  The first VLBI images of water maser emission in the Circinus Galaxy AGN show
both a warped, edge-on accretion disk and an outflow 0.1 to 1 pc from the
central engine. The inferred central mass is 1.3 million suns, while the disk
mass may be on the order of 0.1 million suns, based on a nearly Keplerian
rotation curve. The bipolar, wide-angle outflow appears to contain ``bullets''
ejected from within <0.1 pc of the central mass. The positions of filaments and
bullets observed in the AGN ionization cone on kpc-scales suggest that the disk
channels the flow to a radius of about 0.4 pc, at which the flow appears to
disrupt the disk.
