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| molecules:ism:sh-plus [2021/07/14 10:46] – mueller | molecules:ism:sh-plus [2021/07/14 10:58] (current) – mueller |
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| **[[https://doi.org/10.1051/0004-6361/202040203|//Herschel// observations of EXtraOrdinary Sources: Full //Herschel///HIFI Molecular Line Survey of Sagittarius B2(M)]]**\\ | **[[https://doi.org/10.1051/0004-6361/202040203|//Herschel// observations of EXtraOrdinary Sources: Full //Herschel///HIFI Molecular Line Survey of Sagittarius B2(M)]]**\\ |
| //Astron. Astrophys.// **651**, Art. No. A9 (2021).\\ | //Astron. Astrophys.// **651**, Art. No. A9 (2021).\\ |
| They observe clearly the //J// = 2 − 1 transition of CD<sup>+</sup> near 906.8 GHz mostly in absorption. The //J// = 4 − 2 transition near 1811.2 GHz is seen weakly in absorption.\\ | They observed the //J// = 2 − 1 and 1 − 1 fine structure components of the //N// = 1 − 0 rotational transition of <sup>34</sup>SH<sup>+</sup> near 525.1 and 682.5 GHz, respectively, in absorption.\\ |
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| Contributor(s): H. S. P. Müller; 12, 2010; 07, 2014; 12, 2015. | Contributor(s): H. S. P. Müller; 12, 2010; 07, 2014; 12, 2015; 07, 2021. |
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