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Detection of absorption by H2 in molecular clouds: A direct measurement of the H2:CO ratioVibrational absorption by H2 and CO has been searched for toward infrared sources embedded in molecular clouds. H2 was detected toward NGC 2024 IRS 2 and possibly toward NGC 2264 (GL 989). CO was detected toward both sources. The results are consistent with the H2 ortho:para ratio being equilibrated at the cloud temperature. Toward NGC 2024, H2:CO = (3700(sub -2600)(sup +3100)) (2 sigma limits), and toward NGC 2264, H2:CO less than 6000. Approximately one-third of all carbon is in gas-phase CO.
Document ID
19950030300
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Lacy, J. H.
(Univ. of Texas, Austin, TX United States)
Knacke, R.
(Pennsylvania State Univ. Erie, PA, United States)
Geballe, T. R.
(Joint Astronomy Centre Hilo, HI, United States)
Tokunaga, A. T.
(Univ. of Hawaii, Honolulu, HI United States)
Date Acquired
August 16, 2013
Publication Date
June 20, 1994
Publication Information
Publication: The Astrophysical Journal
Volume: 428
Issue: 2, pt
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
95A61899
Distribution Limits
Public
Copyright
Other

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