The eROSITA view of the Abell 3391/95 field: Case study from the Magneticum cosmological simulation

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

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Fig. 9

Same as Fig. 8, but only for the gas within R₂₀₀ for one of the member clusters, namely GC1 (upper panel) and for the gas in the bridge (lower panel) between the pair clusters, at z = 0.07. Dot-dashed lines mark the average temperature and overdensity values (mass-weighted estimate) of the selected gas.

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