Gaia data enables high-accuracy kinematic studies of nearby stellar groups, galactic rotation, spiral arms, the Radcliffe wave, and vertical phase spirals, including checks for similar waves elsewhere.
However, no significant peri odic perturbations of vertical coordinates and veloci ties characteristic of the Radcliffe wave were found in this structure
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Search for galactic structures and study of their kinematics in the Gaia era
Gaia data enables high-accuracy kinematic studies of nearby stellar groups, galactic rotation, spiral arms, the Radcliffe wave, and vertical phase spirals, including checks for similar waves elsewhere.