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Intermediate-mass black hole
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An intermediate-mass black hole (IMBH) is a class of black hole with mass in the range of 100 to 100,000 (102–105) solar masses: significantly higher than stellar black holes but lower than the hundred thousand to more than one billion (105–109) solar mass supermassive black holes. Several IMBH candidate objects have been discovered in the Milky Way galaxy and others nearby, based on indirect gas cloud velocity and accretion disk spectra observations of various evidentiary strength.
