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--- molecules:ism:heh-plus [2019/04/23 17:45] – mueller
+++ molecules:ism:heh-plus [2020/05/12 13:37] (current) – mueller
@@ Line 2: / Line 2: @@
 R. Güsten, H. Wiesemeyer, D. Neufeld, K. M. Menten, U. U. Graf, K. Jacobs,
-B. Klein, O. Ricken, C. Risacher, and J. Stutzki,\\
+B. Klein, O. Ricken, C. Risacher, and J. Stutzki\\
 reported on the\\
 **[[https://doi.org/10.1038/s41586-019-1090-x|Astrophysical detection of the helium hydride ion HeH<sup>+</sup>]]**\\
@@ Line 10: / Line 10: @@
 instrument using the SOFIA airplane. The column density is quite close to model
 calculations; interestingly, about a factor of four was detected compared to
-the expectations.
+the expectations.\\
+See also the [[https://www.mpifr-bonn.mpg.de/pressreleases/2019/5|MPIfR press release]] (in English; [[https://www.mpifr-bonn.mpg.de/pressemeldungen/2019/5|German version]] also available).\\
+D. A. Neufeld, M. Goto, T. R. Geballe, R. Güsten, K. M. Menten, and H. Wiesemeyer\\
+reported on the\\
+**[[https://doi.org/10.3847/1538-4357/ab7191|Detection of Vibrational Emissions from the Helium Hydride Ion (HeH<sup>+</sup>) in the Planetary Nebula NGC 7027]]**\\
+//Astrophys. J.// **894**, Art. No. 37 (2020).\\
+The //v// = 1 − 0, //P//(1) and //P//(2) transitions were detected near 3.5 and 3.6 μm, respectively, using the iSHELL spectrograph at the Infrared Telescope Facility on Mauna Kea. Their best source model reproduced the  //P//(1) flux very well, but underproduced the fluxes of the //P//(2) and rotational transitions.\\
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-Contributor(s): H. S. P. Müller; 04, 2019
+Contributor(s): H. S. P. Müller; 04, 2019; 05, 2020