| |
| molecules:ism:hcl-plus [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:hcl-plus [2019/10/18 13:12] (current) – mueller |
|---|
| The //J// = 5/2 – 3/2 transition of the lower energy fine structure component <sup>2</sup>Π<sub>3/2</sub> of chloroniumyl has been detected in absorption in the diffuse medium along the sight-lines to the submillimeter continuum sources W31C and W49N by\\ | The //J// = 5/2 – 3/2 transition of the lower energy fine structure component <sup>2</sup>Π<sub>3/2</sub> of chloroniumyl has been detected in absorption in the diffuse medium along the sight-lines to the submillimeter continuum sources W31C and W49N by\\ |
| M. De Luca, H. Gupta, D. Neufeld, M. Gerin, D. Teyssier, B. J. Drouin, J. C. Pearson, D. C. Lis, R. Monje, T. G. Phillips, J. R. Goicoechea, B. Godard, E. Falgarone, A. Coutens, and T. A. Bell,\\ | M. De Luca, H. Gupta, D. Neufeld, M. Gerin, D. Teyssier, B. J. Drouin, J. C. Pearson, D. C. Lis, R. Monje, T. G. Phillips, J. R. Goicoechea, B. Godard, E. Falgarone, A. Coutens, and T. A. Bell,\\ |
| **[[http://dx.doi.org/10.1088/2041-8205/751/2/L37|//Herschel///HIFI Discovery of HCl<sup>+</sup> in the Interstellar Medium]]**\\ | **[[https://doi.org/10.1088/2041-8205/751/2/L37|//Herschel///HIFI Discovery of HCl<sup>+</sup> in the Interstellar Medium]]**\\ |
| //Astrophys. J.// **751**, (2012), Art. No. L37.\\ | //Astrophys. J.// **751**, (2012), Art. No. L37.\\ |
| Two structured features, caused by the <sup>35</sup>Cl and <sup>37</sup>Cl isotopologs, were observed near 1444 and 1442 GHz. The intricate structure of the features was caused by various clouds along the sight-line, Λ-doubling, and Cl hyperfine structure. The inferred column densities are very similar to those of H<sub>2</sub>Cl<sup>+</sup> and HCl in these sources. | Two structured features, caused by the <sup>35</sup>Cl and <sup>37</sup>Cl isotopologs, were observed near 1444 and 1442 GHz. The intricate structure of the features was caused by various clouds along the sight-line, Λ-doubling, and Cl hyperfine structure. The inferred column densities are very similar to those of H<sub>2</sub>Cl<sup>+</sup> and HCl in these sources. |