Show pageOld revisionsBacklinksBack to top This page is read only. You can view the source, but not change it. Ask your administrator if you think this is wrong. ===== Detection of Imidogen, NH, in Extragalactic Sources ===== The detection of the imidogen radical, NH, with //ISO// LWS in an Extragalactic source was described first by\\ E. González-Alfonso, H, A. Smith, J. Fischer, and J. Cernicharo,\\ **[[https://doi.org/10.1086/422868|The Far-Infrared Spectrum of Arp 220]]**\\ //Astrophys. J.// **613**, (2004) 247–261.\\ The two overlapping strongest fine structure components of the //N// = 2 – 1 transition were clearly detected near 153.2 μm as well as the overlapping components of 3 – 2 near 102 μm. There is additional evidence near the noise level for the three weaker fine structure components of 2 – 1. ---- Contributor(s): H. S. P. Müller; 10, 2010. ---- molecules/extragalactic/nh_extragalactic.txt Last modified: 2019/10/22 13:33by mueller