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- W3126000350 abstract "NBody realizations of axisymmetric collisional galaxy cores (e.g. M32, M33, NGC205, Milky Way) with embedded growing black holes are presented. Stars which approach the disruption sphere are disrupted and accreted to the black hole. We measure the zone of influence of the black hole and disruption rates in relaxation time scales. We show that secular gravitational instabilities dominate the initial core dynamics, while the black hole is small and growing due to consumption of stars. Later, the black hole potential dominates the core, and loss cone theory can be applied. Our simulations show that central rotation in galaxies can not be neglected for relaxed systems, and compare and discuss our results with the standard theory of spherically symmetric systems." @default.
- W3126000350 created "2021-02-01" @default.
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- W3126000350 creator A5068014665 @default.
- W3126000350 creator A5086810336 @default.
- W3126000350 date "2011-10-20" @default.
- W3126000350 modified "2023-10-01" @default.
- W3126000350 title "Evolution of growing black holes in axisymmetric galaxy cores" @default.
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- W3126000350 doi "https://doi.org/10.1111/j.1365-2966.2011.19670.x" @default.
- W3126000350 hasPublicationYear "2011" @default.
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