{
  "id": "1002.3433",
  "version": "v1",
  "published": "2010-02-18T06:33:14.000Z",
  "updated": "2010-02-18T06:33:14.000Z",
  "title": "High-resolution spectroscopy of the R Coronae Borealis and Other Hydrogen Deficient Stars",
  "authors": [
    "N. Kameswara Rao",
    "David L. Lambert"
  ],
  "comment": "16 pages, 9 figures, Astrophysics and Space Science Proceedings, Springer-Verlag, Berlin, 2010",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "High-resolution spectroscopy is a very important tool for studying stellar physics, perhaps, particularly so for such enigmatic objects like the R Coronae Borealis and related Hydrogen deficient stars that produce carbon dust in addition to their peculiar abundances. Examples of how high-resolution spectroscopy is used in the study of these stars to address the two major puzzles are presented: (i) How are such rare H-deficient stars created? and (ii) How and where are the obscuring soot clouds produced around the R Coronae Borealis stars?",
  "revisions": [
    {
      "version": "v1",
      "updated": "2010-02-18T06:33:14.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "high-resolution spectroscopy",
      "coronae borealis stars",
      "related hydrogen deficient stars",
      "produce carbon dust",
      "studying stellar physics"
    ],
    "publication": {
      "doi": "10.1007/978-3-642-10322-3_17",
      "journal": "Astrophysics and Space Science Proceedings",
      "year": 2010,
      "volume": 17,
      "pages": 177
    },
    "note": {
      "typesetting": "TeX",
      "pages": 16,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 846103,
      "adsabs": "2010ASSP...17..177R"
    }
  }
}