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| molecules:ism:etoh [2019/04/25 13:38] – mueller | molecules:ism:etoh [2019/10/24 09:47] (current) – mueller |
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| Ethanol in its lowest //anti// configuration was among the early molecules to be detected in space. Its first detection was reported by:\\ | Ethanol in its lowest //anti// configuration was among the early molecules to be detected in space. Its first detection was reported by:\\ |
| B. Zuckerman, B. E. Turner, D. R. Johnson, F. O. Clark, F. J. Lovas, N. Fourikis, P. Palmer, M. Morris, A. E. Lilley, J. A. Ball, C. A. Gottlieb, and H. Penfield,\\ | B. Zuckerman, B. E. Turner, D. R. Johnson, F. O. Clark, F. J. Lovas, N. Fourikis, P. Palmer, M. Morris, A. E. Lilley, J. A. Ball, C. A. Gottlieb, and H. Penfield,\\ |
| **[[http://cdsads.u-strasbg.fr/abs/1975ApJ...196L..99Z|Detection of Interstellar //trans//-Ethyl Alcohol]]**\\ | **[[https://ui.adsabs.harvard.edu/abs/1975ApJ...196L..99Z|Detection of Interstellar //trans//-Ethyl Alcohol]]**\\ |
| //Astrophys. J.// **196**, L99–L102 (1975).\\ | //Astrophys. J.// **196**, L99–L102 (1975).\\ |
| Three //b//-type transitions (6<sub>06</sub> – 5<sub>15</sub>, 4<sub>14</sub> – 3<sub>03</sub>, and 5<sub>15</sub> – 4<sub>04</sub>) were detected with the 36-foot NRAO telescope in the 3 mm region toward the massive star-forming region Sagittarius B2(OH). Since then, //anti//-ethanol was detected in many massive star-forming regions, including W51M, G34.3+0.15, and Orion KL as well as other molecular clouds with somewhat elevated temperatures (around 100 K). | Three //b//-type transitions (6<sub>06</sub> – 5<sub>15</sub>, 4<sub>14</sub> – 3<sub>03</sub>, and 5<sub>15</sub> – 4<sub>04</sub>) were detected with the 36-foot NRAO telescope in the 3 mm region toward the massive star-forming region Sagittarius B2(OH). Since then, //anti//-ethanol was detected in many massive star-forming regions, including W51M, G34.3+0.15, and Orion KL as well as other molecular clouds with somewhat elevated temperatures (around 100 K). |
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| Contributor(s): H. S. P. Müller; 11, 2009; 07, 2012; 11, 2016; 01, 2019 | Contributor(s): H. S. P. Müller; 11, 2009; 07, 2012; 11, 2016; 01, 2019 |
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