Massive black holes interactions during the assembly of heavy sub-structures in the centre of galaxy clusters
Abstract
We performed a series of direct N-body simulations with the aim to follow the dynamical evolution of a galaxy cluster (GC) (Mclus 1014 M) in different environment. The results show the formation of heavy sub-structures in the cluster centre in consequence of multiple merging among the innermost galaxies. Moreover we investigate the dynamics of super-massive black holes (SMBHs) residing in the centre of galaxies that form the most massive sub-structure.
0
Turn this paper into a lesson
ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.