molecules:ism:mex

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molecules:ism:mex [2020/09/18 15:31] – muellermolecules:ism:mex [2020/09/18 15:33] (current) – mueller
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 E. C. Fayolle, K. I. Öberg, J. K. Jørgensen, K. Altwegg, H. Calcutt, H. S. P. Müller, M. Rubin, M. H. D. van der Wiel, P. Bjerkeli, T. L. Bourke, A. Coutens, E. F. van Dishoeck, M. N. Drozdovskaya, R. T. Garrod, N. F. W. Ligterink, M. V. Persson, S. F. Wampfler, and the ROSINA team\\ E. C. Fayolle, K. I. Öberg, J. K. Jørgensen, K. Altwegg, H. Calcutt, H. S. P. Müller, M. Rubin, M. H. D. van der Wiel, P. Bjerkeli, T. L. Bourke, A. Coutens, E. F. van Dishoeck, M. N. Drozdovskaya, R. T. Garrod, N. F. W. Ligterink, M. V. Persson, S. F. Wampfler, and the ROSINA team\\
 reported on the\\ reported on the\\
-[[https://doi.org/2010.1038/s41550-017-0237-7|Protostellar and Cometary Detections of Organohalogens]]\\+[[https://doi.org/10.1038/s41550-017-0237-7|Protostellar and Cometary Detections of Organohalogens]]\\
 //Nat. Astron.// **1** (2017), 703–708.\\ //Nat. Astron.// **1** (2017), 703–708.\\
 The //J// = 13 – 12 transitions with //K// = 0 to 4 of methyl chloride, CH<sub>3</sub>Cl, were detected with ALMA near 345.4 and 340.1 GHz for the <sup>35</sup>Cl and <sup>37</sup>Cl isotopologs, respectively, in emission toward the Solar-type protostar IRAS 16293–2422B. CH<sub>3</sub><sup>35</sup>Cl was also seen toward the companion IRAS 16293–2422A. The <sup>35</sup>Cl/<sup>37</sup>Cl ratio is about 2.1, the same as observed for HCl in that source, but slightly lower than 3.13 on Earth.\\ The //J// = 13 – 12 transitions with //K// = 0 to 4 of methyl chloride, CH<sub>3</sub>Cl, were detected with ALMA near 345.4 and 340.1 GHz for the <sup>35</sup>Cl and <sup>37</sup>Cl isotopologs, respectively, in emission toward the Solar-type protostar IRAS 16293–2422B. CH<sub>3</sub><sup>35</sup>Cl was also seen toward the companion IRAS 16293–2422A. The <sup>35</sup>Cl/<sup>37</sup>Cl ratio is about 2.1, the same as observed for HCl in that source, but slightly lower than 3.13 on Earth.\\
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