High-Velocity Bipolar Molecular Emission from an AGN Torus
  We have detected in ALMA observations CO J = 6 - 5 emission from the nucleus of the Seyfert galaxy NGC 1068. The low-velocity (up to +/- 70 km/s relative to systemic) CO emission resolves into a 12x7 pc structure, roughly aligned with the nuclear radio source. Higher-velocity emission (up to +/- 400 km/s) is consistent with a bipolar outflow in a direction nearly perpendicular (roughly 80 degrees) to the nuclear disk. The position-velocity diagram shows that in addition to the outflow, the velocity field may also contain rotation about the disk axis. These observations provide compelling evidence in support of the disk-wind scenario for the AGN obscuring torus. 
Jack F. Gallimore, Moshe Elitzur, Roberto Maiolino, Alessandro   Marconi, Christopher P. O'Dea, Dieter Lutz, Stefi A. Baum, ...
astro-ph.GA