  We report the detection of the Galactic nuclear disc in line-of-sight
kinematics of stars, measured with infrared spectroscopy from APOGEE. This
stellar component of the nuclear disc has an extent and rotation velocity V ~
120kms comparable to the gas disc in the central molecular zone. The current
data suggest that this disc is kinematically cool and has a small vertical
extent of order 50pc. The stellar kinematics suggest a truncation radius/steep
decline of the stellar disc at a galactocentric radius R ~ 150pc, and provide
tentative evidence for an overdensity at the position of the ring found in the
molecular gas disc.
