molecules:extragalactic:methylformiat

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Next revision
Previous revision
molecules:extragalactic:methylformiat [2022/01/04 13:57] – created muellermolecules:extragalactic:methylformiat [2022/01/04 14:34] (current) mueller
Line 1: Line 1:
 ===== On Methyl Formate in Extragalactic Sources ===== ===== On Methyl Formate in Extragalactic Sources =====
  
-M. Sewiło, S. B. Charnley, PSchilke, V. Taquet, J. M. Oliveira, T. Shimonishi, E. Wirström, R. Indebetouw, J. L. Ward, JThvan Loon, J. Wiseman, SZahorecz, T. Onishi, A. Kawamura, C.-H. R. ChenYFukui, and RH. Golshan,\\+M. Sewiło, R. Indebetouw, S. B. Charnley, SZahorecz, J. M. Oliveira, J. T. van Loon, J. L. Ward, C.-HR. Chen, J. Wiseman, YFukui, A. Kawamura, MMeixnerTOnishi, and PSchilke\\
 reported on\\ 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.1641301025.txt.gz
  • Last modified: 2022/01/04 13:57
  • by mueller