\begin{table}%t4
\caption{\label{model_line}Emergent line luminosities predicted by the model for \object{IRAS~14416-5937} -- A.}
\small%\centering
\par
\begin{tabular}{c r r r} 
\hline \hline\noalign{\smallskip}
Element and & Wavelength & Luminosity & $\frac{L({\rm line})}{L([{\rm C~II}])}$\\
ionisation stage & ($\mu$m) & ($L_{\odot}$) & \\
 \hline
$[$C II$]$ & 157.78 & 17.91 & 1\\
$[$O I$]$  & 145.63 & 0.17  & 0.01\\
$[$N II$]$ & 121.84 & 1.57 & 0.09\\
$[$O III$]$ & 88.42 & 121.40 & 6.78\\
$[$O I$]$ & 63.23 & 2.64 & 0.15\\
$[$N III$]$ & 57.26 & 57.70 & 3.22\\
$[$O III$]$ & 51.85 & 271.54 & 15.16\\
$[$Ne III$]$ & 36.04 & 8.20 & 0.46\\
$[$Si II$]$ & 34.84 & 6.23 & 0.35\\
$[$S III$]$ & 33.50 & 116.71 & 6.52\\
$[$O IV$]$ & 25.91 & 1.12 & 0.06\\
$[$Ar III$]$ & 21.84 & 2.79 & 0.16\\
$[$S III$]$ & 18.69 & 111.75 & 6.24\\
$[$Ne III$]$ & 15.57 & 88.77 & 4.96\\
$[$Ne II$]$ & 12.82 & 23.81 & 1.33\\
$[$S IV$]$ & 10.52 & 50.65 & 2.83\\
$[$Ar III$]$ & 8.99 & 35.51 & 1.98\\
$[$Ar II$]$ & 7.00 & 2.23 & 0.12\\ \hline 
\end{tabular}
\end{table}