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. ===== On Amidogen, NH2, in Extragalactic Sources ===== Amidogen was detected with ALMA within cycle 0 observations in the unnamed foreground galaxy at //z// ≈ 0.89 toward the blazar PKS 1830–211 by\\ S. Muller, F. Combes, M. Guélin, et al.,\\ **[[https://doi.org/10.1051/0004-6361/201423646|An ALMA Early Science survey of molecular absorption lines toward PKS 1830–211 – Analysis of the absorption profiles]]**\\ //Astron. Astrophys.// **566**, (2014) Art. No. A112.\\ The strongest //J// = 1.5 – 1.5 and the weaker 1.5 – 0.5 fine structure components of the 1<sub>10</sub> – 1<sub>01</sub> transition of //para//-amidogen at 462446.5 and around 461440 MHz were detected in absorption, the latter with partially resolved <sup>14</sup>N hyperfine splitting. ---- Contributor(s): H. S. P. Müller; 07, 2014. ---- molecules/extragalactic/nh2_extragalactic.txt Last modified: 2019/10/22 13:50by mueller