Table 2: Fluxes derived from Gaussian fits to the fine-structure lines observed with ISO-LWS grating positioned at $\rm 14^h 45^m 21.0^s$ $-59^{\circ } 48' 14''$ (J2000).
Element and Wavelength Flux $\frac{f({\rm line})}{f([{\rm C~II}])}$

ionisation stage ( $\mu$ m) (10^-17 W cm^-2)

[C II] 157.78 1.23 1

[O I] 145.63 0.18 0.15

[N II] 121.84 0.36 0.29

[O III] 88.42 5.77 4.69

[O I] 63.23 0.68 0.55

[N III] 57.26 3.23 2.63

[O III] 51.85 8.29 6.74

**Table 2:** Fluxes derived from Gaussian fits to the fine-structure lines observed with ISO-LWS grating positioned at $\rm 14^h 45^m 21.0^s$ $-59^{\circ } 48' 14''$ (J2000).
Element and	Wavelength	Flux	$\frac{f({\rm line})}{f([{\rm C~II}])}$
ionisation stage	( $\mu$ m)	(10^-17 W cm^-2)
[C II]	157.78	1.23	1
[O I]	145.63	0.18	0.15
[N II]	121.84	0.36	0.29
[O III]	88.42	5.77	4.69
[O I]	63.23	0.68	0.55
[N III]	57.26	3.23	2.63
[O III]	51.85	8.29	6.74

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