\begin{table}%t2
\caption{Radial velocities (from Si), projected rotational velocities,
macro- and micro-turbulent velocities (all in \kms) and Si abundances, given
as log [$N$(Si)/$N$(H] + 12, of the sample stars 
as determined in the present study. The number in brackets refers to the number
of lines used to derive \vsini and \vmac.}
\label{para_1}
%\centering
\par
\begin{tabular}{llrllrc}
\hline 
\hline
%~\\
\multicolumn{1}{l}{Object}
&\multicolumn{1}{l}{Sp}
&\multicolumn{1}{c}{\Vr}
&\multicolumn{1}{c}{\vsini}
&\multicolumn{1}{c}{\vmac}
&\multicolumn{1}{c}{\vmic}
&\multicolumn{1}{c}{Si abnd}
\\
\hline
HD 185859  &B0.5 Ia   &12      &62(5)  &58(3)   &18  &7.51 \\%69
HD 190603  &B1.5 Ia+  &50      &47(8)  &60(3)   &15  &7.46 \\%69
HD 206165  &B2 Ib     &0       &45(7)  &57(3)   &8   &7.58 \\%69
HD 198478  &B2.5 Ia   &8       &39(9)  &53(3)   &8   &7.58 \\%38
HD 191243  &B5 Ib     &25      &38(4)  &37(3)   &8   &7.48 \\%38
HD 199478  &B8 Iae    &--12     &41(4)  &40(3)   &8   &7.55 \\%52
HD 212593  &B9 Iab    &--13     &28(3)  &25(3)   &7   &7.65 \\%26
HD 202850  &B9 Iab    &13      &33(3)  &33(3)   &7   &7.99 \\%26
\hline
\end{tabular}
\end{table}