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Fig. 3
X-ray emission (0.2–1 keV) of NGC 4388, together with an optical B band image (upper panel) and the Hi map from Oosterloo & van Gorkom (2005; lower panel). The X-ray map was cut at the position, where contribution from the M 86 halo starts to dominate. The first greyscale corresponds to 7 times the rms noise level.
This figure is made of several images, please see below:
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