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Abstract In this paper, we address the question of how a central intermediate-mass black hole (IMBH) in a globular cluster (GC) affects dynamics, core collapse, and formation of the binary… Click to show full abstract
Abstract In this paper, we address the question of how a central intermediate-mass black hole (IMBH) in a globular cluster (GC) affects dynamics, core collapse, and formation of the binary population. It is shown that the central IMBH forms a binary system that affects dynamics of stars in the cluster significantly. The presence of an intermediate-mass black hole with mass ≥ 1.0-1.7%of the total stellar mass in the cluster inhibits the formation of binary stars population.
Keywords:
intermediate mass;
black hole;
mass;
mass black;
cluster
Journal Title: Open Astronomy
Year Published: 2018
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Journal Title: Open Astronomy
Year Published: 2018
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!