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 the Discovery of Methoxyethanol in the ISM ===== Z. T. P. Fried, S. J. El-Abd, B. M. Hays, G. Wenzel, A. N. Byrne, L. Margulès, R. A. Motiyenko, S. T. Shipman, M. P. Horne, J. K. Jørgensen, C. L. Brogan, T. R. Hunter, A. J. Remijan, A. Lipnicky, R. A. Loomis, and B. A. McGuire\\ described the\\ **[[https://doi.org/10.3847/2041-8213/ad37ff|Rotational Spectrum and First Interstellar Detection of 2-methoxyethanol Using ALMA Observations of NGC6334I]]**\\ //Astrophys. J. Lett.// **965**, Art. No. L23 (2024).\\ Methoxyethanol, CH<sub>3</sub>OCH<sub>2</sub>CH<sub>2</sub>OH, was detected toward the high mass star-forming region NGC 6334I in archival ALMA Band 4 data around 131 and around 145 GHz. An excitation temperature of ~140 K was derived with a methoxymethanol to methoxyethanol ratio of ~30. The molecules was not detected in archival Band 7 data of IRAS 16293−2422B with a lower limt of this ratio of > 56.\\ \\ ---- Contributor(s): H. S. P. Müller; 04, 2024 ---- molecules/ism/methoxyethanol.txt Last modified: 2024/04/29 12:28by mueller