Star Cluster Migration Near the Galactic Center
2009 ◽
Vol 5
(S267)
◽
pp. 329-329
Keyword(s):
AbstractWe performed a self-consistent N-body simulation of star clusters in the Galactic center (GC), taking into account the collisions of stars and formation of an intermediate-mass black hole (IMBH). We find that if an IMBH forms in the cluster, it carries young stars to the GC by a 1:1 resonance.
2007 ◽
Vol 3
(S246)
◽
pp. 467-468
Keyword(s):
2021 ◽
Vol 502
(2)
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pp. 2049-2064
Keyword(s):
2007 ◽
Vol 3
(S245)
◽
pp. 259-260
Keyword(s):
2007 ◽
Vol 3
(S246)
◽
pp. 256-260
Keyword(s):
Keyword(s):
2015 ◽
Vol 12
(S316)
◽
pp. 240-245
Keyword(s):
2014 ◽
Vol 10
(S312)
◽
pp. 213-222