GALAH+ is a magnitude-limited survey of high-resolution stellar spectra obtained by the HERMES spectrograph at the Australian Astronomical Observatory. Its third data release provides reduced spectra with new derivations of stellar parameters and abundances of 30 chemical elements for 584015 dwarfs and giants, 88 per cent of them in the Gaia magnitude range 11 < G 3 visits spanning more than a year. The combination of radial velocities from GALAH+ with distances and sky plane motions from Gaia enables studies of dynamics within streams and clusters. For example, we estimate that the open cluster M67 has a total mass of ~3300 M_{sun}_ and its outer parts seem to be expanding, though astrometry with a larger time-span than currently available from Gaia eDR3 is needed to judge if the latter result is real.

Cone search capability for table J/MNRAS/508/4202/table1 (*All RVs presented in this paper forming a value added catalogue of RVs of GALAH+ DR3)

Cone search capability for table J/MNRAS/508/4202/table2 (*List of 4483 stars with variable RV that exceed a 100 km/s)

Cone search capability for table J/MNRAS/508/4202/table3 (*List of 225 stars with constant RVs with at least N => 3 observations that span {Delat}t => 1yr in time and {Delta}RV < 0.2 km/s)