-1. In the last column the unreddened flux is given using EB-V=0.34.
$\lambda (\mu$m) Ident. Flux $^{\rm obs}$ Flux $^{\rm corr}$
2.625 H I Br$\beta$ 13.30 14.01
2.872 H I 5-11 1.30: 1.36:
3.039 H I 5-10 1.71 1.78
3.740 H I Pf$\gamma$ 3.33 3.42
4.051 H I Br$\alpha$ 25.1 25.7
6.984 [Ar II] 139.0 140.5
7.458 H I Pf$\alpha$ 7.69 7.77
8.991 [Ar III] 6.10 6.40
10.51 [S IV] <1.77 <1.86
11.76 [Cl IV] <1.67 <1.72
12.81 [Ne II] 29 8.9 30 4.9
15.55 [Ne III] <2.42 <2.46
18.70 [S III] 60.4 61.7
33.48 [S III] 12.18 12.28
57.30$^\dagger$ [N III] <3.20 <3.21
122.0$^\dagger$ [N II] 1.08: 1.08:
$^\dagger$ From the LWS spectrum.
: Noisy.

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