molecules:ism:h2o

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molecules:ism:h2o [2024/03/22 13:44] – muellermolecules:ism:h2o [2024/03/22 13:53] (current) – mueller
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 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\\ 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\\ detected in their investigation\\
-**[[https://doi.org/10.1051/0004-6361/202245193|ATOMIUM: Probing the inner wind of evolved O-rich stars +**[[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]]**\\
-with new, highly excited H<sub>2</sub>O and OH lines]]**\\+
 //Astron. Astrophys.// **674**, Art. No. A125 (2023)\\ //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.\\ 
 +\\
  
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