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Tracing Intermediate-Mass Black Holes in the Galactic Centre
Published online by Cambridge University Press: 01 September 2007
Abstract
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We have developed a new method for post-Newtonian, high-precision integration of stellar systems containing a super-massive black hole (SMBH), splitting the forces on a particle between a dominant central force and perturbations. We used this method to perform fully collisional N-body simulations of inspiralling intermediate-mass black holes (IMBHs) in the centre of the Milky Way.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 3 , Symposium S246: Dynamical Evolution of Dense Stellar Systems , September 2007 , pp. 367 - 368
- Copyright
- Copyright © International Astronomical Union 2008