molecules:extragalactic:h2cn_extragalactic [CDMS classic documentation]

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===== On the Detection of Methyleneamidogen, H2CN, in Extragalactic Sources =====

B. Tercero, J. Cernicharo, S. Cuadrado, P. de Vicente, and M. Guélin\\
used the Yebes 40 m telescopy in the 7 mm wavelength region (rest frequencies: 58.7 − 93.5 GHz) to study the molecular content of a foreground galaxy at //z// = 0.89 in absorption toward the quasar PKS 1830-211:\\
**[[https://doi.org/10.1051/0004-6361/202037837|New Molecular Species at Redshift //z// = 0.89]]**\\
//Astron. Astrophys.// **636**, (2020) Art. No. L7.\\
The methyleneamidogen radical, H<sub>2</sub>CN, also known as methaniminyl, was identfied by four hyperfine components of the 1<sub>01</sub> − 0<sub>00</sub> //ortho// rotational transition. The lines show good to quite reasonable signal-to-noise ratios. 

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Contributor(s): H. S. P. Müller; 4, 2020

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