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Fig. 12


Cumulative luminosity distribution of X-ray SNRs and candidates in M 31 listed in Tables 3 and 4 for the band of 0.35–2.0 keV (solid line). For comparison, the distribution of SNRs in M 33 is also shown (dash-dotted line, Long et al. 2010). The dotted lines show the power-law fits. The power-law index α is given.

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