\begin{table}%T5
\caption{Data for stars in the region of Bo~7.}
\label{tab05}
%\centerline
{%\scriptsize
\begin{tabular}{llccccc}
\hline\hline
LSS  & Sp.Type & $V^a$ & $B-V^a$ & $E(B-V)$ & $V_0-M_v$ & $RV$\\
  &     &           &            &         &         & (LSR)  \\
\hline
1131      &     O7.5V & 10.80 & 0.51  & 0.83   & 13.33  & +50 \\
1132$^b$ & B3V  & 10.05 & 0.37  & 0.54   & 9.88   & --13 \\
1135      & O6.5V((f))& 10.88 & 0.40  & 0.73   & 13.95  & +55 \\
1137      &    O9V    & 11.38 & 0.49  & 0.80   & 13.40  & +42 \\
1140      &    B0III  & 11.65 & 0.76  & 1.05   & 13.49  & +40 \\
1144      &     O7.5V & 11.27 & 0.64  & 0.96   & 13.39  & +53 \\
1145$^c$  &       WN8 & 10.78 & 0.56  &        &        &  var.\\
1146$^d$  &     B1III & 11.57 & 0.50  &  0.82  & 13.43  & +26 \\
1147$^e$  &      B1Ve &  11.53& 0.58  &  0.78  & 13.11  & +54\\
\hline
\end{tabular}}
\par
\medskip
$^a$ From Moffat \& Vogt (\cite{Moffat}).\\
$^b$ Foreground star, see also Lundstrom \& Stenholm (\cite{Lundstrom}).\\
$^c$ WR 12 cf. van~der~Hucht (\cite{Hucht}). Spectroscopic binary Niemela (\cite{Virpi}). \\
$^d$ Line widths appear variable. May be an unresolved.\\
double--lined binary?\\
$^e$ H Balmer lines H$\beta$ and H$\gamma$ show central emission, see Fig.~\ref{fig01}.\\
\end{table}