All Figures

$\begin{figure} \par\includegraphics[width=15.6cm,clip]{ms3581f2a.eps}\par\includegraphics[width=15.6cm,clip]{ms3581f2b.eps}\end{figure}$ Figure 2: Observed diagrams for our program clusters. The solid line is the normality line whereas the dotted lines are the confidence intervals corresponding to 99.9%. The error bars for each individual object are the mean errors. The measurement errors of V are much smaller than the symbols and have been omitted. The scales for the upper and lower diagrams of NGC 3114, NGC 6204 and NGC 6756 are different because the relevant range for peculiar objects in the a versus (g1-y) diagrams seemed worthwhile to be shown.
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In the text

$\begin{figure} \par\includegraphics[width=15.2cm,clip]{ms3581f1.eps}\par\par\end{figure}$ Figure 1: Finding charts for the program clusters. North is to the right and west is upwards; 1 pixel = 0.5 $\hbox {$^{\prime \prime }$ }$ . The sizes (by area) of the open circles are inversely proportional to the V-magnitudes taken from Tables 4 to 8. Larger open circles denote brighter objects. We have plotted the clusters sorted for the individual field of views.
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In the text

$\begin{figure} \par\includegraphics[width=15.2cm,clip]{ms3581f1.eps}\par\par\end{figure}$	Figure 1: Finding charts for the program clusters. North is to the right and west is upwards; 1 pixel = 0.5 $\hbox {$^{\prime \prime }$ }$ . The sizes (by area) of the open circles are inversely proportional to the V-magnitudes taken from Tables 4 to 8. Larger open circles denote brighter objects. We have plotted the clusters sorted for the individual field of views.
Open with DEXTER