All Figures

$\begin{figure} \par\includegraphics[width=17cm,clip]{0529fig1.ps} \end{figure}$ Figure 1: A montage of the three newly discovered eclipsing systems. Each row depicts from left to right: an H $\alpha$ image of the nebula, an OGLE-III I-band image, and a phased OGLE-III light curve of the central star (marked on the I-band image). Periods and ephemerides are given in Table 1. All images are $30 \times 30$ arcsec² with North to top and East to left. The solid curve is a binned light curve representation sampled at $\delta \phi =0.01$ .
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=8.4cm,clip]{0529fig2.ps} \end{figure}$ Figure 2: AAOmega spectroscopy for M 3-16 ( top) and M 2-19 ( bottom) showing stellar He II absorption lines (dotted lines). Contaminating nebular emission lines are also present. The spectra have been rectified and smoothed.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=8.4cm,clip]{0529fig2.ps} \end{figure}$	Figure 2: AAOmega spectroscopy for M 3-16 ( top) and M 2-19 ( bottom) showing stellar He II absorption lines (dotted lines). Contaminating nebular emission lines are also present. The spectra have been rectified and smoothed.
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