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--- molecules:ism:hcnh-plus [2019/02/25 22:38] – external edit 127.0.0.1
+++ molecules:ism:hcnh-plus [2020/10/28 11:59] (current) – mueller
@@ Line 3: / Line 3: @@
 L. M. Ziurys and B. E. Turner\\
 reported on\\
-**[[http://cdsads.u-strasbg.fr/abs/1986ApJ...302L..31Z|HCNH<sup>+</sup> – A New Interstellar Molecular Ion]]**,\\
+**[[https://ui.adsabs.harvard.edu/abs/1986ApJ...302L..31Z|HCNH<sup>+</sup> – A New Interstellar Molecular Ion]]**,\\
 //Astrophys. J.// **302**, L31 – L36 (1986).\\
 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\\
-**[[http://cdsads.u-strasbg.fr/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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