$\begin{figure} \par\includegraphics[width=8.15cm,clip]{4389fig1.eps} \end{figure}$ Figure 1: The fractional emission measure of the blue wing as a function of the logarithm of the total H $\alpha$ luminosity.
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In the text

$\begin{figure} \par\includegraphics[width=8.15cm,clip]{4389fig2.eps} \end{figure}$ Figure 2: The fractional emission measure of the red wing as a function of the logarithm of the total H $\alpha$ luminosity.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{4389fig3.eps} \end{figure}$ Figure 3: The velocity separation of the blue wing from the bright, central component as a function of the logarithm of the total H $\alpha$ luminosity.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{4389fig4.eps} \end{figure}$ Figure 4: The velocity separation of the red wing from the bright, central component as a function of the logarithm of the total H $\alpha$ luminosity.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{4389fig5.eps} \end{figure}$ Figure 5: The velocity dispersion of the blue wing as a function of the logarithm of the total H $\alpha$ luminosity.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{4389fig6.eps} \end{figure}$ Figure 6: The velocity dispersion of the red wing as a function of the logarithm of the total H $\alpha$ luminosity.
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In the text

$\begin{figure} \par\includegraphics[width=7.85cm,clip]{4389fig7.eps} \end{figure}$ Figure 7: The ratio of the kinetic energy of the shells and the energy in stellar winds as a function of the H $\alpha$ luminosity, supposing shells with $R_{{\rm shell}} = 0.2~R_{\rm reg}$ .
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In the text

$\begin{figure} \par\includegraphics[width=8.15cm,clip]{4389fig1.eps} \end{figure}$	Figure 1: The fractional emission measure of the blue wing as a function of the logarithm of the total H $\alpha$ luminosity.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.15cm,clip]{4389fig2.eps} \end{figure}$	Figure 2: The fractional emission measure of the red wing as a function of the logarithm of the total H $\alpha$ luminosity.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{4389fig3.eps} \end{figure}$	Figure 3: The velocity separation of the blue wing from the bright, central component as a function of the logarithm of the total H $\alpha$ luminosity.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{4389fig4.eps} \end{figure}$	Figure 4: The velocity separation of the red wing from the bright, central component as a function of the logarithm of the total H $\alpha$ luminosity.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{4389fig5.eps} \end{figure}$	Figure 5: The velocity dispersion of the blue wing as a function of the logarithm of the total H $\alpha$ luminosity.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{4389fig6.eps} \end{figure}$	Figure 6: The velocity dispersion of the red wing as a function of the logarithm of the total H $\alpha$ luminosity.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.85cm,clip]{4389fig7.eps} \end{figure}$	Figure 7: The ratio of the kinetic energy of the shells and the energy in stellar winds as a function of the H $\alpha$ luminosity, supposing shells with $R_{{\rm shell}} = 0.2~R_{\rm reg}$ .
Open with DEXTER