$\begin{figure} \par\includegraphics[height=8cm,width=8.4cm,clip]{fig1.eps} \end{figure}$ Figure 1: Mz 3 in the [Ne II] 12.8 micron line with the ISO apertures superposed. The [Ne II] image is the deconvolved map of Smith & Gehrz (2005).
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In the text

$\begin{figure} \par\includegraphics[height=8cm,width=8.4cm,clip]{fig1.eps} \end{figure}$	Figure 1: Mz 3 in the [Ne II] 12.8 micron line with the ISO apertures superposed. The [Ne II] image is the deconvolved map of Smith & Gehrz (2005).
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{fig2.eps} \end{figure}$	Figure 2: The ISO spectrum with 12 and 25 micron IRAS fluxes overplotted as crosses.
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$\begin{figure} \par\includegraphics[width=8.4cm,clip]{fig3.ps} \end{figure}$	Figure 3: $T_{\rm e}$ and $N_{\rm e}$ across the nebula.
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$\begin{figure} \par\includegraphics[width=8.5cm,clip]{fig4.ps} \end{figure}$	Figure 4: Stellar ionizing radiation - Incident (continuous line) and transmitted (broken line).
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