Show pageOld revisionsBacklinksBack to top This page is read only. You can view the source, but not change it. Ask your administrator if you think this is wrong. ===== On the Cyanate Radical, NCO, in the ISM ===== N. Marcelino, M. Agúndez, J. Cernicharo, E. Roueff, and M. Tafalla\\ reported on the\\ **[[https://doi.org/10.1051/0004-6361/201833074|Discovery of the Elusive Radical NCO and Confirmation of H<sub>2</sub>NCO<sup>+</sup> in Space]]**\\ //Astron. Astrophys.// **612**, Art. No. L10 (2018).\\ The cyanate (or isocyanate) radical was detected in the course of a 3 mm line survey of the dense core L483 toward the young stellar object IRAS 18148–0440 carried out with the IRAM 30 m telescope. Two Λ-components were detected in emission for each of the three strong hyperfine components of two transitions, //J// = 3.5 – 2.5 near 81.411 GHz and //J// = 4.5 – 3.5 near 104.67 GHz. The derived abundance is only about a factor of five lower than that of HNCO. ---- Contributor(s): H. S. P. Müller; 05, 2018 ---- molecules/ism/nco.txt Last modified: 2019/02/25 22:38by 127.0.0.1