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 Detection of Silyl Cyanide, SiH3CN, in Space ===== J. Cernicharo, M. Agúndez, L. Velilla Prieto, M. Guélin, J. R. Pardo, C. Kahane, C. Marka, C. Kramer, S. Navarro, G. Quintana-Lacaci, J. P. Fonfría, N. Marcelino, B. Tercero, E. Moreno, S. Massalkhi, M. Santander-García, M. C. McCarthy, C. A. Gottlieb, and J. L. Alonso\\ reported on the\\ **[[https://doi.org/10.1051/0004-6361/201731672|Discovery of Methyl Silane and Confirmation of Silyl Cyanide in IRC +10216]]**\\ //Astron. Astrophys.// **606**, Art. No. L5 (2017).\\ 6 sets of silyl cyanide, SiH<sub>3</sub>CN, transitions with //J'// between 9 and 17 (between 89 and 170 GHz) were detected with the IRAM 30 m telescope in emission toward the late-type C-rich star CW Leonis. The //K// level structure is partly resolved. At least some degree of blending by emission lines of other molecules is present. ---- Contributor(s): H. S. P. Müller; 10, 2017 ---- molecules/ism/sih3cn.txt Last modified: 2019/05/09 12:42by mueller