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Paper: Dynamics of Globular Clusters with Intermediate-Mass Black Holes
Volume: 510, Stars: From Collapse to Collapse
Page: 496
Authors: Ryabova, M. V.; Shchekinov, Yu. A.; Vasiliev, E. O.
Abstract: Recent photometric and spectroscopic analysis of several Galactic globular clusters have shown that they may contain black holes of intermediate mass (around 1% of the cluster mass). Using N-body simulations we follow dynamical evolution of globular clusters in the presence of such an intermediate-mass black hole.
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