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:hcnh-plus [2020/10/28 11:55]
mueller
molecules:ism:hcnh-plus [2020/10/28 11:59] (current)
mueller
Line 9: Line 9:
 P. Schilke, C. M. Walmsley, T. J. Millar, and C. Henkel\\ P. Schilke, C. M. Walmsley, T. J. Millar, and C. Henkel\\
 reported on the\\ reported on the\\
-**[[https://​ui.adsabs.harvard.edu/#​abs/​1991A&​A...247..487S/​abstract|Detection of the Quadrupole Hyperfine Structure ​in HCNH<​sup>​+</​sup>​]]**,\\+**[[https://​ui.adsabs.harvard.edu/#​abs/​1991A&​A...247..487S/​abstract|Protonated HCN in molecular clouds]]**,\\
 //Astron. Astrophys.//​ **247**, 487 – 496 (1991).\\ //Astron. Astrophys.//​ **247**, 487 – 496 (1991).\\
 They detected the //J"// = 1 and 2 transition toward the dark cloud TMC-1 using the IRAM 30 m dish. They detected the //J"// = 1 and 2 transition toward the dark cloud TMC-1 using the IRAM 30 m dish.
  • molecules/ism/hcnh-plus.1603882535.txt.gz
  • Last modified: 2020/10/28 11:55
  • by mueller