{
  "id": "0909.2906",
  "version": "v1",
  "published": "2009-09-16T02:24:34.000Z",
  "updated": "2009-09-16T02:24:34.000Z",
  "title": "Tracing the Bipolar Outflow from Orion Source I",
  "authors": [
    "R. L. Plambeck",
    "M. C. H. Wright",
    "D. N. Friedel",
    "S. L. Widicus Weaver",
    "A. D. Bolatto",
    "M. W. Pound",
    "D. P. Woody",
    "J. W. Lamb",
    "S. L. Scott"
  ],
  "comment": "4 pages, 4 figures; accepted for publication in Ap J Letters",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "Using CARMA, we imaged the 87 GHz SiO v=0 J=2-1 line toward Orion-KL with 0.45 arcsec angular resolution. The maps indicate that radio source I drives a bipolar outflow into the surrounding molecular cloud along a NE--SW axis, in agreement with the model of Greenhill et al. (2004). The extended high velocity outflow from Orion-KL appears to be a continuation of this compact outflow. High velocity gas extends farthest along a NW--SE axis, suggesting that the outflow direction changes on time scales of a few hundred years.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2009-09-16T02:24:34.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "bipolar outflow",
      "orion source",
      "high velocity gas extends farthest",
      "arcsec angular resolution",
      "extended high velocity outflow"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1088/0004-637X/704/1/L25",
      "journal": "The Astrophysical Journal",
      "year": 2009,
      "month": "Oct",
      "volume": 704,
      "number": 1
    },
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 831391,
      "adsabs": "2009ApJ...704L..25P"
    }
  }
}