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--- molecules:ism:hac [2019/04/26 15:41] – mueller
+++ molecules:ism:hac [2020/12/05 12:39] (current) – mueller
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 //Astrophys. J.// **576**, 264–273 (2002).
+J. K. Jørgensen, M. H. D. van der Wiel, A. Coutens, J. M. Lykke, H. S. P. Müller, E. F. van Dishoeck, H. Calcutt, P. Bjerkeli, T. L. Bourke, M. N. Drozdovskaya, C. Favre, E. C. Fayolle, R. T. Garrod, S. K. Jacobsen, K. I. Öberg, M. V. Persson, and S. F. Wampfler\\
+reported on\\
+**[[https://doi.org/10.1051/0004-6361/201628648|The ALMA Protostellar Interferometric Line Survey (PILS): First Results from an Unbiased Submillimeter Wavelength Line Survey of the Class 0 Protostellar Binary IRAS 16293–2422 with ALMA]]**,\\
+//Astron. Astrophys.// **595**, Art. No. A117 (2016).\\
+The authors report the first unambiguous detection of acetic acid around a low-mass protostar. There were earlier tentative reports.\\
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+C. Xue, A. J. Remijan, C. L. Brogan, T. R. Hunter, E. Herbst, and B. A. McGuire\\
+reported on\\
+**[[https://doi.org/10.3847/1538-4357/ab32e0|ALMA Detection of Vibrationally Excited (//v//<sub>t</sub> = 1, 2) Acetic Acid toward NGC 6334I]]**,\\
+//Astrophys. J.// **882**, Art. No. 118 (2019).\\
+Unfortunately, the authors do not presen their model for the ground vibrational state.\\
-Contributor(s): H. S. P. Müller; 2002.
+----
+Contributor(s): H. S. P. Müller; 2002; 06, 2019; 12, 2020.
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