A comprehensive catalogue of high-mass X-ray binaries in the Large Magellanic Cloud detected during the first eROSITA all-sky survey

Open Access

Fig. 21

eROSITA spectra of the Gamma-ray binary CXOU J053600.0−673507 merged over all eRASS like Fig. 17. The dark yellow curve shows the best-fit model for the source (absorbed power law). The blue curve and shaded area show the best fit for a sum of particle background and a

vapec

model for the SNR contribution in the on-region. The background spectrum is dominated by the SNR emission up to ∼2 keV, where the particle background takes over. The black curve and shaded area are the sum of the source and background models.

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