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--- molecules:ism:h2o [2024/03/22 13:06] – mueller
+++ molecules:ism:h2o [2024/03/22 13:44] – mueller
@@ Line 58: / Line 58: @@
 **[[https://doi.org/10.1051/0004-6361/201629838|An observational study of dust nucleation in Mira (o Ceti) — II. Titanium oxides are negligible for nucleation at high temperatures]]**\\
 //Astron. Astrophys.// **599**, Art. No. A59 (2017)\\
-the identification of highly rotationally and vibrationally excited lines of H<sub>2</sub>O, among them a formally ro-vibrational transition //v//<sub>1</sub> = 1 – //v//<sub>3</sub> = 1, 12<sub>3,9</sub> – 11<sub>5,6</sub>
+the identification of highly rotationally and vibrationally excited lines of H<sub>2</sub>O, among them a formally ro-vibrational transition //v//<sub>1</sub> = 1 – //v//<sub>3</sub> = 1, 12<sub>3,9</sub> – 11<sub>5,6</sub> near 345.67 GHz.\\
+\\
+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)\\
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