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| molecules:ism:h2ccn [2021/02/26 15:42] – mueller | molecules:ism:h2ccn [2021/02/26 15:50] (current) – mueller |
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| reported on the\\ | reported on the\\ |
| **[[https://doi.org/10.1051/0004-6361/202040210|Space and laboratory observation of the deuterated cyanomethyl radical HDCCN]]**\\ | **[[https://doi.org/10.1051/0004-6361/202040210|Space and laboratory observation of the deuterated cyanomethyl radical HDCCN]]**\\ |
| //Astron. Astrophys.// **646**, Art. No. L1 (2021). | //Astron. Astrophys.// **646**, Art. No. L1 (2021).\\ |
| | The 2<sub>02</sub> − 1<sub>01</sub> transition near 37.49 GHz with fine and hyperfine structure splitting was detected toward TMC-1 using the Yebes 40 m radio telescope in the course of a molecular line survey. The derived H<sub>2</sub>CCN to HDCCN ratio is 20 ± 4, i.e., ~40 per H atom, quite normal for TMC-1. |
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| Contributor(s): H. S. P. Müller; 12, 2003; 07, 2011 | Contributor(s): H. S. P. Müller; 12, 2003; 07, 2011; 02, 2021 |
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