{
  "id": "1409.6353",
  "version": "v1",
  "published": "2014-09-22T22:00:18.000Z",
  "updated": "2014-09-22T22:00:18.000Z",
  "title": "Spectropolarimetry of massive stars: Requirements and potential from today to 2030",
  "authors": [
    "G. A. Wade"
  ],
  "comment": "Proceedings of IAUS 307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We develop the requirements and potential of spectropolarimetry as applied to understanding the physics of massive stars during the immediate, intermediate-term and long-term future.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2014-09-22T22:00:18.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "massive stars",
      "spectropolarimetry",
      "requirements"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "adsabs": "2015IAUS..307..490W"
    }
  }
}