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molecules:ism:mec5n [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:mec5n [2019/04/24 16:19] – mueller | ||
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L. E. Snyder, T. L. Wilson, C. Henkel, P. R. Jewell, and C. M. Walmsley,\\ | L. E. Snyder, T. L. Wilson, C. Henkel, P. R. Jewell, and C. M. Walmsley,\\ | ||
**[[http:// | **[[http:// | ||
- | //Bull. Am. Atron. Soc.// **16**, 959 (1984).\\ | + | //Bull. Am. Astron. Soc.// **16**, 959 (1984).\\ |
Only three lines were detected, of which one apparently was blended. Therefore, this detection was deemed tentative. | Only three lines were detected, of which one apparently was blended. Therefore, this detection was deemed tentative. | ||
More recently, the 100 m GBT was used to detect the //J// = 12 – 11 to 16 – 15 transitions with //K// = 0 and 1 between 18.6 and 24.9 GHz in emission, also toward TMC-1, by\\ | More recently, the 100 m GBT was used to detect the //J// = 12 – 11 to 16 – 15 transitions with //K// = 0 and 1 between 18.6 and 24.9 GHz in emission, also toward TMC-1, by\\ | ||
L. E. Snyder, J. M. Hollis, P. R. Jewell, F. J. Lovas, and A. Remijan,\\ | L. E. Snyder, J. M. Hollis, P. R. Jewell, F. J. Lovas, and A. Remijan,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||