The Orientation of Accretion Disks Relative to Dust Disks in Radio   Galaxies
  We study the orientation of accretion disks, traced by the position angle of the jet, relative to the dust disk major axis in a sample of 20 nearby Radio Galaxies. We find that the observed distribution of angles between the jet and dust disk major axis is consistent with jets homogeneously distributed over a polar cap of 77 degrees. 
Henrique R. Schmitt (NRAO)