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Comparative study between N-body and Fokker-Planck simulations for rotating star clusters - II. 2-component models
Jongsuk Hong, Eunhyeuk Kim, Hyung Mok Lee +1
To understand the effects of the initial rotation on the evolution of the tidally limited clusters with mass spectrum, we have performed N-body simulations of the clusters with dif…
Enhanced accretion rates of stars on Super-massive Black Holes by star-disk interactions in galactic nuclei
Andreas Just, Denis Yurin, Maxim Makukov +4
We investigate the dynamical interaction of a central star cluster surrounding a super-massive black hole and a central accretion disk. The dissipative force acting on stars in the…
Mergers of Unequal Mass Galaxies: Supermassive Black Hole Binary Evolution and Structure of Merger Remnants
Fazeel Mahmood Khan, Miguel Preto, Peter Berczik +3
Galaxy centers are residing places for Super Massive Black Holes (SMBHs). Galaxy mergers bring SMBHs close together to form gravitationally bound binary systems which, if able to c…
Interaction of Recoiling Supermassive Black Holes with Stars in Galactic Nuclei
Shuo Li, F. K. Liu, Peter Berczik +2
Supermassive black hole binaries (SMBHBs) are the products of frequent galaxy mergers. The coalescence of the SMBHBs is a distinct source of gravitational wave (GW) radiation. The…