Astronomy & Astrophysics

$\begin{figure} {\resizebox{8.1cm}{!}{\includegraphics[clip]{2039fig3.eps}} } \end{figure}$ Figure 3: Distribution of characteristic sizes, as explained in the text. Note that the scale of the horizontal axis is arbitrary. The dotted and solid lines are for CHARM and CHARM2, respectively.
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In the text

$\begin{figure} {\resizebox{8.1cm}{!}{\includegraphics[clip]{2039fig6.eps}} } \end{figure}$ Figure 6: Distribution of luminosity class. The bin for luminosity class III contains 5181 entries and is shown clipped for clarity.
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In the text

$\begin{figure} {\resizebox{8.1cm}{!}{\includegraphics[clip]{2039fig1.eps}} } \end{figure}$	Figure 1: Distribution of publications included in CHARM2 by year. Each bin is two years wide.
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$\begin{figure} {\resizebox{8.1cm}{!}{\includegraphics[clip]{2039fig2.eps}} } \end{figure}$	Figure 2: Distribution of V, K and 12 $\mu$ m magnitudes (dotted, solid and dashed lines respectively).
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$\begin{figure} {\resizebox{8.1cm}{!}{\includegraphics[clip]{2039fig3.eps}} } \end{figure}$	Figure 3: Distribution of characteristic sizes, as explained in the text. Note that the scale of the horizontal axis is arbitrary. The dotted and solid lines are for CHARM and CHARM2, respectively.
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$\begin{figure} {\resizebox{8.1cm}{!}{\includegraphics[clip]{2039fig4.eps}} } \end{figure}$	Figure 4: Distribution of binary separations.
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$\begin{figure} {\resizebox{8.1cm}{!}{\includegraphics[clip]{2039fig5.eps}} } \end{figure}$	Figure 5: Distribution of the main spectral types.
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$\begin{figure} {\resizebox{8.1cm}{!}{\includegraphics[clip]{2039fig6.eps}} } \end{figure}$	Figure 6: Distribution of luminosity class. The bin for luminosity class III contains 5181 entries and is shown clipped for clarity.
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