Young star clusters tied to the Radcliffe wave exhibit vertical perturbations up to 200 pc persisting from 30 Myr ago through 20 Myr in the future, questioning the Parker instability scenario for the wave's formation.
Fleck, Nature 583, 24 (2020)
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A study of the spatial evolution of the Radcliffe wave in a sample of young open star clusters
Young star clusters tied to the Radcliffe wave exhibit vertical perturbations up to 200 pc persisting from 30 Myr ago through 20 Myr in the future, questioning the Parker instability scenario for the wave's formation.