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Laboratory and astronomical measurement of the millimeter wave spectrum of the ethynyl radical CCHThe N = 0 yields 1 and 1 yields 2 rotational transitions of CCH at 87 and 174 GHz, respectively, have been detected in a laboratory glow discharge in a mixture of He and C2H2. The spectroscopic constants of CCH derived from measurements of the hfs of the transitions agree well with those derived from astronomical observations, confirming the astronomical detection of CCH. As the CCH lines in the Orion Nebula are narrower than the laboratory lines but less certain in rest frequency owing to uncertainty in the radial velocity, the most accurate values for the spectroscopic constants of CCH are obtained from a simultaneous fit of both the laboratory and astronomical data. For the rotation, centrifugal distortion, spin-rotation, and hyperfine constants, respectively, the values found are within 0.006 of 43674.534 MHz, within 0.0008 of 0.1071 MHz, within 0.004 of -62.606 MHz, b = within 0.019 MHz of 40.426, and c is within 0.026 of 12.254 MHz.
Document ID
19830038302
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Gottlieb, C. A.
(NASA Goddard Inst. for Space Studies New York, NY, United States)
Gottlieb, E. W.
(NASA Goddard Inst. for Space Studies New York, NY, United States)
Thaddeus, P.
(NASA Goddard Institute for Space Studies; Columbia University New York, NY, United States)
Date Acquired
August 11, 2013
Publication Date
January 15, 1983
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
83A19520
Funding Number(s)
CONTRACT_GRANT: NSG-7105
CONTRACT_GRANT: NCC5-16
Distribution Limits
Public
Copyright
Other

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