{
  "id": "astro-ph/0207018",
  "version": "v1",
  "published": "2002-07-01T09:16:23.000Z",
  "updated": "2002-07-01T09:16:23.000Z",
  "title": "Radio Continuum Observations towards Optical and Molecular Outflows",
  "authors": [
    "J. M. Girart",
    "S. Curiel",
    "L. F. Rodriguez",
    "J. Canto"
  ],
  "comment": "17 pages, including 9 figures. Accepted for publication in RevMexAA, Vol. 38 no 2. (October 2002)",
  "categories": [
    "astro-ph"
  ],
  "abstract": "We present multi-frequency VLA continuum observations towards 8 star forming regions with molecular and optical outflows: L1489, HH 68-69, HH 94-95, NGC 2264D, L1681B, L778, MWC 1080 and V645 Cyg. We detect three thermal radio jets, L1489, YLW 16A in L1681B and NGC 2264D VLA 7, associated with molecular and/or HH outflows. The L1489 and NGC 2264D VLA 7 thermal radio jets appear elongated in the direction of the larger scale outflow. We report the first tentative detection of a non-thermal radio jet, L778 VLA 5, associated with a low mass Class I protostar and powering a molecular outflow. For HH68-69, HH 94-95 and the molecular outflow in NGC 2264D we could not identify a candidate of the exciting source of these outflows. The radio emission associated with V645 Cyg is quite extended, ~0.1 pc, and time variable. We detect three radio sources in the MWC 1080 that could be associated with YSOs.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2002-07-01T09:16:23.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "molecular outflow",
      "radio continuum observations",
      "ngc 2264d vla",
      "radio jets appear",
      "multi-frequency vla continuum observations"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 17,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 589542
    }
  }
}