{
  "id": "2208.11704",
  "version": "v1",
  "published": "2022-08-24T18:00:00.000Z",
  "updated": "2022-08-24T18:00:00.000Z",
  "title": "Weighing the Local Interstellar Medium using Gamma Rays and Dust",
  "authors": [
    "Axel Widmark",
    "Michael Korsmeier",
    "Tim Linden"
  ],
  "comment": "5 pages, 3 figures; appendix adds 16 pages, 9 figures; to be submitted to PRL, comments are welcome",
  "categories": [
    "astro-ph.GA",
    "astro-ph.HE"
  ],
  "abstract": "Cold gas forms a significant mass fraction of the Milky Way disk, but is its most uncertain baryonic component. The density and distribution of cold gas is of critical importance for Milky Way dynamics, as well as models of stellar and galactic evolution. Previous studies have used correlations between gas and dust to obtain high-resolution measurements of cold gas, but with large normalization uncertainties. We present a novel approach that uses Fermi-LAT $\\gamma$-ray data to measure the total gas density, achieving a similar precision as previous works, but with independent systematic uncertainties. Notably, our results have sufficient precision to distinguish between the tension in current world-leading experiments.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2022-08-24T18:00:00.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "local interstellar medium",
      "gamma rays",
      "independent systematic uncertainties",
      "milky way disk",
      "uncertain baryonic component"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 5,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}