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Fig. 3.

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Location of the XRISM/Resolve measurements superimposed on a XMM-Newton/EPIC surface brightness map of the Coma cluster. The white squares show the footprint of the two Resolve pointings split into four individual quadrants, with the number showing the bulk velocity of each region with respect to the cluster rest frame. The blue arrows show the positions of the two dominant galaxies NGC 4874 and NGC 4889 with their respective peculiar velocities. Figure reproduced with modifications from X25.

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