  We present ALMA band 6 images of the 12CO, 13CO and C18O J=2-1 line emissions
for the circumstellar disc around HD 169142, at ~8 au spatial resolution. We
resolve a central gas depleted cavity, along with two independent
near-symmetric ring-like structures in line emission: a well-defined inner gas
ring [~25 au] and a second relatively fainter and diffuse outer gas ring [~65
au]. We identify a localised super-Keplerian feature or vertical flow with a
magnitude of ~75m/s in the 12CO map. This feature has the shape of an arc that
spans azimuthally across a PA range of ~60 to 45 degrees and radially in
between the B1[26au] and B2[59au] dust rings. Through reconstruction of the gas
surface density profile, we find that the magnitude of the background
perturbations by the pressure support and self-gravity terms are not
significant enough to account for the kinematic excess. If of planetary origin,
the relative depletion in the gas-density profile would suggest a 1 Mj planet.
In contrast, the central cavity displays relatively smooth kinematics,
suggesting either a low mass companion and/or a binary orbit with a minimal
vertical velocity component.
