False-color view of the X-ray emission from the central part of the Virgo cluster.
This image is centered on M87. The second brightest
X-ray source in the upper right is M86, which
traverses the hot intergalactic medium at high peculiar velocity, and thus causes
heavy interaction; due to this effect, it has a comet-like shape.
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Identify the Galaxies on our Virgo Cluster optical image
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Compare the visual and X-ray appearance of the Virgo cluster
Last Modification: 18 Mar 1998, 20:45 MET