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C. L. Joseph, D. Merritt, R. Olling, M. Valluri (Rutgers)
Many physical processes associated with the formation and growth of supermassive black holes in galactic nuclei leave unique signatures in the stellar density and phase-space distributions. We report on the first attempts to use HST/STIS data to determine the mechanism responsible for the creation of the 3-billion solar mass black hole in the nucleus of M87.
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