Differences
This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision | ||
molecules:extragalactic:methylformiat [2022/01/04 14:00] – mueller | molecules: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, 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:// | ||
+ | in the Large Magellanic Cloud]]**\\ | ||
+ | // | ||
+ | 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): | ||
+ | |||
+ | ---- | ||