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--- molecules:ism:nh2 [2022/05/28 11:37] – mueller
+++ molecules:ism:nh2 [2023/02/10 16:17] – mueller
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 **[[https://doi.org/10.1086/187076|Discovery of the Interstellar NH<sub>2</sub> Radical]]**\\
 //Astrophys. J.// **416**, L83–L86 (1993).\\
-Three fine structure components were observed with partially resolved <sup>14</sup>N hyperfine structure which obviously secures the identification.
+Three fine structure components were observed with partially resolved <sup>14</sup>N hyperfine structure which obviously secures the identification.\\
+\\
 Further transitions were reported in\\
 J. R. Goicoechea, N. J. Rodríguez-Fernández and J. Cernicharo,\\
-**[[https://doi.org/10.1086/379704|The Far-Infrared Spectrum of the Sagittarius B2 Region:\\
+**[[https://doi.org/10.1086/379704|The Far-Infrared Spectrum of the Sagittarius B2 Region: Extended Molecular Absorption, Photodissociation, and Photoionization]]**\\
-Extended Molecular Absorption, Photodissociation, and Photoionization]]**\\
+//Astrophys. J.// **600**, 214–233 (2004).\\
-//Astrophys. J.// **600**, 214–233 (2004).
+\\
+ M. Melosso, L. Bizzocchi, O. Sipilä, B. M. Giuliano, L. Dore, F. Tamassia, M.-A. Martin-Drumel, O. Pirali, E. Redaelli, and P. Caselli\\
+reported on the\\
+**[[https://doi.org/10.1051/0004-6361/202038490|First detection of NHD and ND2 in the interstellar medium — Amidogen deuteration in IRAS 16293–2422]]**\\
+//Astron. Astrophys.// **641**, Art. No. A153 (2020).\\
+Both isotopologs were detected in archival HIFI///Herschel// data taken toward the Class 0 protostar IRAS 16293−2422. Very high degrees of deuteration were inferred.\\
+\\
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-Contributor(s): H. S. P. Müller; 03, 2007
+Contributor(s): H. S. P. Müller; 03, 2007; 02, 2023
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