\begin{table}%t2
%\centering
\par
\caption{\label{detect-vels}Main sequence A-type stars in which evidence of velocity fields is directly detected in line profiles.}
\begin{tabular}{llllllllll}
\hline\hline
  HD     &  other    & spectral & binarity & \te & $\xi$  & depressed & line shape  & \multicolumn{2}{c}{\vsi} \\ \cline{9-10}
         &           & type     &          &     &        & blue wing & discrepancy & weak lines & strong lines \\
         &           &          &          & (K) & (\kms) &           &             & (\kms)    &  (\kms)     \\
\hline
2421 A   & HR 104 A  & A2Vs &       SB2 &  10~000 & 1.0    &    weak   & none        & 3.5       & 3.5 \\
72660    & HR 3383   & A1V  &           &  9650  & 2.3    &    weak   & weak        & 5.0       & 6.1 \\
114330   & $\theta$ Vir & A1Vs &    VB2 &  9250  & 1.3    &    weak   & weak        & 4.0       & 5.5 \\
157486 A & HR 6470 A & A0V  &       SB2 &  9150  & 1.9    &    weak   & weak        & 1.5       & 3.5 \\
27962    & 68 Tau    & A2IV m &     SB1 &  8975  & 2.0    &    weak   & weak        & 11        & 11.5 \\
103578 A & 95 Leo A  & A3V &        SB2 &  8300  & 2.0    &    strong & strong      & 3         & 9 \\
107168   & 8 Com     & A8 m &           &  8150  & 3.0    &    weak   & weak        & 13        & 14 \\
108642 A & HR 4750 A & A2 m &       SB1 &  8100  & 4.0    &    strong & strong      & 2         & 10 \\
209625   & 32 Aqr    & A5 m &       SB1 &  7700  & 4.0    &    strong & strong      & 4.5       & 10 \\
\hline
\end{tabular}
\end{table}