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
molecules:ism:hcnh-plus [2019/10/22 16:40]
mueller
molecules:ism:hcnh-plus [2020/10/28 11:59] (current)
mueller
Line 7: Line 7:
 The //​J"//​ = 0,​ 1, and 2 transitions near 74.1, 148.2 and 222.3 GHz were detected in emission toward Sgr B2(OH) using the NRAO 12 m dish for the former, and the Texas MWO 4.9 m dish for the latter two transitions. The //​J"//​ = 0,​ 1, and 2 transitions near 74.1, 148.2 and 222.3 GHz were detected in emission toward Sgr B2(OH) using the NRAO 12 m dish for the former, and the Texas MWO 4.9 m dish for the latter two transitions.
  
-L. M. ZiurysA. J. Apponi, and J. TYoder\\+P. Schilke, C. M. WalmsleyT. J. Millar, and CHenkel\\
 reported on the\\ reported on the\\
-**[[https://​ui.adsabs.harvard.edu/​abs/​1992ApJ...397L.123Z|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]]**,\\ 
-//Astrophys. J.// **397**, L123 – L126 (1992).\\ +//Astron. ​Astrophys.//​ **247**, 487 – 496 (1991).\\ 
-They detected the ground state transition toward the dark cloud TMC-1 using the NRAO 12 m dish.+They detected the //J"// = 1 and 2 transition toward the dark cloud TMC-1 using the IRAM 30 m dish.
  
  
 ---- ----
  
-Contributor(s):​ H. S. P. Müller; 07, 2015+Contributor(s):​ H. S. P. Müller; 07, 2015; 10, 2020
  
 ---- ----
  
  
  • molecules/ism/hcnh-plus.1571755212.txt.gz
  • Last modified: 2019/10/22 16:40
  • by mueller