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| molecules:ism:h2cn [2021/10/13 14:16] – mueller | molecules:ism:h2cn [2021/10/13 14:16] – 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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