**Table 4:** Comparison of predicted line fluxes^a with the observed values for AFGL 2591.
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a(b) means $a\times10^b$ .
^a The line fluxes are given in W cm^-2 $\mu$ m^-1, except for the 538.3 $\mu$ m line observed with SWAS, for which the integrated intensity
in K km s^-1 is listed. To convert to W cm^-2, multiply by $\Delta \lambda = \lambda/R$ in $\mu$ m, with $R\approx 9200$ . A negative value indicates absorption.
^b The upper limits are 3 $\sigma$ values.
^c Tentative detection at the 2.5 $\sigma$ level.

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