$\begin{figure} \par\resizebox{15cm}{!}{\includegraphics[clip]{ms3627_fig1.eps}} \end{figure}$ Figure 1: Luminosity function and distribution according to morphological type derived for the galaxies in the catalogue. Darker histograms represent AGN hosts, while light gray bars include all galaxies in the sample.
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In the text

$\begin{figure} \par\resizebox{15.5cm}{!}{\includegraphics[clip]{ms3627_fig2a.eps}\includegraphics[clip]{ms3627_fig2b.eps}} \end{figure}$ Figure 2: Comparison between the mean Log M/L ratios for HI (left panels) and for molecular gas (right panels) extracted from the present catalogue and mean Log M/L ratios of previous studies (Casoli et al. 1998; Bregman et al. 1992). In the upper panel the mean masses are normalized with respect to D²₂₅, as adopted by Casoli et al. (1998), while in the lower panel $L_{\rm B}$ is the normalization factor, as adopted by Bregman et al. (1992). Our estimates agree with those published by Casoli et al. (1998) only for types later than S0.
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In the text

$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics[clip]{ms3627_fig3.eps}} \end{figure}$ Figure 3: The mean molecular to atomic gas content ratio as a function of Hubble type. The open symbols are derived from our catalogue, while full symbols represent ratios published by Casoli et al. (1998, full symbols).
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In the text

$\begin{figure} \par\resizebox{8.5cm}{!}{\includegraphics[clip]{ms3627_fig4.eps}} \end{figure}$ Figure 4: Variation of mean Log $L_{\rm X}$ /D²₂₅ and Log $L_{\rm X}$ / $L_{\rm B}$ ratios either including or excluding AGN host galaxies.
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In the text

$\begin{figure} \par\resizebox{15cm}{!}{\includegraphics[clip]{ms3627_fig1.eps}} \end{figure}$	Figure 1: Luminosity function and distribution according to morphological type derived for the galaxies in the catalogue. Darker histograms represent AGN hosts, while light gray bars include all galaxies in the sample.
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$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics[clip]{ms3627_fig3.eps}} \end{figure}$	Figure 3: The mean molecular to atomic gas content ratio as a function of Hubble type. The open symbols are derived from our catalogue, while full symbols represent ratios published by Casoli et al. (1998, full symbols).
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$\begin{figure} \par\resizebox{8.5cm}{!}{\includegraphics[clip]{ms3627_fig4.eps}} \end{figure}$	Figure 4: Variation of mean Log $L_{\rm X}$ /D²₂₅ and Log $L_{\rm X}$ / $L_{\rm B}$ ratios either including or excluding AGN host galaxies.
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