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158 micron forbidden C II mapping of the Orion molecular cloudA fully sampled, 1000-point, 1-arcmin-resolution map of the inner 6.5 x 10 arcmin (alpha x delta) regions of the Orion Nebula in the 157.7409-micron forbidden fine-structure line is constructed. Large-scale strip maps in forbidden C II across the face of the Orion molecular cloud, and CO(17-16), (14-13), and (7-6) spectra are obtained at selected positions in the Orion H II region/molecular cloud interface. Strong forbidden C II line emission is observed across the face of the Orion molecular. The total forbidden C II luminosity from the Orion molecular cloud is about 1500 solar luminosities, or 0.3 percent of the FIR luminosity. The extended forbidden C II emission probably arises in either the UV-exposed surface of the molecular cloud or from the surfaces of UV-exposed clumps within the molecular cloud.
Document ID
19930041421
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Stacey, G. J.
(Cornell Univ. Ithaca, NY, United States)
Jaffe, D. T.
(Texas Univ. Austin, United States)
Geis, N.
(California Univ. Berkeley, United States)
Grenzel, R.
(NASA Ames Research Center Moffett Field, CA, United States)
Harris, A. I.
(NASA Ames Research Center Moffett Field, CA, United States)
Poglitsch, A.
(Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Stutzki, J.
(Koeln, Univ. Cologne, Germany)
Townes, C. H.
(California Univ. Berkeley, United States)
Date Acquired
August 16, 2013
Publication Date
February 10, 1993
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 404
Issue: 1
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
93A25418
Funding Number(s)
CONTRACT_GRANT: NAG2-208
Distribution Limits
Public
Copyright
Other

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