{
  "id": "1704.04616",
  "version": "v1",
  "published": "2017-04-15T10:13:12.000Z",
  "updated": "2017-04-15T10:13:12.000Z",
  "title": "Massive stars, successes and challenges",
  "authors": [
    "Georges Meynet",
    "André Maeder",
    "Cyril Georgy",
    "Sylvia Ekström",
    "Patrick Eggenberger",
    "Fabio Barblan",
    "Han Feng Song"
  ],
  "comment": "12 pages, 3 figures, IAU Symposium 329, The Lives and Death-Throes of Massive Stars, Auckland, 2016",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We give a brief overview of where we stand with respect to some old and new questions bearing on how massive stars evolve and end their lifetime. We focus on the following key points that are further discussed by other contributions during this conference: convection, mass losses, rotation, magnetic field and multiplicity. For purpose of clarity, each of these processes are discussed on its own but we have to keep in mind that they are all interacting between them offering a large variety of outputs, some of them still to be discovered.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2017-04-15T10:13:12.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "challenges",
      "large variety",
      "brief overview",
      "mass losses",
      "magnetic field"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 12,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}