In N-body merger simulations, recoiling supermassive black holes escape major-merger remnants at velocities up to 25 percent lower than static analytical galaxy models predict, implying more spatially offset AGNs.
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Recoiling supermassive black holes in analytical and numerical galaxy potential
In N-body merger simulations, recoiling supermassive black holes escape major-merger remnants at velocities up to 25 percent lower than static analytical galaxy models predict, implying more spatially offset AGNs.