{
  "id": "astro-ph/9311045",
  "version": "v2",
  "published": "1993-11-18T13:00:42.000Z",
  "updated": "1993-11-19T10:04:41.000Z",
  "title": "Gravitational microlensing by the dark halo of M31",
  "authors": [
    "Philippe Jetzer"
  ],
  "comment": "4, latex, ZU-TH 27/93",
  "categories": [
    "astro-ph"
  ],
  "abstract": "It has been shown by Paczy\\'nski that gravitational microlensing is potentially a useful method for detecting the dark constituents of the halo of our galaxy, if their mass lies in the approximate domain $10^{-6}<M/M_\\odot<10^{-1}$. Microlensing observations now im progress monitor several millions of stars in the Large Magellanic Cloud and in the Galactic Bulge. Here I discuss the main features of the microlensing events: in particular their rates and probability.",
  "revisions": [
    {
      "version": "v2",
      "updated": "1993-11-19T10:04:41.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "dark halo",
      "gravitational microlensing",
      "large magellanic cloud",
      "im progress monitor",
      "dark constituents"
    ],
    "note": {
      "typesetting": "LaTeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 358293
    }
  }
}