  The first VLBI images of water maser emission in the Circinus Galaxy AGN show
both an accretion disk and outflow 0.1 to 1 pc from the central engine. The
maser traces a warped, edge-on accretion disk between radii of about 0.1 and
0.4 pc that is bound by a 1.3x10^6 Msun central mass. The rotation curve is
somewhat flatter than a Keplerian rotation law and is consistent with a disk
mass on the order of 10^5 Msun. Clumpy substructure may display a kinematic
signature consistent with spiral arms. Away from the disk, a second population
of water masers traces broadly a bipolar, wide-angle outflow that contains
(bullet-like) clumps ejected from a region centered on the central engine and
<0.1 pc in radius. Out to a radius of about 0.4 pc, the warp of the accretion
disk appears to channel the outflow, the orientation of which on the sky
coincides with the orientation of the known kiloparsec-scale ionization cone.
Beyond this radius, the flow crosses the disk and truncates it. This suggests
that the current accretion event and associated disk-outflow geometry have a
lifetime on the order of 10^7 years.
