| Both sides previous revision Previous revision Next revision | Previous revision |
| molecules:ism:nh2 [2022/05/28 11:37] – mueller | molecules:ism:nh2 [2023/02/10 16:31] (current) – mueller |
|---|
| **[[https://doi.org/10.1086/187076|Discovery of the Interstellar NH<sub>2</sub> Radical]]**\\ | **[[https://doi.org/10.1086/187076|Discovery of the Interstellar NH<sub>2</sub> Radical]]**\\ |
| //Astrophys. J.// **416**, L83–L86 (1993).\\ | //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\\ | Further transitions were reported in\\ |
| J. R. Goicoechea, N. J. Rodríguez-Fernández and J. Cernicharo,\\ | 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.\\ |
| | \\ |
| | |
| | A similar account was given shortly thereafter by\\ |
| | A. Bacmann, A. Faure, P. Hily-Blant, K. Kobayashi, H. Ozeki, S. Yamamoto, L. Pagani, and F. Lique,\\ |
| | **[[https://doi.org/10.1093/mnras/staa2903|Deuterium fractionation of nitrogen hydrides: detections of NHD and ND2]]**\\ |
| | //Mon. Not. R. Astron. Soc.// **499**, 1795 (2020).\\ |
| | NHD observations are based on archival APEX data, ND<sub>2</sub> observations on archival HIFI///Herschel// data as above. The numbers are very similar to the ones above. One can deduce deuteration degrees per A atom of ~0.25 and ~0.35 for NHD and ND<sub>2</sub>, respectively, from their total column densities.\\ |
| | \\ |
| |
| ---- | ---- |
| |
| Contributor(s): H. S. P. Müller; 03, 2007 | Contributor(s): H. S. P. Müller; 03, 2007; 02, 2023 |
| |
| ---- | ---- |
| |
| |