Accurate laboratory rest frequencies of vibrationally excited CO up to \(varv = 3\) and up to 2 THz

Astronomical observations of (sub)millimeter wavelength pure rotational emission lines of the second most abundant molecule in the Universe, CO, hold the promise of probing regions of high temperature and density in the innermost parts of circumstellar envelopes. The rotational spectrum of vibration...

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Bibliographic Details
Published in:arXiv.org 2009-02
Main Authors: Gendriesch, R, Lewen, F, Klapper, G, Menten, K M, Winnewisser, G, Coxon, J A, Müller, H S P
Format: Article
Language:English
Subjects:
Distortion
Excitation spectra
High temperature
Laboratories
Rotational spectra
Stellar envelopes
Universe
Online Access:Get full text
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Summary:Astronomical observations of (sub)millimeter wavelength pure rotational emission lines of the second most abundant molecule in the Universe, CO, hold the promise of probing regions of high temperature and density in the innermost parts of circumstellar envelopes. The rotational spectrum of vibrationally excited CO up to \(\varv = 3\) has been measured in the laboratory between 220 and 1940 GHz with relative accuracies up to \(5.2 \times 10^{-9}\), corresponding to \(\sim 5\) kHz near 1 THz. The rotational constant \(B\) and the quartic distortion parameter \(D\) have been determined with high accuracy and even the sextic distortion term \(H\) was determined quite well for \(\varv = 1\) while reasonable estimates of \(H\) were obtained for \(\varv = 2\) and 3. The present data set allows for the prediction of accurate rest frequencies of vibrationally excited CO well beyond 2 THz.
ISSN:2331-8422
DOI:10.48550/arxiv.0902.3382