molecules:ism:hcocn

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
molecules:ism:hcocn [2021/06/30 16:19] muellermolecules:ism:hcocn [2021/06/30 16:19] (current) mueller
Line 8: Line 8:
 J. Cernicharo, C. Cabezas, Y. Endo, M. Agúndez, B. Tercero, J. R. Pardo, N. Marcelino, and P. de Vicente\\ J. Cernicharo, C. Cabezas, Y. Endo, M. Agúndez, B. Tercero, J. R. Pardo, N. Marcelino, and P. de Vicente\\
 report on\\ report on\\
-**[[https://doi.org/10.1051/0004-6361/202141297|The sulphur saga in TMC-1: Discovery of HCSCN and HCSCCH]]**\\+**[[https://doi.org/10.1051/0004-6361/202141297|The Sulphur Saga in TMC-1: Discovery of HCSCN and HCSCCH]]**\\
 //Astron. Astrophys.// **650**, Art. No. L14 (2021).\\ //Astron. Astrophys.// **650**, Art. No. L14 (2021).\\
 Formyl cyanide was indentified besides these two new and several other molecules. HC(O)CN was identified through 2 //a//-type transitions with //K<sub>a</sub>// = 0 and //J// = 4 − 3 or 5 − 4. The identifications were made in the course of an ongoing unbiased molecular line survey between 31.1 and 50.4 GHz using the Yebes 40 m radio telescope. The column density ratio of propynal and formyl cyanide is about 4.\\ Formyl cyanide was indentified besides these two new and several other molecules. HC(O)CN was identified through 2 //a//-type transitions with //K<sub>a</sub>// = 0 and //J// = 4 − 3 or 5 − 4. The identifications were made in the course of an ongoing unbiased molecular line survey between 31.1 and 50.4 GHz using the Yebes 40 m radio telescope. The column density ratio of propynal and formyl cyanide is about 4.\\
  • molecules/ism/hcocn.1625062745.txt.gz
  • Last modified: 2021/06/30 16:19
  • by mueller