First studies of the diffuse X-ray emission in the Large Magellanic Cloud with eROSITA

The Early Data Release of eROSITA and Mikhail Pavlinsky ART-XC on the SRG mission

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Fig. 13

N_H,LMC in the LMC obtained from the fit of the eROSITA spectra (left) vs. N_H.cold,LMC directly calculated from cold H I and dust (right) in cm^–2. Both images are shown in log-scale using the same lower and upper cuts. The contours of N_H,cold,LMC are plotted in both panels.

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