Table 1: Spectral parameters of X-ray sources associated with HH 210 using a 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.
COUP CXOONCJ Net $N_{\rm H}$ kT EM $\chi^2_\nu$ ($\nu $) Q $\log L_{\rm S}/\log L_{\rm S,c}$
#   counts 1021 cm-2 keV 1055 cm-3   % erg s-1
(1) (2) (3) (4) (5) (6) (7) (8) (9)
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


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