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molecules:ism:cn-minus [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:cn-minus [2019/10/18 13:11] (current) – mueller | ||
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The cyanide ion has been detected with the IRAM 30 m telescope in the circumstellar shell of the carbon rich star CW Leo (IRC +10216) in 3 rotational transitions from //J// = 1 – 0 to 3 – 2 which occur between 110 and 340 GHz:\\ | The cyanide ion has been detected with the IRAM 30 m telescope in the circumstellar shell of the carbon rich star CW Leo (IRC +10216) in 3 rotational transitions from //J// = 1 – 0 to 3 – 2 which occur between 110 and 340 GHz:\\ | ||
M. Agúndez, J. Cernicharo, M. Guélin, C. Kahane, E. Roueff, J. Klos, F. J. Aoiz, F. Lique, N. Marceliño, J. R. Goicoechea, M. González García, C. A. Gottlieb, M. C. McCarthy, and P. Thaddeus,\\ | M. Agúndez, J. Cernicharo, M. Guélin, C. Kahane, E. Roueff, J. Klos, F. J. Aoiz, F. Lique, N. Marceliño, J. R. Goicoechea, M. González García, C. A. Gottlieb, M. C. McCarthy, and P. Thaddeus,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
It should be mentioned that the 1 – 0 transition is heavily blended with a line of C< | It should be mentioned that the 1 – 0 transition is heavily blended with a line of C< |