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--- molecules:extragalactic:methylformiat [2022/01/04 13:59] – mueller
+++ molecules:extragalactic:methylformiat [2022/01/04 14:34] (current) – mueller
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 ===== On Methyl Formate in Extragalactic Sources =====
-M. Sewiło, S. B. Charnley, P. Schilke, V. Taquet, J. M. Oliveira, T. Shimonishi, E. Wirström, R. Indebetouw, J. L. Ward, J. Th. van Loon, J. Wiseman, S. Zahorecz, T. Onishi, A. Kawamura, C.-H. R. Chen, Y. Fukui, and R. H. Golshan,\\
+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/10.1021/acsearthspacechem.9b00065|Complex Organic Molecules in Star-Forming Regions of the
+**[[https://doi.org/10.3847/2041-8213/aaa079|The Detection of Hot Cores and Complex Organic Molecules
-Magellanic Clouds]]**\\
+in the Large Magellanic Cloud]]**\\
-//ACS Earth Space Chem.// **3**, (2019) 2088−2109.\\
+//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.\\
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+Contributor(s): H. S. P. Müller; 01, 2022
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