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The millimeter and submillimeter spectrum of CN in its first four vibrational states

Skatrud, David D. and De Lucia, Frank C. and Blake, Geoffrey A. and Sastry, K. V. L. N. (1983) The millimeter and submillimeter spectrum of CN in its first four vibrational states. Journal of Molecular Spectroscopy, 99 (1). pp. 35-46. ISSN 0022-2852. http://resolver.caltech.edu/CaltechAUTHORS:20120911-140831511

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Abstract

The rotational absorption frequencies of 65 new lines in the millimeter and submillimeter region of the spectrum have been measured for the CN radical in its ground electronic state. These measurements were made in a low pressure glow discharge of methane and nitrogen and include 25 lines from the v = 2 and v = 3 vibrational states, in addition to 40 lines from v = 0 and v = 1. The Dunham constants, as well as the spin-rotation and hyperfine constants of these four vibrational states, were calculated by means of a global nonlinear least squares fit of these data.


Item Type:Article
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http://dx.doi.org/10.1016/0022-2852(83)90290-4DOIUNSPECIFIED
http://www.sciencedirect.com/science/article/pii/0022285283902904PublisherUNSPECIFIED
Additional Information:© 1983 Academic Press. Inc. Received: November 15, 1982. Work Supported by: NASA Grant No. NAGW-189.
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Funding AgencyGrant Number
NASA NAGW-189
Record Number:CaltechAUTHORS:20120911-140831511
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20120911-140831511
Official Citation:David D. Skatrud, Frank C. De Lucia, Geoffrey A. Blake, K.V.L.N. Sastry, The millimeter and submillimeter spectrum of CN in its first four vibrational states, Journal of Molecular Spectroscopy, Volume 99, Issue 1, May 1983, Pages 35-46, ISSN 0022-2852, 10.1016/0022-2852(83)90290-4. (http://www.sciencedirect.com/science/article/pii/0022285283902904)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:34003
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:11 Sep 2012 21:22
Last Modified:11 Sep 2012 21:22

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