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- W2129691360 abstract "Abstract Massive black holes (MBHs) with a mass below ~ 10 7 M ⊙ are likely to reside at the centre of dense stellar nuclei shaped by 2-body relaxation, close interactions with the MBH and direct collisions. In this contribution, we stress the role of mass segregation of stellar-mass black holes into the innermost tenths of a parsec and point to the importance of hydrodynamical collisions between stars. At the Galactic centre, collisions must affect giant stars and some of the S-stars." @default.
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- W2129691360 date "2007-07-01" @default.
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- W2129691360 title "Dynamics of galactic nuclei: mass segregation and collisions" @default.
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- W2129691360 doi "https://doi.org/10.1017/s1743921308017675" @default.
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