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molecules:ism:hc_ns [2022/11/17 11:51] – mueller | molecules:ism:hc_ns [2022/11/17 12:59] (current) – mueller | ||
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//Astron. Astrophys.// | //Astron. Astrophys.// | ||
The ethenthionyl radical, HCCS, was identified through 2 < | The ethenthionyl radical, HCCS, was identified through 2 < | ||
+ | \\ | ||
+ | R. Fuentetaja, M. Agúndez, C. Cabezas, B. Tercero, N. Marcelino, J. R. Pardo, P. de Vicente, and J. Cernicharo\\ | ||
+ | reported on\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | Butatrienethionyl was detected through six consecutive transitions with 19/2 ≤ //J"// ≤ 29/2 between 31.0 and 50.3 GHz in the course of a molecular line survey of the prototypical cold dark molecular cloud TMC-1 carried out with the Yebes 40 m radio telescope. The column densities of HCS and HCCS are about factors of 58 and 7.2, respectively, | ||
+ | \\ | ||