\begin{table}%t1
%\centering
\par
\caption{Parameters of the program stars. The data were taken from the Bright
Star Catalogue (Hoffleit \& Warren \cite{bsc}). Distances have been calculated using 
\mbox{HIPPARCOS} parallaxes (ESA \cite{hipp}). The last column indicates whether 
a star was observed from \mbox{ESO (E)} or \mbox{SAO (S)}.}
\label{stars}
\begin{tabular}{rrrclrrrrrrc}
\hline\hline
HR   &Name               &HD      &$m_{v}$& Sp.~   & $T_{\rm eff}$~&  $\log g$~~        & $v \sin i$  &$d$~~ & RA             & DEC           &Obs.\\
     &                   &        &       & Type   &      (K)~     &$(\mbox{cm~s}^{-2}$)&   (km~s$^{-1}$)  &(pc) & h~~m~~~s        & $^{\circ}$~~~$^{\prime}$~~~$^{\prime}$~$^{\prime}$           & \\
%\cline{1-10}\\[-2.0mm]
\hline
 806 &    $\epsilon$ Hyi &  16~978 &  4.11 & B9~V  & 10~910 & 4.29 &$ 100\pm2$ & 47.01& 02 39 35 & - 68 16 01 &E ~\\
1070 &         17    Eri &  21~790 &  4.73 & B9~V  & 11~540 & 3.61 &$  86\pm2$&116.69& 03 30 37 & - 05 04 31 &E ~\\
1092 &                   &  22~252 &  5.83 & B8~V  & 11~860 & 3.27 &$ 260\pm15$&261.10& 03 30 52 & - 66 29 23 &E ~\\
1214 &                   &  24~626 &  5.11 & B6~V  & 14~300 & 4.12 &$  29\pm2$&108.81& 03 53 39 & - 34 43 56 &E ~\\
1339 &         53    Tau &  27~295 &  5.35 & B9~IV & 12~000 & 4.19 &$   5\pm2$& 81.96& 04 19 26 & + 21 08 32 &S ~\\
1582 &         62    Eri &  31~512 &  5.51 & B6~V  & 15~190 & 3.87 &$  89\pm4$&226.76& 04 56 24 & - 05 10 17 &E ~\\
1723 &                   &  34~310 &  5.07 & B9~V  & 11~180 & 4.12 &$ 158\pm2$& 83.47& 05 15 24 & - 26 56 36 &E ~\\
1728 &         17    Aur &  34~364 &  6.14 & B9.5~V& 11~010 & 4.34 &$  30\pm4$&121.95& 05 18 19 & + 33 46 02 &S ~\\
1973 &                   &  38~170 &  5.29 & B9.5~V& 10~250 & 3.69 &$  60\pm4$&111.24& 05 42 15 & - 34 40 04 &E ~\\
2056 &     $\lambda$ Col &  39~764 &  4.87 & B5~V  & 15~370 & 4.22 &$ 101\pm3$&104.71& 05 53 07 & - 33 48 05 &E ~\\
2948 &                   &  61~555 &  4.50 & B6~V  & 15~460 & 4.20 &$  50\pm5$&139.28& 07 38 49 & - 26 48 06 &E ~\\
3158 &                   &  66~552 &  6.15 & B9~V  & 10~450 & 4.09 &$  75\pm4$& 91.57& 08 04 45 & + 18 50 32 &S ~\\
3439 &                   &  74~067 &  5.20 & B9~V  & 10~880 & 4.14 &$  36\pm3$& 85.98& 08 40 19 & - 40 51 15 &E ~\\
3717 &                   &  80~781 &  6.28 & B5~V  & 14~980 & 3.22 &$  30\pm3$&1052.63&09 19 33 & - 55 11 12 &E ~\\
4116 &      $\delta$ Sex &  90~882 &  5.21 & B9.5~V& 10~360 & 3.84 &$ 140\pm3$& 91.99& 10 29 29 & - 02 44 21 &S ~\\
4119 &       $\beta$ Sex &  90~994 &  5.09 & B6~V  & 14~570 & 4.21 &$  85\pm4$&105.71& 10 30 18 & - 00 38 13 &E ~\\
4943 &         14    CVn & 113~797 &  5.25 & B9~V  & 11~260 & 4.06 &$ 130\pm3$& 86.58& 13 05 45 & + 35 47 56 &S ~\\
5501 &        108    Vir & 129~956 &  5.69 & B9.5~V& 10~250 & 3.75 &$  84\pm4$&188.32& 14 45 30 & + 00 43 02 &E ~\\
5685 &       $\beta$ Lib & 135~742 &  2.61 & B8~V  & 12~040 & 3.26 &$ 320\pm20$& 49.06& 15 17 00 & - 09 22 59 &S ~\\
5994 &   $\iota^{2}$ Nor & 144~480 &  5.57 & B9.5~V& 10~580 & 4.29 &$  87\pm3$& 83.19& 16 09 19 & - 57 56 04 &E ~\\
6628 &                   & 161~840 &  4.83 & B8~V  & 11~990 & 3.38 &$  38\pm2$&186.22& 17 49 11 & - 31 42 12 &E ~\\
6633 &                   & 161~941 &  6.22 & B9.5~V&  9960 & 3.26 &$  36\pm3$&757.58& 17 48 20 & + 03 48 15 &E ~\\
6647 &                   & 162~374 &  5.90 & B6~V  & 16~900 & 3.72 &$  38\pm2$&254.45& 17 52 14 & - 34 47 57 &E ~\\
6668 &                   & 162~817 &  5.96 & B9.5~V&  9190 & 3.15 &$  76\pm4$&258.40& 17 54 27 & - 34 27 59 &E ~\\
6878 &                   & 169~009 &  6.33 & B9.5~V& 10~440 & 3.95 &$  47\pm5$&105.15& 18 23 02 & - 10 13 07 &E ~\\
7337 &    $\beta^{1}$Sgr & 181~454 &  4.01 & B9~V  & 11~960 & 3.83 &$  77\pm2$&116.01& 19 22 38 & - 44 27 32 &E ~\\
8781 &      $\alpha$ Peg & 218~045 &  2.49 & B9~V  &  9810 & 3.51 &$ 130\pm2$& 42.80& 23 04 46 & + 15 12 19 &S ~\\
\hline
\end{tabular}
\end{table}