Fig. 8
Comparison of the XLF of S254-S258 (thick grey line) to the XLF of the Orion Nebula Cluster (from the COUP data; Getman et al. 2005b, black line). The straight lines show the results of the power-law fits to the distributions in the luminosity range LX = 1030.5−1032.0 erg s-1.
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