molecules:extragalactic:methylformiat

Differences

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

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
Last revisionBoth sides next revision
molecules:extragalactic:methylformiat [2022/01/04 14:09] muellermolecules:extragalactic:methylformiat [2022/01/04 14:31] mueller
Line 3: Line 3:
 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\\ 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\\ 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 around 216.835 GHz were close to the noise limit. 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 14:34
  • by mueller