| Autor: |
Ryabova, Marina V., Gorban, Alena S., Shchekinov, Yuri A., Vasiliev, Evgenii O. |
| Předmět: |
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| Zdroj: |
Advances in Materials Science; Dec2018, Vol. 18 Issue 4, p1-6, 6p |
| Abstrakt: |
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. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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