{
  "id": "2003.02315",
  "version": "v1",
  "published": "2020-03-04T20:14:28.000Z",
  "updated": "2020-03-04T20:14:28.000Z",
  "title": "A minimum-hypothesis explanation for the Radcliffe Wave: Kelvin-Helmholtz instability",
  "authors": [
    "Robert Fleck"
  ],
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "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.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2020-03-04T20:14:28.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "kelvin-helmholtz instability",
      "minimum-hypothesis explanation",
      "solar neighborhood-the radcliffe wave-may",
      "galactic disk",
      "interstellar clouds"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}