N-body simulation of a clumpy torus: application to active galactic nuclei
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/424/2/820/3229656/424-2-820.pdf
Reference40 articles.
1. Dynamical Evolution of Clusters of Galaxies, I
2. Gravitational N-Body Simulations
3. Unified Models for Active Galactic Nuclei and Quasars
4. A dipolar vortex model for the obscuring tori in active galactic nuclei
5. Gravitational potential of a homogeneous circular torus: a new approach
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1. Apparent counter-rotation in the torus of NGC 1068: influence of an asymmetric wind;Monthly Notices of the Royal Astronomical Society;2022-10-28
2. Dynamical model of an obscuring clumpy torus in AGNs – I. Velocity and velocity dispersion maps for interpretation of ALMA observations;Monthly Notices of the Royal Astronomical Society;2021-02-18
3. The Role of Infrared Radiation Pressure in Shaping Dusty Winds in AGNs;The Astrophysical Journal;2020-09-01
4. A surface integral approach to Poisson's equation and analytic expressions for the gravitational field of toroidal mass distributions;Applied Numerical Mathematics;2020-02
5. Interior potential of a toroidal shell from pole values;Monthly Notices of the Royal Astronomical Society;2019-05-04
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