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| molecules:ism:h3-plus [2020/09/18 14:02] – mueller | molecules:ism:h3-plus [2020/09/18 14:11] (current) – [On the Detection of H2D+] mueller |
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| used the GREAT instrument on board the SOFIA aircraft observatory to detect the 1<sub>0,1</sub> – 0<sub>0,0</sub> ground state transition of //para//-H<sub>2</sub>D<sup>+</sup> at 1370.085 GHz in absorption toward IRAS 16293-2422 and to deduce\\ | used the GREAT instrument on board the SOFIA aircraft observatory to detect the 1<sub>0,1</sub> – 0<sub>0,0</sub> ground state transition of //para//-H<sub>2</sub>D<sup>+</sup> at 1370.085 GHz in absorption toward IRAS 16293-2422 and to deduce\\ |
| **[[https://doi.org/10.1038/nature13924|H<sub>2</sub>D<sup>+</sup> observations give an age of at least one million years for a cloud core forming Sun-like stars]]**\\ | **[[https://doi.org/10.1038/nature13924|H<sub>2</sub>D<sup>+</sup> observations give an age of at least one million years for a cloud core forming Sun-like stars]]**\\ |
| //Nature// **516**, 219–221 (2014).// | //Nature// **516**, 219–221 (2014).\\ |
| See also the [[https://www.mpifr-bonn.mpg.de/pressreleases/2014/11|MPIfR press release]] (in English; German version also available) or the [[https://portal.uni-koeln.de/universitaet/aktuell/presseinformationen/detail/das-alter-von-stellaren-kinderstuben|Universität zu Köln press release]] (in German). | See also the **[[https://www.mpifr-bonn.mpg.de/pressreleases/2014/11|MPIfR press release]]** (in English; **[[https://www.mpifr-bonn.mpg.de/pressemeldungen/2014/11|German version]]** also available) or the **[[https://portal.uni-koeln.de/universitaet/aktuell/presseinformationen/detail/das-alter-von-stellaren-kinderstuben|Universität zu Köln press release]]** (in German). |
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