All Figures

$\begin{figure} \par\includegraphics[height=12.7cm,width=13.5cm,angle=-90,clip]{4743_1.ps} \end{figure}$ Figure 1: Diagnostic diagrams confirming the strong correlations between integrated radio continuum, B-band, UV, and soft X-ray (0.3-2.0 keV) luminosities. X-ray luminosities also correlate well with the energy input rate by SNe ( $\dot{E}_{\rm A}$ ) and with FIR and H $\alpha$ SFRs. Circles address our sample, squares represent data from Strickland et al. (2004b), and triangles denote data collected from the literature (cf. Table 1). Filled (open) symbols refer to galaxies with (un)detected multi-phase gaseous halos. Solid lines are best fits from linear regression, while dashed lines indicate the trend expected for a relationship of unit slope. $r_{\rm s}$ is the Spearman rank-order correlation coefficient.
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In the text

$\begin{figure} \par\includegraphics[height=12.2cm,width=8.7cm,angle=-90,clip]{4743_2.ps} \end{figure}$ Figure 2: Functional dependence between soft X-ray luminosities and $L_{\rm FIR}/D^{2}_{25}$ ( upper left), the dust mass of a galaxy ( upper right), its H I mass ( lower left), and the baryonic mass ( lower right).
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In the text

$\begin{figure} \par\includegraphics[height=12.2cm,width=8.7cm,angle=-90,clip]{4743_3.ps} \end{figure}$ Figure 3: Functional dependence between $L_{\rm X,h}$ , the soft (0.3-2.0 keV) X-ray luminosity of the halo, and $L_{\rm FIR}/D^{2}_{25}$ ( upper left), $\dot{E}_{\rm A}$ ( upper right), ${\it SFR}_{\rm FIR}$ ( lower left), and ${\it SFR}_{\rm H\alpha }$ ( lower right). Solid symbols represent our sample, open symbols denote data taken from Strickland et al. (2004a). Solid and dashed lines have the same meaning as described in Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[height=12.2cm,width=8.7cm,angle=-90,clip]{4743_2.ps} \end{figure}$	Figure 2: Functional dependence between soft X-ray luminosities and $L_{\rm FIR}/D^{2}_{25}$ ( upper left), the dust mass of a galaxy ( upper right), its H I mass ( lower left), and the baryonic mass ( lower right).
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