Some characteristic timescales in a numerical model of the central parts of active galactic nuclei

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A realistic number of particles in the simulations of the cental parts of active galactic nuclei (AGNs) remains a computational challenge. For this reason, we describe the timescales of the dynamic processes of our AGN model as a function of the number of particles.

Keywords: Active galactic nuclei; Stellar dynamics; Timescales

Document Type: Research Article


Affiliations: 1: Observatory, Fesenkov Astrophysical Institute, 050020, Almaty, Kazakhstan 2: Astronomisches Rechen-Institut, Mönchhofstrasse 12-14, 69120, Heidelberg, Germany

Publication date: August 1, 2005

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