论文标题
Radcliffe Wave的最小解释解释：开尔文 - 霍尔姆尔兹不稳定性
A minimum-hypothesis explanation for the Radcliffe Wave: Kelvin-Helmholtz instability
论文作者
论文摘要
有人建议，最近发现的2.7千摩尔巴索克在太阳街区的星际云的相干复合物（Radcliffe Wave）是kelvin-helmholtz的结果，这是基尔文 - 螺旋兹不稳定的结果，这是在银河系磁盘和非corotate Halo之间产生的。
It is suggested that the wavelike character of the recently discovered 2.7-kiloparsec spatially and kinematically coherent complex of interstellar clouds in the solar neighborhood--the Radcliffe Wave--may be the result of a Kelvin-Helmholtz instability arising at the interface between the Galactic disk and non-corotating halo.
