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A Self-Consistent Study of Triaxial Black-Hole Nuclei
ASTROPHYSICAL JOURNAL, no. 2 (2004): 774-787
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We construct models of triaxial galactic nuclei containing central black holes using the method of orbital superposition and then verify their stability by advancing N-body realizations of the models forward in time. We assume a power-law form for the stellar density, rho proportional to r(-gamma), with gamma=1 and 2; these values corresp...More
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