molecules:ism:h2cn

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molecules:ism:h2cn [2021/10/13 14:16] – muellermolecules:ism:h2cn [2021/10/13 14:19] (current) – mueller
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 **[[https://doi.org/10.1051/0004-6361/201935010|Isocyanogen Formation in the Cold Interstellar Medium]]**,\\ **[[https://doi.org/10.1051/0004-6361/201935010|Isocyanogen Formation in the Cold Interstellar Medium]]**,\\
 //Astron. Astrophys.// **625**, art. no. A91 (2019).\\ //Astron. Astrophys.// **625**, art. no. A91 (2019).\\
-A molecular line survey of the prestellar cor L1544 between 71.74 and 115.87 GHz was carried out with the IRAM 30 m telescope. Methyleneamidogen was observed through six hyperfine transitions around 73.4 GHz.\\+A molecular line survey of the prestellar core L1544 between 71.74 and 115.87 GHz was carried out with the IRAM 30 m telescope. Methyleneamidogen was observed through six hyperfine transitions around 73.4 GHz.\\
  
  
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-Contributor(s): H. S. P. Müller; 12, 2017; 11, 2020+Contributor(s): H. S. P. Müller; 09, 2021; 10, 2021
  
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