molecules:ism:hccn_etc

Differences

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

Link to this comparison view

Last revisionBoth sides next revision
molecules:ism:hccn_etc [2019/02/25 22:38] – external edit 127.0.0.1molecules:ism:hccn_etc [2019/05/09 12:39] – mueller
Line 10: Line 10:
 More recently, the detection of the next member, cyanoethynylmethylene, was also detected with the same instrument in the outer part of the circumstellar shell of CW Leo:\\ More recently, the detection of the next member, cyanoethynylmethylene, was also detected with the same instrument in the outer part of the circumstellar shell of CW Leo:\\
 J. Cernicharo, M. Guélin, and J. R. Pardo,\\ J. Cernicharo, M. Guélin, and J. R. Pardo,\\
-**[[http://dx.doi.org/10.1086/426439|Detection of the Linear Radical HC<sub>4</sub>N in IRC +10216]]**\\+**[[https://doi.org/10.1086/426439|Detection of the Linear Radical HC<sub>4</sub>N in IRC +10216]]**\\
 //Astrophys. J.// **615**, L145–L148 (2004).\\ //Astrophys. J.// **615**, L145–L148 (2004).\\
 12 fine structure components of 4 rotational transitions (//N// = 18 – 17 to 21 – 20) between 82 and 97 GHz were detected; 4 lines were partially blended. A rotational temperature of 25±4 K was derived, similar to that of HC<sub>3</sub>N in this source. 12 fine structure components of 4 rotational transitions (//N// = 18 – 17 to 21 – 20) between 82 and 97 GHz were detected; 4 lines were partially blended. A rotational temperature of 25±4 K was derived, similar to that of HC<sub>3</sub>N in this source.
  • molecules/ism/hccn_etc.txt
  • Last modified: 2019/10/22 16:39
  • by mueller