scholarly journals Evidence for an intermediate-mass black hole in the globular cluster NGC 6624

2017 ◽  
Vol 468 (2) ◽  
pp. 2114-2127 ◽  
Author(s):  
B. B. P. Perera ◽  
B. W. Stappers ◽  
A. G. Lyne ◽  
C. G. Bassa ◽  
I. Cognard ◽  
...  
2006 ◽  
Vol 371 (4) ◽  
pp. 1587-1593 ◽  
Author(s):  
K. K. Ghosh ◽  
V. Suleymanov ◽  
I. Bikmaev ◽  
S. Shimansky ◽  
N. Sakhibullin

2007 ◽  
Vol 661 (2) ◽  
pp. L151-L154 ◽  
Author(s):  
James S. Ulvestad ◽  
Jenny E. Greene ◽  
Luis C. Ho

2018 ◽  
Vol 27 (1) ◽  
pp. 1-6 ◽  
Author(s):  
Marina V. Ryabova ◽  
Alena S. Gorban ◽  
Yuri A. Shchekinov ◽  
Evgenii O. Vasiliev

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.


Nature ◽  
2017 ◽  
Vol 542 (7640) ◽  
pp. 203-205 ◽  
Author(s):  
Bülent Kızıltan ◽  
Holger Baumgardt ◽  
Abraham Loeb

2002 ◽  
Vol 124 (6) ◽  
pp. 3255-3269 ◽  
Author(s):  
Roeland P. van der Marel ◽  
Joris Gerssen ◽  
Puragra Guhathakurta ◽  
Ruth C. Peterson ◽  
Karl Gebhardt

2010 ◽  
Vol 712 (1) ◽  
pp. L1-L4 ◽  
Author(s):  
Jimmy A. Irwin ◽  
Thomas G. Brink ◽  
Joel N. Bregman ◽  
Timothy P. Roberts

2013 ◽  
Vol 554 ◽  
pp. A63 ◽  
Author(s):  
A. Feldmeier ◽  
N. Lützgendorf ◽  
N. Neumayer ◽  
M. Kissler-Patig ◽  
K. Gebhardt ◽  
...  

2011 ◽  
Vol 142 (4) ◽  
pp. 113 ◽  
Author(s):  
J. M. Wrobel ◽  
J. E. Greene ◽  
L. C. Ho

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