\begin{table}%T1
%\centering
\par
\caption{Spectral parameters of X-ray sources associated with HH~210
using a {\tt WABS$\times$APEC} plasma model with solar elemental
abundances. We used Chi statistics with
standard weighting. Confidence ranges at the 68\% level
($\Delta\chi^2=1$; corresponding to $\sigma=1$ for Gaussian
statistics) are given in parentheses. $Q$ in Col.~(8) is the
probability that the best-fit model matches the data, given the value
of $\chi^2$ and $\nu$, the degree of freedom in Col.~(7). The emission
measure in Col.~(6) and the logarithm of the X-ray luminosities in the
0.5--2~keV energy range observed/corrected for absorption in
Col.~(9) were computed assuming a distance of 450~pc.}
\label{fit}
{
\begin{tabular}{ccccccccc}
\hline\hline\\[-3.2mm]
COUP & CXOONCJ & Net & $N_{\rm H}$ & $kT$ & $EM$ & $\chi^2_\nu$ ($\nu$) & $Q$ & $\log L_{\rm S}/\log L_{\rm S,c}$ \\
\#   &         & counts & $10^{21}$~cm$^{-2}$ & keV & $10^{55}$~cm$^{-3}$ & & \% & erg~s$^{-1}$ \\
(1) & (2) & (3) & (4) & (5) & (6) & (7) & (8) & (9) \\
\hline
703 & 053515.4-052040.3 &  31 & 8 (5--11) & 0.07 (0.05--0.14) & 1.5 & 0.70 (5) & 62 &  27.3~/~30.0\\
704 & 053515.4-052045.5 &  24 & 0 ($\le$0.3)& 0.33 (0.22--0.45) &
$3\times10^{-5}$ & 1.08 (3) & 36 & 27.1~/~27.1 \\
 &  &  & 10 (7--13)&  0.07 ($\le$0.09) & 48 & 1.20 (3) & 31 & 27.1~/~30.3 \\
\hline
\end{tabular}}
\end{table}