KhNU > Institute of Astronomy > Models > Active Galactic Nuclei

Dynamical model of an obscuring clumpy torus in AGNs: I. Velocity and velocity dispersion maps for interpretation of ALMA observations

  E.Yu. Bannikova, A.V. Sergeyev, N.A. Akerman, P.P. Berczik, M.V. Ishchenko, M. Capaccioli, V.S. Akhmetov


Torus evolution (N=128k, half-opening angle (θ=π/6))



Torus evolution (N=128k, half-opening angle (θ=π/4))



3D torus evolution for N=128k. Visualization is made using Glnemo