Star Cluster Migration Near the Galactic Center

Details Star Cluster Migration Near the Galactic Center Star Cluster Migration Near the Galactic Center

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..267..329f&link_type=abstract

Co-Evolution of Central Black Holes and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 267

Astronomy and Astrophysics

Astronomy

Galaxy: Center, Galaxy: Kinematics And Dynamics, Galaxies: Star Clusters

Scientific paper

We 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.

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