  We find strong evidence for outflows originating in the dense molecular core
NGC 6334 I(North): a 1000 Msol molecular core distinguished by its lack of HII
regions and mid-IR emission. New observations were obtained of the SiO 2-1 and
5-4 lines with the SEST 15-m telescope and the H2 (1-0) S(1) line with the ESO
2.2-m telescope. The line profiles of the SiO transitions show broad wings
extending from -50 to 40 km/s, and spatial maps of the line wing emission
exhibit a bipolar morphology with the peaks of the red and blue wing separated
by 30". The estimated mass loss rate of the outflow is comparable to those for
young intermediate to high-mass stars. The near-IR images show eight knots of
H2 emission. Five of the knots form a linear chain which is displaced from the
axis of the SiO outflow; these knots may trace shock excited gas along the path
of a second, highly collimated outflow. We propose that I(N) is a rare example
of a molecular core in an early stage of cluster formation.
