$\begin{figure} \par\includegraphics[width=8cm,height=7.5cm,clip]{3722-f1a}\hspac... ...ce*{2mm} \includegraphics[width=8.5cm,height=7.5cm,clip]{3722-f1d} \end{figure}$ Figure 1: Model output for $\alpha$ Ori. From top left to bottom left: modelled visibility curve with interferometric data for the bands K, L, and N; bottom right: modelled spectral energy distribution with photometric data. Model parameters (see Table 5): $T_\star=3640~{\rm K}$ , $R_\star=21.8~{\rm mas}$ , $r_{\rm i}=45.9~R_\star$ , $r_{\rm o}=48.2~R_\star$ , and $\tau _{11}=0.0065$ .
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In the text

$\begin{figure} \par\includegraphics[width=8cm,height=7.5cm,clip]{3722-f2a}\hspac... ...ce*{2mm} \includegraphics[width=8.5cm,height=7.5cm,clip]{3722-f2d} \end{figure}$ Figure 2: Model output for SW Vir. Top left and right: modelled visibility curve with interferometric data for the K and L bands; bottom left: expected visibility curve for the N band; bottom right: modelled spectral energy distribution with photometric data. Model parameters (see Table 5): $T_\star=2800~{\rm K}$ , $R_\star=8.65~{\rm mas}$ , $r_{\rm i}=15.0~R_\star$ , $r_{\rm o}=1000~R_\star$ , and $\tau _{11}=0.045$ .
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In the text

$\begin{figure} \par\includegraphics[width=8cm,height=7.5cm,clip]{3722-f3a}\hspac... ...ce*{2mm} \includegraphics[width=8.5cm,height=7.5cm,clip]{3722-f3d} \end{figure}$ Figure 3: Model output for R Leo. From top left to bottom left: modelled visibility curve with interferometric data for the bands K, L, and N; bottom right: modelled spectral energy distribution with photometric data. Model parameters (see Table 5): $T_\star=2500~{\rm K}$ , $R_\star=14.9~{\rm mas}$ , $r_{\rm i}=3.5~R_\star$ , $r_{\rm o}=140~R_\star$ , and $\tau _{11}=0.1$ .
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In the text

$\begin{figure} \par\includegraphics[width=8cm,height=7.5cm,clip]{3722-f1a}\hspac... ...ce*{2mm} \includegraphics[width=8.5cm,height=7.5cm,clip]{3722-f1d} \end{figure}$	Figure 1: Model output for $\alpha$ Ori. From top left to bottom left: modelled visibility curve with interferometric data for the bands K, L, and N; bottom right: modelled spectral energy distribution with photometric data. Model parameters (see Table 5): $T_\star=3640~{\rm K}$ , $R_\star=21.8~{\rm mas}$ , $r_{\rm i}=45.9~R_\star$ , $r_{\rm o}=48.2~R_\star$ , and $\tau _{11}=0.0065$ .
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$\begin{figure} \par\includegraphics[width=8cm,height=7.5cm,clip]{3722-f3a}\hspac... ...ce*{2mm} \includegraphics[width=8.5cm,height=7.5cm,clip]{3722-f3d} \end{figure}$	Figure 3: Model output for R Leo. From top left to bottom left: modelled visibility curve with interferometric data for the bands K, L, and N; bottom right: modelled spectral energy distribution with photometric data. Model parameters (see Table 5): $T_\star=2500~{\rm K}$ , $R_\star=14.9~{\rm mas}$ , $r_{\rm i}=3.5~R_\star$ , $r_{\rm o}=140~R_\star$ , and $\tau _{11}=0.1$ .
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