{
  "id": "0907.3031",
  "version": "v1",
  "published": "2009-07-17T09:57:03.000Z",
  "updated": "2009-07-17T09:57:03.000Z",
  "title": "Evidence of triggered star formation in G327.3-0.6. Dust-continuum mapping of an infrared dark cloud with P-ArTéMiS",
  "authors": [
    "V. Minier",
    "Ph. André",
    "P. Bergman",
    "F. Motte",
    "F. Wyrowski",
    "J. Le Pennec",
    "L. Rodriguez",
    "O. Boulade",
    "E. Doumayrou",
    "D. Dubreuil",
    "P. Gallais",
    "G. Hamon",
    "P. -O. Lagage",
    "M. Lortholary",
    "J. Martignac",
    "V. Revéret",
    "H. Roussel",
    "M. Talvard",
    "G. Willmann",
    "H. Olofsson"
  ],
  "comment": "4 pages",
  "journal": "Astronomy and Astrophysics 501 (2009) L1-L4",
  "doi": "10.1051/0004-6361/200912308",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "Aims. Expanding HII regions and propagating shocks are common in the environment of young high-mass star-forming complexes. They can compress a pre-existing molecular cloud and trigger the formation of dense cores. We investigate whether these phenomena can explain the formation of high-mass protostars within an infrared dark cloud located at the position of G327.3-0.6 in the Galactic plane, in between two large infrared bubbles and two HII regions. Methods: The region of G327.3-0.6 was imaged at 450 ? m with the CEA P-ArT\\'eMiS bolometer array on the Atacama Pathfinder EXperiment telescope in Chile. APEX/LABOCA and APEX-2A, and Spitzer/IRAC and MIPS archives data were used in this study. Results: Ten massive cores were detected in the P-ArT\\'eMiS image, embedded within the infrared dark cloud seen in absorption at both 8 and 24 ?m. Their luminosities and masses indicate that they form high-mass stars. The kinematical study of the region suggests that the infrared bubbles expand toward the infrared dark cloud. Conclusions: Under the influence of expanding bubbles, star formation occurs in the infrared dark areas at the border of HII regions and infrared bubbles.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2009-07-17T09:57:03.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "infrared dark cloud",
      "triggered star formation",
      "dust-continuum mapping",
      "hii regions",
      "infrared bubbles"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "journal": "Astronomy and Astrophysics",
      "year": 2009,
      "month": "Jul",
      "volume": 501,
      "number": 1
    },
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 825997,
      "adsabs": "2009A&A...501L...1M"
    }
  }
}