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--- molecules:ism:po [2024/08/21 16:20] – mueller
+++ molecules:ism:po [2024/08/21 16:33] (current) – mueller
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+S. H. J. Wallström, T. Danilovich, H. S. P. Müller, C. A. Gottlieb, S. Maes, M. Van de Sande, L. Decin, A. M. S. Richards, A. Baudry, J. Bolte, T. Ceulemans, F. De Ceuster, A. de Koter, I. El Mellah, M. Esseldeurs, S. Etoka, D. Gobrecht, E. Gottlieb, M. Gray, F. Herpin, M. Jeste, D. Kee, P. Kervella, T. Khouri, E. Lagadec, J. Malfait, L. Marinho, I. McDonald, K. M. Menten, T. J. Millar, M. Montargès, J. A. Nuth, J. M. C. Plane, R. Sahai, L. B. F. M. Waters, K. T. Wong, J. Yates, and A. Zijlstra\\
+reported on\\
+**[[https://doi.org/10.1051/0004-6361/202347632|ATOMIUM: Molecular Inventory of 17 Oxygen-rich Evolved Stars Observed with ALMA]]**\\
+//Astron. Astrophys.// **681**, Art. No. A50 (2024).\\
+The authors detect in their ALMA measurements in Band 6 vibrationally excited PO toward AH Sco, IRC+10011, IRC−10529,
+R Hya, and S Pav. The Ω = 3/2, //J// = 11/2 − 9/2, //F// = 6 − 5 and 5 − 4 lines near 239.9 GHz with unresolved Λ-doubling were detected near the //v// = 0, Ω = 1/2, //J// = 11/2 − 9/2, //F// = 6 − 5 and 5 − 4 //e//-lines near 240.0 GHz; the //f//-lines were not covered.\\
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