molecules:ism:hcnh-plus

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molecules:ism:hcnh-plus [2019/10/22 16:40] – muellermolecules:ism:hcnh-plus [2020/10/28 11:59] (current) – mueller
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 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. Ziurys, A. J. Apponi, and J. T. Yoder\\+P. Schilke, C. M. Walmsley, T. J. Millar, and C. Henkel\\
 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.
  
  
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-Contributor(s): H. S. P. Müller; 07, 2015+Contributor(s): H. S. P. Müller; 07, 2015; 10, 2020
  
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  • molecules/ism/hcnh-plus.txt
  • Last modified: 2020/10/28 11:59
  • by mueller