Differences
This shows you the differences between two versions of the page.
Next revision | Previous revision | ||
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\\ | L. M. Ziurys and B. E. Turner\\ | ||
reported on\\ | reported on\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
The // | The // | ||
- | 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\\ | ||
- | **[[http://cdsads.u-strasbg.fr/abs/1992ApJ...397L.123Z|Detection of the Quadrupole Hyperfine Structure | + | **[[https://ui.adsabs.harvard.edu/#abs/1991A&A...247..487S/ |
- | //Astrophys. J.// **397**, L123 – L126 (1992).\\ | + | //Astron. |
- | 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): | + | Contributor(s): |
---- | ---- | ||