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The central galaxy in this cluster harbors a supermassive black hole.
A similar argument applies to the growth of the central galaxy.
The erupting supermassive black hole is located in the central galaxy of NGC 5813.
A good example is IC 1101, the central galaxy in the cluster Abell 2029.
This X-ray emission extends outward from the central galaxy for at least 300,000 light years and shows that the known radio source is in the central galaxy of a massive cluster.
It is the collapse of cold gas that creates new stars, especially in the cluster's central galaxy.
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Astronomers, Dr. Fabian said, suspected that black holes in the central galaxies of clusters might be keeping the cluster gas hot, but the astronomers did not know how.
"We should see stars forming in central galaxies," said Dr. Kimberly Weaver, an astronomer at the Goddard Space Flight Center in Greenbelt, Md. But they do not, she said.
Solid lines indicate masses of central galaxies, while dashed lines indicate satellite galaxies.
This is particularly noticeable in the top-left panel for higher mass central galaxies, and is apparent in all panels for low mass satellite galaxies.
Several sources of heat have been discussed, most promising being heating by the SMBH in central galaxies through inflation of bubbles of relativistic plasma.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com