molecules:ism:3b

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:3b [2020/10/08 15:45] muellermolecules:ism:3b [2021/04/12 17:11] mueller
Line 5: Line 5:
 **[[https://doi.org/10.3847/2041-8213/aba632|Early Science from GOTHAM: Project Overview, Methods, and the Detection of Interstellar Propargyl Cyanide (HCCCH<sub>2</sub>CN) in TMC-1]]**\\ **[[https://doi.org/10.3847/2041-8213/aba632|Early Science from GOTHAM: Project Overview, Methods, and the Detection of Interstellar Propargyl Cyanide (HCCCH<sub>2</sub>CN) in TMC-1]]**\\
 //Astrophys. J. Lett.// **900**, Art. No. L10 (2020).\\ //Astrophys. J. Lett.// **900**, Art. No. L10 (2020).\\
-The observations were obtained in the course of the line survey Green Bank Telescope Observations of TMC-1: Hunting for Aromatic Molecules. The data were recorded with very high resolution which resolves, at least in part, the complex velocity structure and the <sup>14</sup>N hyperfine structure splitting of the 4<sub>1,3</sub>−3<sub>1,2</sub>, 5<sub>1,5</sub>−4<sub>1,4</sub>, 5<sub>0,5</sub>−4<sub>0,4</sub>, and 5<sub>1,4</sub>−4<sub>1,3</sub> transitions near 22.6, 26.6, 27.3, and 28.2 GHz, respectively, at the expense of noise levels of about the same level as the individual lines. The analysis was improved by employing a stacking technique.+The observations were obtained in the course of the line survey Green Bank Telescope Observations of TMC-1: Hunting for Aromatic Molecules. The data were recorded with very high resolution which resolves, at least in part, the complex velocity structure and the <sup>14</sup>N hyperfine structure splitting of the 4<sub>1,3</sub>−3<sub>1,2</sub>, 5<sub>1,5</sub>−4<sub>1,4</sub>, 5<sub>0,5</sub>−4<sub>0,4</sub>, and 5<sub>1,4</sub>−4<sub>1,3</sub> transitions near 22.6, 26.6, 27.3, and 28.2 GHz, respectively, at the expense of noise levels of about the same level as the individual lines. The analysis was improved by employing a stacking technique.\\
  
 +
 +N. Marcelino, B. Tercero, M. Agúndez and J. Cernicharo\\
 +reported shortly thereafter on\\
 +**[[https://doi.org/10.1051/0004-6361/202040177|A study of C<sub>4</sub>H<sub>3</sub>N isomers in TMC-1: Line by line detection of HCCCH<sub>2</sub>CN in TMC-1]]**\\
 +//Astron. Astrophys.// **646**, Art. No. L9 (2021).\\
  
 ---- ----
  
-Contributor(s): H. S. P. Müller; 10, 2020+Contributor(s): H. S. P. Müller; 10, 2020; 04, 2021
  
 ---- ----
  
  • molecules/ism/3b.txt
  • Last modified: 2021/04/12 17:14
  • by mueller