Table 5: Ultraviolet (IUE) and optical line fluxes in units of 10-12 erg cm-2 s-1 for BD+30 3639. The optical lines are from Aller & Hyung (1995).
$\lambda$ (nm) Ident. Flux $^{\rm obs}$ Flux $^{\rm corr}$
190.9$^\dagger$ C III] 1.76 21.7
232.6$^\star$ C II 19.7 292.5
372.6 [O II] 98.8 417.3
372.9 [O II] 40.2 169.6
406.9 [S II] 6.04 23.6
407.6 [S II] 1.62 6.31
447.1 He I 0.77 2.73
486.1$^\sharp$ H $_{{\rm\beta }}$ 93.3 293.9
493.3 [O III] 0.06 0.18
495.9 [O III] 2.09 6.39
519.9 [N I] 0.24 0.68
520.1 [N I] 0.18 0.51
551.8 [Cl III] 0.12 0.31
553.8 [Cl III] 0.37 0.97
575.4 [N II] 5.15 12.89
587.6 He I 4.06 9.94
630.0 [O I] 1.88 4.30
631.2 [S III] 1.32 3.01
636.3 [O I] 0.71 1.61
658.3 [N II] 457.0 1002.9
671.6 [S II] 5.18 11.12
673.1 [S II] 11.17 24.0
858.1 [Cl II] 1.01 1.68
912.6 [Cl II] 0.27 0.43
$^\dagger$ From the IUE observations (see Sect. 2.2).
$^\star$ Taken from Torres-Peimbert & Peña (1981).
$^\sharp$ From Acker et al. (1992).


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