Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3940fig1a.ps}\par\vspace{... ...}\par\vspace{3mm} \includegraphics[width=8.8cm,clip]{3940fig1c.ps} \end{figure}$	Figure 1: The distribution of the stars from the data-base in Galactic coordinates. Top: all stars, middle: only stars with complete photometry, bottom: stars without or with partial photometry.
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$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics{3940fig2a.ps}}\par\vspa... ...\vspace*{5mm} \resizebox{8.8cm}{!}{\includegraphics{3940fig2c.ps}} \end{figure}$	Figure 2: First two panels: the distribution of the stars with complete photometry and stars without or with partial photometry over the V-magnitude range. Bottom: the completeness of the data-base in percent for successive V-magnitude intervals.
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