The effect of gaseous accretion disk on dynamics of the stellar cluster
  in AGN
  There is a supermassive black hole, a gaseous accretion disk and compact star
cluster in the center of active galactic nuclei, as known today. So the
activity of AGN can be represented as the result of interaction of these three
subsystems. In this work we investigate the dynamical interaction of a central
star cluster surrounding a supermassive black hole and a central accretion
disk. The dissipative force acting on stars in the disk leads to an asymmetry
in the phase space distribution of the central star cluster due to the rotating
accretion disk. In our work we present some results of Stardisk model, where we
see some changes in density and phase space of central star cluster due to
influence of rotating gaseous accretion disk.
