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| molecules:ism:hac [2019/10/24 09:38] – mueller | molecules:ism:hac [2020/12/05 12:39] (current) – mueller |
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| **[[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]]**,\\ | **[[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).\\ | //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. | 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.\\ |
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| Contributor(s): H. S. P. Müller; 2002; 06, 2019. | Contributor(s): H. S. P. Müller; 2002; 06, 2019; 12, 2020. |
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