molecules:ism:h2nc

Differences

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

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
Last revisionBoth sides next revision
molecules:ism:h2nc [2021/10/12 12:43] muellermolecules:ism:h2nc [2022/03/08 15:44] mueller
Line 1: Line 1:
-===== On the Detection of Aminomethylidyne, H2NC, in the ISM =====+===== On the Detection of Aminomethylidyne, H<sub>2</sub>NC, in the ISM =====
  
 C. Cabezas, M. Agúndez, N. Marcelino, B. Tercero, S. Cuadrado, and J. Cernicharo\\ C. Cabezas, M. Agúndez, N. Marcelino, B. Tercero, S. Cuadrado, and J. Cernicharo\\
 reported on the\\ reported on the\\
-**[[https://doi.org/10.1051/0004-6361/202141491|Interstellar Detection of the Simplest Aminocarbyne H<sub>2</sub>NC: An ignored but Abundant Molecule]]**\\ +**[[https://doi.org/10.1051/0004-6361/202141491|Interstellar Detection of the Simplest Aminocarbyne H<sub>2</sub>NC: An ignored but Abundant Molecule]]**\\ 
-//Astron. Astrophys.// **654**, artno. A45 (2021).\\ +//Astron. Astrophys.// **654**, ArtNo. A45 (2021).\\ 
-The aminomethylidyne isomer was observed in the course of molecular line surveys of L483 and B1-b protostellar objects carried out at 3 mm using the IRAM 30 m telescope. The molecule was not detected in corresponding data of the prestellar core TMC-1. The column densities of H<sub>2</sub>CN and H<sub>2</sub>NC were essentially the same in these two sources.\\+The aminomethylidyne isomer was observed in the course of molecular line surveys of L483 and B1-b protostellar objects carried out at 3 mm using the IRAM 30 m telescope. The molecule was not detected in corresponding data of the prestellar core TMC-1. The column densities of H<sub>2</sub>CN and H<sub>2</sub>NC were essentially the same in the first two sources.\\
  
 ---- ----
  • molecules/ism/h2nc.txt
  • Last modified: 2023/06/09 11:02
  • by mueller