Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ragt.meet..135n&link_type=abstract
In Proceedings of RAGtime 4/5 Workshops on black holes and neutron stars, 14-16/13-15 October 2002/2003, Eds: S. Hledík and Z. S
Astronomy and Astrophysics
Astrophysics
Monte Carlo, Numerical Simulations, Active Galactic Nuclei, Star Clusters, Clouds
Scientific paper
This article deals with the numerical simulations of the astrophysical systems located in the inner most parts of the galaxies - so called Active Galactic Nuclei (AGNs). Our simulation we are going to describe in this paper is treated in the Monte Carlo way and is used to solve the Fokker-Planck equation of our system to obtain its time evolution while taking into account all the relevant physical mechanisms involved in the system evolution. In the beginning of the paper we outline the system we would like to study in our simulations and then we summarise the physical ingredients involved in our model of the system. The largest part of the paper will be devoted to the description of the simulation method used to simulate a spherical star cluster as one part of the model of our system. Finally we present some results of such a simulation and draw an outline of the future prospects of our research.
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