{
  "id": "1012.1626",
  "version": "v1",
  "published": "2010-12-07T22:01:35.000Z",
  "updated": "2010-12-07T22:01:35.000Z",
  "title": "The Radio-X-ray Relation in Cool Stars: Are we headed toward a divorce?",
  "authors": [
    "Jan Forbrich",
    "Scott J. Wolk",
    "Manuel Güdel",
    "Arnold Benz",
    "Rachel Osten",
    "Jeffrey L. Linsky",
    "Margaret McLean",
    "Laurent Loinard",
    "Edo Berger"
  ],
  "comment": "12 pages, Cool Stars 16 splinter session summary, to appear in conference proceedings",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "This Cool Stars 16 splinter session was devoted to reviewing our current knowledge of correlated X-ray and radio emission from cool stars in order to prepare for new large radio observatories such as the EVLA. A key interest was to discuss why the X-ray and radio luminosities of some cool stars are in clear breach of a correlation that holds for other active stars, the so-called G\\\"udel-Benz relation. This article summarizes the contributions whereas the actual presentations can be accessed on the splinter website (http://cxc.harvard.edu/cs16xrayradio/).",
  "revisions": [
    {
      "version": "v1",
      "updated": "2010-12-07T22:01:35.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "cool stars",
      "radio-x-ray relation",
      "large radio observatories",
      "splinter session",
      "radio emission"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 12,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 880060,
      "adsabs": "2011ASPC..448..455F"
    }
  }
}