\begin{table}%t2
%\centering
\par
\caption{Upper limits ($1 \sigma$ and $3 \sigma$) for the projected 
rotational 
velocities of the stars from Paper~I. $1 \sigma$ limits have not been 
published previously.
}
\label{nonrotating}
\begin{tabular}{lccc} \hline \hline\noalign{\smallskip}
WD & White dwarf &  $v \sin i$ (\kms)&  $v \sin i$ (\kms) \\ 
   &             &   $1 \sigma$              &  $3 \sigma$   \\ 
\hline
0352+096 & HZ~4    & $<$13  & $<$21  \\
0406+169 & LB~227  & $<$20  &  $<$28  \\
0421+162 & VR~7    & $<$8  &  $<$18\\
0425+168 & VR~16   & $<$18  &  $<$26\\
0431+125 & HZ~7    & $\rm 15^{+7}_{-5}$  & $<$35  \\
0438+108 & HZ~14   & $<$14  & $<$28  \\
0836+197 & LB~5893 & $<$22  & $<$43  \\
0837+199 & LB~393  & $<$9  & $<$29  \\
0413$-$077 & 40~Eri~B & $<$~1 & $<$~8   \\
0726+393 & LP207-7  & $<$7 & $<$18  \\
1143+321 & G148-7   & $<$2 & $<$12  \\
1314+293 & HZ43     & $<$11 & $<$29  \\
1911+135 & G142-B2B & $<$2 & $<$9  \\ \hline  
\end{tabular}%\\[3mm]
\end{table}