$\begin{figure} \par\includegraphics[width=10.5cm, height=11.1cm,clip]{0770fi1.ps}\end{figure}$ Figure 1: Positions of OB classified stars with an automated method of correlation. The circles present the regions of SN explosions.
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In the text

$\begin{figure} \par\includegraphics[width=6.1cm,height=6.5cm,clip]{0770fi2a.ps}\... ...*{6mm} \includegraphics[width=6.1cm, height=6.5cm,clip]{0770fi2d.ps}\end{figure}$ Figure 2: Upper left: isodensity contours for main sequence OB stars younger than $8 \times 10^6$ yr. Upper right: isodensity contours for main sequence B stars with ages between $8 \times 10^6$ and $1.2 \times 10^7$ yr. Lower left: isodensity contours for main sequence B stars with ages between $1.2 \times 10^7$ and $3 \times 10^7$ yr. Lower right: density distribution for main sequence B stars with ages older than $3 \times 10^7$ yr. The octagons present the regions of SN explosions. Subslices for these star ages do not give any significant contours.
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In the text

$\begin{figure} \par\includegraphics[width=10.5cm, height=11.1cm,clip]{0770fi1.ps}\end{figure}$	Figure 1: Positions of OB classified stars with an automated method of correlation. The circles present the regions of SN explosions.
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