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- W2028446236 abstract "We study the evolution of orbits of supermassive black holes in the nuclei of galaxies under the gravitational influence of the stars in the galaxy, as well as the cooling flow of gas into the black holes and their accretion discs. The number of supermassive black holes in the nucleus is increased by successive mergers of galaxies, while the number is decreased by mergers of black holes. We find that, typically, successive mergers create few black hole systems. We calculate the initial configurations of such systems, which allows one to estimate their further evolution. Many slingshot ejections of supermassive black holes result close to, or slightly above, the escape velocity from the galaxy." @default.
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- W2028446236 date "1996-01-01" @default.
- W2028446236 modified "2023-10-03" @default.
- W2028446236 title "Triple black hole systems formed in mergers of galaxies" @default.
- W2028446236 doi "https://doi.org/10.1093/mnras/278.1.186" @default.
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