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.
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Kinematic study of 4003 open star clusters yields galactic rotation rates Ω0=28.99 km/s/kpc and |ΔΩ|=2.0 km/s/kpc, indicating the Sun lies close to corotation at 7.6 or 8.6 kpc.
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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.
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Analysis of spatial velocities of several samples of open star clusters
Kinematic study of 4003 open star clusters yields galactic rotation rates Ω0=28.99 km/s/kpc and |ΔΩ|=2.0 km/s/kpc, indicating the Sun lies close to corotation at 7.6 or 8.6 kpc.