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+ | The identification was made by stacking data from the line survey up to 30 GHz; most signal-contribution came from the 13.1 to 19.2 GHz region. The authors also report a tentative detection of C< | ||
+ | \\ | ||
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+ | More recently,\\ | ||
+ | J. R. Pardo, C. Cabezas, M. Agúndez, B. Tercero, N. Marcelino, P. de Vicente, M. Guélin, and J. Cernicharo\\ | ||
+ | found\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | This time around, the molecule was identified in 15 not or not strongly blended transitions with 51 ≤ //J// ≤ 71 between 31 and 43 GHz in the course of a molecular line survey of the famous carbon rich AGB star CW Leonis carried out with the Yebes 40 m radio telescope.\\ | ||
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