{
  "id": "astro-ph/0207336",
  "version": "v1",
  "published": "2002-07-16T15:40:35.000Z",
  "updated": "2002-07-16T15:40:35.000Z",
  "title": "High Resolution 18 Micron Imaging of Hot Molecular Cores",
  "authors": [
    "James M. De Buizer"
  ],
  "comment": "7 pages, 5 figures, to appear in 'Galactic Star Formation Across the Stellar Mass Spectrum', eds. J.M. De Buizer & N.S. van der Bliek (ASP coference Series, 2002)",
  "categories": [
    "astro-ph"
  ],
  "abstract": "I present the latest results from a search for hot molecular cores at mid-infrared wavelengths from the largest optical telescopes available at the present time. Three well-observed hot molecular cores were imaged, G29.96-0.02, G19.61-0.23, and G34.26+0.15. Even though mid-infrared sources have been claimed to be detected previously at the hot molecular core locations of both G19.61-0.23 and G34.26+0.15, only the hot molecular core in G29.96-0.02 resulted in a detection. New upper limits on mid-infrared emission are given for the hot molecular cores that were not detected.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2002-07-16T15:40:35.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "high resolution",
      "micron imaging",
      "hot molecular core locations",
      "well-observed hot molecular cores",
      "largest optical telescopes"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 7,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 590599
    }
  }
}