  We report molecular line observations of the NGC 1333 IRAS 4C outflow in the
Perseus Molecular Cloud with the Atacama Large Millimeter/Submillimeter Array.
The CCH and CS emission reveal an outflow cavity structure with clear
signatures of rotation with respect to the outflow axis. The rotation is
detected from about 120 au up to about 1400 au above the envelope/disk
mid-plane. As the distance to the central source increases, the rotation
velocity of the outflow decreases while the outflow radius increases, which
gives a flat specific angular momentum distribution along the outflow. The mean
specific angular momentum of the outflow is about 100 au km/s. Based on
reasonable assumptions on the outward velocity of the outflow and the protostar
mass, we estimate the range of outflow launching radii to be 5-15 au. Such a
launching radius rules out that this outflow is launched as an X-wind, but
rather, it is more consistent to be a slow disk wind launched from relatively
large radii on the disk. The radius of the centrifugal barrier is roughly
estimated, and the role of the centrifugal barrier in the outflow launching is
discussed.
