Abstract
We investigate with numerical Af-body integrations the time-evolution of stellar systems with centrally peaked density profiles harboring a massive black hole (galactic nuclei) or with varied initial conditions (such as rotation) using directintegration integrators. The computer programmes EUROSTAR and NBODY6++ developped for use with mpi libraries maintain high accuracy over billions of integration timesteps, allowing a detailed analysis of the orbit of the black hole(s), the precise diffusion of angular momentum between stars, and the ejection of stars from a cluster orbiting a host galaxy Below we consider each topic in turn.
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Hemsendorf, M., Baumgardt, H., Boily, C., Spurzem, R., Sigurdsson, S. (2002). Collisional Dynamics of Black Holes, Star Clusters and Galactic Nuclei. In: Krause, E., Jäger, W. (eds) High Performance Computing in Science and Engineering ’01. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-56034-7_5
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DOI: https://doi.org/10.1007/978-3-642-56034-7_5
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