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 Methyl Formate in Extragalactic Sources ===== M. Sewiło, R. Indebetouw, S. B. Charnley, S. Zahorecz, J. M. Oliveira, J. T. van Loon, J. L. Ward, C.-H. R. Chen, J. Wiseman, Y. Fukui, A. Kawamura, M. Meixner, T. Onishi, and P. Schilke\\ reported on\\ **[[https://doi.org/10.3847/2041-8213/aaa079|The Detection of Hot Cores and Complex Organic Molecules in the Large Magellanic Cloud]]**\\ //Astrophys. J. Lett.// **853**, (2018) Art. No. L19.\\ ALMA was used at 1.3 mm to study the N 113 hot core region of the LMC. One line of methyl formate near 216.97 GHz was detected with reasonable signal-to-noise ratio toward the A1 peak and two more lines around 216.835 GHz look a bit too strong. The derived column density is about a factor of 15 lower than that of methanol.\\ ---- Contributor(s): H. S. P. Müller; 01, 2022 ---- molecules/extragalactic/methylformiat.txt Last modified: 2022/01/04 14:34by mueller