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High spectral and spatial resolution observations of the 12.28 micron emission from H2 in the Orion Molecular CloudThe pure rotational S(2) line of H2 at 12.28 microns was sought in 44 positions in the Orion Molecular Cloud with 6-arcsec beams and 35 km/s spectral resolution; and it was detected in 27 positions. The lines are approximately symmetric and have full widths at half-maximum ranging from 100 km/s down to the resolution limit. The distribution of intensities and line shapes is largely consistent with that observed in the 2-micron hydrogen transitions; however, unexpectedly complex line profiles and point-to-point variations in line shapes appear, particularly in the region near IRc9.
Document ID
19820043797
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Beck, S. C.
(Hawaii Univ. Honolulu, HI, United States)
Tokunaga, A. T.
(Hawaii, University Honolulu, HI, United States)
Bloemhof, E. E.
(Hawaii Univ. Honolulu, HI, United States)
Serabyn, E.
(Hawaii Univ. Honolulu, HI, United States)
Townes, C. H.
(Hawaii Univ. Honolulu, HI, United States)
Lacy, J. H.
(Hawaii Univ. Honolulu, HI, United States)
Smith, H. A.
(Hawaii Univ. Honolulu, HI, United States)
Date Acquired
August 10, 2013
Publication Date
February 15, 1982
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
82A27332
Funding Number(s)
CONTRACT_GRANT: NGL-05-003-272
CONTRACT_GRANT: NSF AST-78-24453
CONTRACT_GRANT: NASW-3159
Distribution Limits
Public
Copyright
Other

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