\begin{table}%T1
\caption{Data for the three Taurus low mass members.}\label{tab1}
%\centerline
 {
\begin{tabular}{cccc}
\hline\hline
                            &\multicolumn{3}{c}{KPNO-Tau}\\
\cline{2-4}
                            &   \#3            &    \#5   &  \#8 \\
\hline                                                                                                    
$Ic$                        & 15.77            &15.08            &15.10            \\
$J$                         & $13.323\pm0.022$ &$12.640\pm0.024$ &$12.946\pm0.022$ \\
$H$                         & $12.501\pm0.022$ &$11.918\pm0.024$ &$12.367\pm0.021$ \\
$Ks$                        & $12.079\pm0.021$ &$11.536\pm0.018$ &$11.985\pm0.022$ \\
%(I-J)                       & 2.447  	       & 2.440           & 2.154 \\
%(I-H)                       & 3.269  	       & 3.162           & 2.733 \\
%(I-K)                       & 3.691  	       & 3.544           & 3.115 \\
%(J-H)                       & 0.822  	       & 0.722           & 0.579 \\
%(H-K)                       & 0.422  	       & 0.382           & 0.382 \\
%(R-I)                       & 2.10   	       & 2.30            & 2.10  \\
Sp. type                     & M~6 (M~6)	       & M~7 (M~7.5)       & M~6 (M~5.75) \\
Width H$\alpha$ (km~s$^{-1}$)      & 310    	       & 125             & 240$^1$\\
$W$(H$\alpha$) (\AA)          &$81.4\pm5.7$ (130)&$21.1\pm0.9$ (30)& $12.0\pm1.0$ (17.5)\\
$W$(HeI 6678)   (\AA)          & 3.5: (6.5)       &  0.2:           & 0.2: \\
$W$(Li)        (\AA)          & 0.60 (Yes)       &  0.48           & 0.78 \\
log Lum(bol)/$L_\odot$      & $-$1.66/$-$1.76$^2$  & $-$1.70/$-$1.66$^2$ & $-$1.65/$-$1.76$^2$    \\
Mass ($M_\odot$)            & 0.07$^3$         & 0.06            & 0.07$^3$     \\
log {$L$(H$\alpha$)}/{$L$(bol)} & $-$2.87            &  $-$3.70          & $-$3.70  \\
$T_{\rm eff}$ (Luhman \cite{Luhman99})          & 2990             & 2890            & 2990 \\       
\hline
\end{tabular}
}\smallskip
Values in parenthesis are  from low resolution spectroscopy by
  Brice\~no et~al. (\cite{Briceno02}). A double colon implies a large
uncertainty in the measurement.\\
$^1$ 180~km~s$^{-1}$ without the asymmetry. \\
$^2$ From $Ic$ and $Ks$, respectively. \\
$^3$ 0.08~$M_\odot$ from the HR diagram. 
The listed values are from $Ic$ and Baraffe et~al. (\cite{Baraffe98})\\
\end{table}