molecules:ism:menco

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:menco [2019/04/29 17:14] – muellermolecules:ism:menco [2020/07/06 10:13] (current) – mueller
Line 7: Line 7:
 Several clear, slightly, and heavily blended features were detected in emission in a molecular line survey of Sagittarius B2(N) in the 4 and 3 mm wavelength region using the 12 m ARO dish. The molecule occurs in both main hot cores with similar column densities at rotational temperatures of about 25 K. It is less abundant than HNCO by about factors of 35 and 53. Several clear, slightly, and heavily blended features were detected in emission in a molecular line survey of Sagittarius B2(N) in the 4 and 3 mm wavelength region using the 12 m ARO dish. The molecule occurs in both main hot cores with similar column densities at rotational temperatures of about 25 K. It is less abundant than HNCO by about factors of 35 and 53.
  
-J. Cernicharo1, Z. Kisiel, B. Tercero, L. Kolesniková, I. R. Medvedev, A. López, S. Fortman, M. Winnewisser, F. C. de Lucia, J. L. Alonso, and J.-C. Guillemin,\\+J. Cernicharo, Z. Kisiel, B. Tercero, L. Kolesniková, I. R. Medvedev, A. López, S. Fortman, M. Winnewisser, F. C. de Lucia, J. L. Alonso, and J.-C. Guillemin,\\
 reported on the\\ reported on the\\
 **[[https://doi.org/10.1051/0004-6361/201527531|A Rigorous Detection of Interstellar CH<sub>3</sub>NCO: An important Missing Species in Astrochemical Networks]]**\\ **[[https://doi.org/10.1051/0004-6361/201527531|A Rigorous Detection of Interstellar CH<sub>3</sub>NCO: An important Missing Species in Astrochemical Networks]]**\\
  • molecules/ism/menco.1556550898.txt.gz
  • Last modified: 2019/04/29 17:14
  • by mueller