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It is suggested that the wavelike character of the recently discovered2.7-kiloparsec spatially and kinematically coherent complex of interstellarclouds in the solar neighborhood--the Radcliffe Wave--may be the result of aKelvin-Helmholtz instability arising at the interface between the Galactic diskand non-corotating halo.

A minimum-hypothesis explanation for the Radcliffe Wave: Kelvin-Helmholtz instability