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A new search for insterstellar H2O absorption in the spectrum of Zeta Ophiuchi

Authors :
Snow, T. P., Jr
Smith, W. H
Source :
Astrophysical Journal.
Publication Year :
1981
Publisher :
United States: NASA Center for Aerospace Information (CASI), 1981.

Abstract

Intensive 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.

Subjects

Subjects :
Astrophysics

Details

Language :
English
Database :
NASA Technical Reports
Journal :
Astrophysical Journal
Notes :
NSG-5246, , NSG-5355
Publication Type :
Report
Accession number :
edsnas.19820031707
Document Type :
Report
Full Text :
https://doi.org/10.1086/159358