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 Calcium Isocyanide, CaNC, toward CW Leonis ===== J. Cernicharo, L. Velilla-Prieto, M. Agúndez, J. R. Pardo, J. P. Fonfría, G. Quintana-Lacaci, C. Cabezas, C. Bermúdez, and M. Guélin\\ reported on the\\ **[[https://doi.org/10.1051/0004-6361/201936040|Discovery of the First Ca-bearing molecule in Space: CaNC]]**\\ //Astron. Astrophys.// **627**, Art. No. L4 (2019).\\ Nine rotational transitions with //N// = 9 − 8 to 21 − 20 were observed in emission between 72.8 and 169.9 GHz using the IRAM 30 m telecope. One transition is severely blended, a few others slightly to considerably. In addition, the signal-to-noise ratio is poor for some transitions, but reasonable for many. All transitions display fine structure splitting, and each of the FS components has U-shape typical for envelope species. The molecule is about 60 times less abundant than the lighter homolog MgNC and about similar abundant as FeCN in this source.\\ ---- Contributor(s): H. S. P. Müller; 07, 2019 ---- molecules/ism/canc.txt Last modified: 2019/07/09 16:33by mueller