First study of the supernova remnant population in the Large Magellanic Cloud with eROSITA - II. Spectral analysis and X-ray luminosity function

Open Access

Fig. 2

Histogram of the luminosity and flux in the energy band of 0.38.0 keV for the SNRs and SNR candidates in the LMC. The solid red line shows the best fit of the distribution with the dashed lines indicating the two Gaussian components of the best fit.

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