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A new search for insterstellar H2O absorption in the spectrum of Zeta OphiuchiIntensive Copernicus scans of the 1(11)-0(00) line of the F-X band of H2O were carried out, resulting in a 2 sigma upper limit of 1.04 mA for this line at 1114.225 A. The recently published f-value implies a column density limit of 5.3 x 10 to the 12th/sq cm, marginally above the level expected from recent chemical model calculations. A 1.8 sigma feature appears at the expected position of the H2O line, implying a column density for the ground rotational state of 2.8 x 10 to the 12th/sq cm.
Document ID
19820031707
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Snow, T. P., Jr.
(Colorado, University Boulder, CO, United States)
Smith, W. H.
(Washington University St. Louis, MO, United States)
Date Acquired
August 10, 2013
Publication Date
November 1, 1981
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
82A15242
Funding Number(s)
CONTRACT_GRANT: NSG-5246
CONTRACT_GRANT: NSG-5355
Distribution Limits
Public
Copyright
Other

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