{
  "id": "2106.13145",
  "version": "v1",
  "published": "2021-06-24T16:22:15.000Z",
  "updated": "2021-06-24T16:22:15.000Z",
  "title": "Modelling the chemical evolution of the Milky Way",
  "authors": [
    "Francesca Matteucci"
  ],
  "comment": "93 pages,37 figures. Accepted in Astronomy & Astrophysics Review",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "In this review I will discuss the comparison between model results and observational data for the Milky Way, the predictive power of such models as well as their limits. Such a comparison, known as Galactic archaeology, allows us to impose constraints on stellar nucleosynthesis and timescales of formation of the various Galactic components (halo, bulge, thick disk and thin disk).",
  "revisions": [
    {
      "version": "v1",
      "updated": "2021-06-24T16:22:15.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "milky way",
      "chemical evolution",
      "galactic archaeology",
      "comparison",
      "model results"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 93,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}