molecules:ism:h2o

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:h2o [2024/03/22 13:40] muellermolecules:ism:h2o [2024/03/22 13:53] (current) mueller
Line 61: Line 61:
 \\ \\
  
 +A. Baudry, K. T. Wong, S. Etoka, A. M. S. Richards, H. S. P. Müller, F. Herpin, T. Danilovich, M. D. Gray, S. Wallström, D. Gobrecht, T. Khouri, L. Decin, C. A. Gottlieb, K. M. Menten, W. Homan, T. J. Millar, M. Montargès, B. Pimpanuwat, J. M. C. Plane, and P. Kervella\\ 
 +detected in their investigation\\ 
 +**[[https://doi.org/10.1051/0004-6361/202245193|ATOMIUM: Probing the inner wind of evolved O-rich stars with new, highly excited H<sub>2</sub>O and OH lines]]**\\ 
 +//Astron. Astrophys.// **674**, Art. No. A125 (2023)\\ 
 +10 highly rotationally or vibrationally excited lines of H<sub>2</sub>O, of which 9 are new detections. The lines were obtained in selected ranges in the frequency region betweeb 222 and 269 GHz. Three of the lines involve the second triad, consisting of the states //v//<sub>2</sub> = //v//<sub>3</sub> = 1, //v//<sub>1</sub> = //v//<sub>2</sub> = 1, and //v//<sub>2</sub> = 3.\\ 
 +\\
  
 ---- ----
  • molecules/ism/h2o.1711111224.txt.gz
  • Last modified: 2024/03/22 13:40
  • by mueller