Abundance of carbon monoxide in the stratosphere of Titan from millimeter heterodyne observations
β Scribed by A. Marten; D. Gautier; L. Tanguy; A. Lecacheux; C. Rosolen; G. Paubert
- Publisher
- Elsevier Science
- Year
- 1988
- Tongue
- English
- Weight
- 350 KB
- Volume
- 76
- Category
- Article
- ISSN
- 0019-1035
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High sensitivity observations were performed at 1.2-and 3-mm wavelengths with the IRAM 30-m telescope (Spain) between April 1996 and December 1999 to investigate the nitrile composition of Titan's stratosphere. A part of our dataset consists of high resolution spectra of HC 14 N taken at 88.6 GHz as
A transient infrared spectrum observed following the photolysis of gas phase W (CO), in the presence of CO is shown to be due to internally excited W (CO): formed by the two-body recombination of W(CO)s and CO. The internal excitation is shown to be predominantly vibrational.