A kinematic excess in the annular gap and gas-depleted cavity in the disc around HD 169142

We present ALMA band 6 images of the (CO)-C-12, (CO)-C-13, and (CO)-O-18 J = 2-1 line emissions for the circumstellar disc around HD 169142, at similar to 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 [similar to 25 au] and a second relatively fainter and diffuse outer gas ring [similar to 65 au]. We identify a localized super-Keplerian feature or vertical flow with a magnitude of similar to 75 ms(-1) in the (CO)-C-12 map. This feature has the shape of an arc that spans azimuthally across a position angle range of -60 degrees 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 M-J 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.