molecules:extragalactic:nh_extragalactic

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molecules:extragalactic:nh_extragalactic [2019/02/25 22:38] – external edit 127.0.0.1molecules:extragalactic:nh_extragalactic [2019/10/22 13:33] (current) – mueller
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 The detection of the imidogen radical, NH, with //ISO// LWS in an Extragalactic source was described first by\\ 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,\\ E. González-Alfonso, H, A. Smith, J. Fischer, and J. Cernicharo,\\
-**[[http://dx.doi.org/10.1086/422868|The Far-Infrared Spectrum of Arp 220]]**\\+**[[https://doi.org/10.1086/422868|The Far-Infrared Spectrum of Arp 220]]**\\
 //Astrophys. J.// **613**, (2004) 247–261.\\ //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. 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.
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 Contributor(s): H. S. P. Müller; 10, 2010. Contributor(s): H. S. P. Müller; 10, 2010.
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