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molecules:ism:h2o [2024/03/22 12:41] – mueller | molecules:ism:h2o [2024/03/22 13:53] (current) – mueller | ||
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the detection of the 6< | the detection of the 6< | ||
+ | \\ | ||
+ | |||
+ | T. Kamiński, H. S. P. Müller, M. R. Schmidt, I. Cherchneff, K. T. Wong, S. Brünken, K. M. Menten, J. M. Winters, C. A. Gottlieb, and N. A. Patel\\ | ||
+ | mentioned in their account on\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | the identification of highly rotationally and vibrationally excited lines of H< | ||
+ | \\ | ||
+ | |||
+ | 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:// | ||
+ | //Astron. Astrophys.// | ||
+ | 10 highly rotationally or vibrationally excited lines of H< | ||
\\ | \\ | ||