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**[[https:// | **[[https:// | ||
//Mon. Not. R. Astron. Soc.// **474**, 5068–5075 (2018); by\\ | //Mon. Not. R. Astron. Soc.// **474**, 5068–5075 (2018); by\\ | ||
- | A. M. Burkhardt, E. Herbst, S. V. Kalenskii, M. C. McCarthy, A. J. Remijan, and B. A. McGuire. | + | A. M. Burkhardt, E. Herbst, S. V. Kalenskii, M. C. McCarthy, A. J. Remijan, and B. A. McGuire.\\ |
+ | |||
+ | J. R. Pardo, C. Bermúdez, C. Cabezas, M. Agúndez, J. D. Gallego, J. P. Fonfría, L. Velilla-Prieto, | ||
+ | reported on the\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | The authors carried out an unbiased molecular line survey with the Yebes 40 m dish between 31 and 50 GHz toward the circumstellar envelope of the famous C-rich AGB star CW Leonis. Numerous transitions of HC< | ||
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- | Contributor(s): | + | Contributor(s): |
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