Differences

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

--- molecules:ism:ch3oh [2026/02/09 12:14] – mueller
+++ molecules:ism:ch3oh [2026/04/13 12:16] (current) – mueller
@@ Line 112: / Line 112: @@
 //Astron. Astrophys.// **688**, Art. No. A201 (2023).\\
 The authors report a tentative detection of torsionally excited CH<sub>3</sub><sup>18</sup>OH in the ReExploring Molecular Complexity with ALMA survey at 3 mm besides several a clear identification of this isotopolog in its ground torsional state.\\
+\\
+=== (Far) Infrared Observations of Methanol ===
+S. L. Nickerson, N. Rangwala, K. Sung, X. Huang, E. J. Montiel, C. DeWitt, V. J. M. Le Gouellec, S. W. J. Colgan, J. Dittmann, J. P. Fonfría, G. M. Harper, K. E. Kraemer, J. Li, C. A. Nixon, M. F. Rashman, C. Sousa-Silva, A. G. G. M. Tielens, and W. D. Vacca\\
+announced\\
+**[[https://doi.org/10.3847/2041-8213/adf632|The Discovery of 25 μm Interstellar Methanol]]**\\
+//Astrophys. J. Lett. // **989**, Art. No. L51 (2025).\\
+More than 70 transitions were detected with EXES on board of SOFIA toward the massive protostar NGC 7538 IRS 1. Most of the transitions belong to the torsional overtone 2//v//<sub>12</sub>, some also to the torsional fundamental //v//<sub>12</sub>. The derived rotational temperature as well as the column density agree with submillimeter observations.\\
 \\
 ----
-Contributor(s): H. S. P. Müller; 04, 2022; 08, 2024; 02, 2026
+Contributor(s): H. S. P. Müller; 04, 2022; 08, 2024; 02, 2026; 04, 2026
 ----