$\begin{figure} \par {\includegraphics[width=8.8cm,clip]{2437fig7.eps} } \end{figure}$ Figure 7: Maser luminosities versus infrared luminosity. The least squares fits to the data are shown by dashed (red), thin (green) and thick (blue) lines for OH, CH₃OH and H₂O sources, respectively.
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In the text

$\begin{figure} \par {\includegraphics[width=17.8cm,clip]{2437fig1.eps} } \end{figure}$	Figure 1: Spectra of the newly detected water masers.
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$\begin{figure} \par {\includegraphics[width=17.5cm,clip]{2437fig2.eps} } \end{figure}$	Figure 2: Spectra of previously known water masers.
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$\begin{figure} \par {\includegraphics[width=8.8cm,clip]{2437fig3.eps} } \end{figure}$	Figure 3: Histograms of the velocity extent of three maser lines.
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$\begin{figure} \par {\includegraphics[width=8.8cm,clip]{2437fig4.eps} } \end{figure}$	Figure 4: Histograms of the difference in the centroid of the velocity maser intervals.
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$\begin{figure} \par {\includegraphics[width=8.8cm,clip]{2437fig5.eps} } \end{figure}$	Figure 5: Histograms of the maser luminosity for three species assuming the near kinematic distance.
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$\begin{figure} \par {\includegraphics[width=8.8cm,clip]{2437fig6.eps} } \end{figure}$	Figure 6: Histograms of the H₂O maser luminosity for our sample and that of Sridharan et al. (2002).
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$\begin{figure} \par {\includegraphics[width=8.8cm,clip]{2437fig7.eps} } \end{figure}$	Figure 7: Maser luminosities versus infrared luminosity. The least squares fits to the data are shown by dashed (red), thin (green) and thick (blue) lines for OH, CH₃OH and H₂O sources, respectively.
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