$\begin{figure} \par\includegraphics[width=8.4cm,clip]{fig1.epsi}\par\end{figure}$ Figure 1: HST image of the planetary nebula NGC 6886 as observed through the [O III] and [N II] filters, where the overall morphology is clearly visible. North is up and East is left.
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In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{fig3.epsi} \end{figure}$ Figure 3: Stellar ionizing radiation - Incident (line) and transmitted (points); the y axis values are suitably scaled.
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In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{fig1.epsi}\par\end{figure}$	Figure 1: HST image of the planetary nebula NGC 6886 as observed through the [O III] and [N II] filters, where the overall morphology is clearly visible. North is up and East is left.
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$\begin{figure} \par\includegraphics[width=8.3cm,clip]{fig2.epsi} \end{figure}$	Figure 2: $T_{\rm e}$ and $N_{\rm e}$ across the nebula.
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$\begin{figure} \par\includegraphics[width=8.4cm,clip]{fig3.epsi} \end{figure}$	Figure 3: Stellar ionizing radiation - Incident (line) and transmitted (points); the y axis values are suitably scaled.
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