\begin{table}%tA.1
\caption{\label{tablefour}Parameters for the brightest stellar members of
	Tr~14. Values include: luminosity$^a$ ($L$); effective temperature$^a$ ($T_{{\rm eff}}$); FUV
	luminosity$^b$ ($L_{{\rm FUV}}$); ionizing photon flux per second$^b$
	($N_{\rm L}$), stellar wind terminal velocity$^c$ ($v_{\infty}$); stellar wind
	mass-loss rate$^d$ ({\it \.M}) and the
	mechanical luminosity ($L_W$) given by $0.5 \times Mv_{\infty}^2$.}
%\centerline
{
\begin{tabular}{@{}lllllllll} 
\hline
\hline 
	Star$^a$ 
	& Spectral$^a$  
	& $L$ 
	& $T_{{\rm eff}}$    
	& $L_{{\rm FUV}}$ 
        & $N_{\rm L}$
	& $v_{\infty}$
	& {\it \.M}	 
	& $L_W$ \\ 
\hline 
	& Type 
	& $10^{5}$ $L_{\odot}$ 
	& $10^4$~K 
	& $10^{5}$ $L_{\odot}$ 
	& $10^{47}$ s$^{-1}$ 
	& km s$^{-1}$ 
	& $10^{-7}$ $M_{\odot}$ yr$^{-1}$ 
	& $10^{43}$ erg yr$^{-1}$ \\ 
\hline 
	HD93129A 
	& O3I 
	& 47.9 
	& 4.7 
	& 22.4 
	& 594 
	& 3000 
	& 533 
	& 477  \\ 
	HD93160 
	& O6III 
	& 9.1 
	& 4.0 
	& 5.5 
	& 90 
	& 2500 
	& 23 
	& 14 \\ 
	HD93161W 
	& O6.5V 
	& 5.5 
	& 4.0 
	& 3.3 
	& 55 
	& 2600 
	& 11 
	& 8 \\ 
	HD93161E 
	& O6.5V 
	& 10.0 
	& 4.3 
	& 4.7 
	& 163 
	& 2600 
	& 27 
	& 19 \\ 
	HD93128 
	& O3V 
	& 15.5 
	& 5.3 
	& 5.6 
	& 214 
	& 3200 
	& 48 
	& 49 \\	
	HD93129B 
	& O3V 
	& 13.5 
	& 5.3 
	& 4.9 
	& 186 
	& 3200 
	& 40 
	& 41 \\ 
	7  
	& O6.5V 
	& 2.4 
	& 4.0 
	& 1.4 
	& 24 
	& 2600 
	& 3.8 
	& 2.6 \\ 
	8 
	& O6V 
	& 3.9 
	& 4.1 
	& 2.3 
	& 35 
	& 2600 
	& 7.5 
	& 5.0 \\
	11 
	& O8V 
	& 2.0 
	& 3.6 
	& 1.3 
	& 12	 
	& 1900 
	& 3.6 
	& 1.3 \\
	13  
	& O9V 
	& 0.72 
	& 3.3 
	& 0.5 
	& 6 
	& 1500 
	& 1.1 
	& 0.25 \\
	15 
	& O9V 
	& 1.0 
	& 3.3 
	& 0.6 
	& 8 
	& 1500 
	& 1.6 
	& 0.36 \\
	23 
	& 09V 
	& 0.22 
	& 3.3 
	& 0.7 
	& 2 
	& 1500 
	& 0.2 
	& 0.05 \\
	25 
	& 09V 
	& 0.3 
	& 3.3 
	& 0.2 
	& 2 
	& 1500 
	& 0.3 
	& 0.06 \\ 
%\\ 
        {\it Total} 
	& 
	&{\it $\sim$110} 
	& 
	&{\it $\sim$50} 
	&{\it $\sim$1400} 
	& 
	& 
	& {\it $\sim$600} \\ 
\hline 
\end{tabular}}  
\medskip
$^a$ Taken from \citet{Vazquez96}.\\
$^b$ Derived using stellar models of \citet{Kurucz97}.\\
$^c$ Taken from Table~\ref{tableone} in \citet{Kudritzki00}.\\
$^d$ According to the wind-momentum luminosity relation given in Eq.~(10) by \citet{Kudritzki00}.
\end{table}