molecules:ism:ch3oh

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
molecules:ism:ch3oh [2026/04/13 12:02] muellermolecules:ism:ch3oh [2026/04/13 12:16] (current) mueller
Line 115: Line 115:
  
  
-=== (Far) Infrared observations of Methanol ===+=== (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\\ 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.\\
 +\\
  
 ---- ----
  • molecules/ism/ch3oh.1776074572.txt.gz
  • Last modified: 2026/04/13 12:02
  • by mueller