molecules:ism:sic3

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

molecules:ism:sic3 [2019/02/25 22:38] – external edit 127.0.0.1molecules:ism:sic3 [2019/10/22 17:07] (current) mueller
Line 4: Line 4:
  
 A. J. Apponi, M. C. McCarthy, C. A. Gottlieb, and P. Thaddeus\\ A. J. Apponi, M. C. McCarthy, C. A. Gottlieb, and P. Thaddeus\\
-reported on the **[[http://dx.doi.org/10.1086/311998|Astronomical Detection of Rhomboidal SiC<sub>3</sub>]]**\\+reported on the\\ 
 +**[[https://doi.org/10.1086/311998|Astronomical Detection of Rhomboidal SiC<sub>3</sub>]]**\\
 //Astrophys. J.// **516**, L103–L106 (1999).\\ //Astrophys. J.// **516**, L103–L106 (1999).\\
 7 emission lines of 9 rotational transitions with //J"// between 6 and 8 were detected in the circumstellar envelope of CW Leo (IRC +10216) with the 12 m NRAO telescope between 80 and 103 GHz. 7 emission lines of 9 rotational transitions with //J"// between 6 and 8 were detected in the circumstellar envelope of CW Leo (IRC +10216) with the 12 m NRAO telescope between 80 and 103 GHz.
Line 12: Line 13:
  
 Contributor(s): H. S. P. Müller; 05, 2015 Contributor(s): H. S. P. Müller; 05, 2015
- 
  
 ---- ----
  
  
  • molecules/ism/sic3.1551130727.txt.gz
  • Last modified: 2019/02/25 22:38
  • by 127.0.0.1