Fig. 12
Comparison of the X-ray luminosity function of the Chandra sources in our Gum 31 observation (grey-shaded histogram) to (top) the XLF of the Orion nebula cluster (dashed histogram) (from the COUP data; Getman et al. 2005), and to (bottom) the XLF for the CCCP sources as shown in Fig. 3 of Feigelson et al. (2011), scaled to account for the different sample sizes.
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