All Tables

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.