\begin{table}%t2 [t]
%\centering
\par
\caption{Sine fits to the \Ha\ emission line radial
  velocities\label{t-rvfits}. The methods employed were a convolution
  with a single Gaussian (SG) or \citeauthor{schneider+young80-2}'s
  (\citeyear{schneider+young80-2}) double-Gaussian prescription (DG).}
%
%\begin{flushleft}
\begin{tabular}{ccccccc}
\hline\hline\noalign{\smallskip} Object & Method & {\it FWHM}/Sep. (\kms) & \T\ & Period
(days) & $K$ (\kms) & $\gamma$ (\kms)\\ \hline\noalign{\smallskip}
%
HS~0139+0559 & SG & 600 & $2452998.985\pm0.013$ & $0.16923\pm0.00034$ &
$84.4\pm4.8$ & $18.4\pm3.5$ \\ 
HS~0229+8016 & SG & 600 & $2452992.457\pm0.006$ & $0.161493\pm0.000034$ & 
$179.0\pm5.2$ & $35.5\pm3.5$ \\ 
HS~0506+7725 & DG & 700/1500 & $2452990.679\pm0.022$ & $0.14770\pm0.00014$ & 
$42.6\pm4.4$ & $-66.7\pm3.0$\\
%
\noalign{\smallskip}\hline
\end{tabular}
%\end{flushleft}
\end{table}