An artist’s impression of an accretion disk rotating around an unseen supermassive black hole. (IMAGE)
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An artist’s impression of an accretion disk rotating around an unseen supermassive black hole. The accretion process produces random fluctuations in luminosity from the disk over time, a pattern found to be related to the mass of the black hole in a new study led by University of Illinois Urbana-Champaign researchers.
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Graphic courtesy Mark A. Garlick/Simons Foundation
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