{
  "id": "astro-ph/9611080",
  "version": "v1",
  "published": "1996-11-11T16:40:44.000Z",
  "updated": "1996-11-11T16:40:44.000Z",
  "title": "Dark Matter",
  "authors": [
    "Neta Bahcall"
  ],
  "comment": "Figures can be obtained by e-mail to neta@astro.princeton.edu",
  "categories": [
    "astro-ph"
  ],
  "abstract": "Observations in the optical, in X-rays, and gravitational lensing of galaxies, clusters of galaxies, and large-scale structure are beginning to provide clues to the dark matter problem. I review the impact of these observations on some of the main questions relating to dark matter: How much dark matter is there? Where is it located? What is the nature of the dark matter? and what is the amount of baryonic dark matter.",
  "revisions": [
    {
      "version": "v1",
      "updated": "1996-11-11T16:40:44.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "baryonic dark matter",
      "dark matter problem",
      "large-scale structure",
      "observations",
      "gravitational"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 425826
    }
  }
}