{
  "id": "1706.01374",
  "version": "v1",
  "published": "2017-06-05T15:31:33.000Z",
  "updated": "2017-06-05T15:31:33.000Z",
  "title": "Self-consistent modelling of our Galaxy with Gaia data",
  "authors": [
    "James Binney"
  ],
  "comment": "8 pages, 1 figure to appear in proceedings of IAU Symposium 330, eds. Recio-Blanco, de Laverny & Brown",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "Galaxy models are fundamental to exploiting surveys of our Galaxy. There is now a significant body of work on axisymmetric models. A model can be defined by giving the DF of each major class of stars and of dark matter. Then the self-consistent gravitational potential is determined. Other modelling techniques are briefly considered before an overview of some early work on non-axisymmetric models.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2017-06-05T15:31:33.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "gaia data",
      "self-consistent modelling",
      "self-consistent gravitational potential",
      "non-axisymmetric models",
      "dark matter"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 8,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}