{
  "id": "1309.4115",
  "version": "v2",
  "published": "2013-09-16T21:02:54.000Z",
  "updated": "2013-09-25T14:25:04.000Z",
  "title": "Pulsation and Mass Loss Across the HR Diagram: From OB stars to Cepheids to Red Supergiants",
  "authors": [
    "Hilding R. Neilson"
  ],
  "comment": "8 pages, 1 figure, review presented at IAU Symposium 301, Precision Asteroseismology, August 2013, Wroclaw, Poland, corrected errors in reference list",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "Both pulsation and mass loss are commonly observed in stars and are important ingredients for understanding stellar evolution and structure, especially for massive stars. There is a growing body of evidence that pulsation can also drive and enhance mass loss in massive stars and that pulsation-driven mass loss is important for stellar evolution. In this review, I will discuss recent advances in understanding pulsation driven mass loss in massive main sequence stars, classical Cepheids and red supergiants and present some challenges remaining.",
  "revisions": [
    {
      "version": "v2",
      "updated": "2013-09-25T14:25:04.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "red supergiants",
      "ob stars",
      "hr diagram",
      "stellar evolution",
      "understanding pulsation driven mass loss"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1017/S1743921313014336"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 8,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1254362,
      "adsabs": "2014IAUS..301..205N"
    }
  }
}