\begin{table}%t1
%\centering
\par
\caption{\label{tabfluxha}H$\alpha$ fluxes, equivalent widths, and Rossby numbers 
of the LMXBs displayed in Fig.~\ref{figrharo}.}    
%\centering
\par
\begin{tabular}{lrrrrrrrrr}
\hline
\hline
\noalign{\smallskip}
Object & $EW$(H$\alpha$)$^{a}$ & \teff & \logg & $\log F({\rm H}\alpha)$ & $\log R({\rm H}\alpha)$ & $\tau_{\rm c}$$^{b}$ & $P_{\rm orb}$ & $\log R_0$ & Refs.$^{c}$\\       
\noalign{\smallskip}
   & [\AA] & [K] & [dex] & [$10^6$ erg cm$^{-2}$ s$^{-1}$] & [dex] & [days] & [days] & [dex] & \\       \noalign{\smallskip}
\hline
\noalign{\smallskip}
A0620--00         & $2.82\pm0.34$ & $4900\pm100$ & 4.2 & $6.95\pm0.05$ & $-3.57\pm0.06$ & 22.7 & 0.32 & $-$1.85 & 1, 2 \\
Nova Muscae 1991  & $3.65\pm0.32$ & $4500\pm100$$^{d}$ & 4.1$^{d}$ & $6.89\pm0.08$ & $-3.48\pm0.09$ & 24.6 & 0.43 & $-$1.74 & 3,4 \\
Cen X-4$^{e}$     & $2.27\pm0.67$ & $4500\pm100$ & 3.9 & $6.68\pm0.11$ & $-3.68\pm0.12$ & 24.7 & 0.63 & $-$1.58 & 5, 6 \\
Cen X-4$^{f}$     & $4.40\pm0.50$ & $4500\pm100$ & 3.9 & $6.96\pm0.05$ & $-3.40\pm0.06$ & 24.7 & 0.63 & $-$1.58 & 6, 7 \\
Nova Scorpii 1994 & $10.0\pm0.50$ & $6100\pm100$ & 3.7 & $7.92\pm0.02$ & $-2.97\pm0.04$ & 7.6  & 2.62 & $-$0.60 & 8, 9, 10 \\
\noalign{\smallskip}
\hline     
\end{tabular}
\tablefoot{
$^{a}$ Corrected equivalent width of narrow H$\alpha$ component
of the secondary star. $^{b}$ Convective turnover time derived from the equations in 
\citet{noy84} for dwarfs stars and using the turnover times given in
\citet{bas87} for subgiant and giant stars. $^{c}$ References: (1) \citet{gon04}, (2) \citet{mar86}, (3) \citet{cas97}, (4) \citet{rem92}, (5) \citet{tor02},
(6) \citet{gon05}, (7) \citet{dav05}, (8) \citet{sha99}, 
(9) \citet{gon08a}, (10) \citet{hoo98}. $^{d}$ Adopted values according to the effective temperature and surface 
gravity for the spectral type and orbital period. $^{e}$ H$\alpha$ equivalent width obtained from \citet{tor02}.
 $^{f}$H$\alpha$ equivalent width obtained from \citet{dav05}.}
\end{table}