Differences

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

Link to this comparison view

molecules:extragalactic:menh2_extragalactic [2019/02/25 22:38]
127.0.0.1 external edit
molecules:extragalactic:menh2_extragalactic [2019/10/22 16:31]
mueller
Line 3: Line 3:
 S. Muller, A. Beelen, M. Guélin, S. Aalto, J. H. Black, F. Combes, S. J. Curran, P. Theule, and S. N. Longmore\\ S. Muller, A. Beelen, M. Guélin, S. Aalto, J. H. Black, F. Combes, S. J. Curran, P. Theule, and S. N. Longmore\\
 used the Australia Telescope Compact Array (ATCA) to study the molecular content of a foreground galaxy at //​z//​ = 0.89 (FG0.89 consisting of two subsources, FG0.89SW and FG0.89NO) in absorption toward the quasar PKS 1830-211:​\\ used the Australia Telescope Compact Array (ATCA) to study the molecular content of a foreground galaxy at //​z//​ = 0.89 (FG0.89 consisting of two subsources, FG0.89SW and FG0.89NO) in absorption toward the quasar PKS 1830-211:​\\
-**[[http://dx.doi.org/​10.1051/​0004-6361/​201117096|Molecules at //​z//​ = 0.89:​ A 4-mm-Rest-Frame Absorption-Line Survey toward PKS 1830-211]]**\\+**[[https://​doi.org/​10.1051/​0004-6361/​201117096|Molecules at //​z//​ = 0.89:​ A 4-mm-Rest-Frame Absorption-Line Survey toward PKS 1830-211]]**\\
 //Astron. Astrophys.//​ **535**, (2011) Art. No. A103.\\ //Astron. Astrophys.//​ **535**, (2011) Art. No. A103.\\
 Methylamine,​ CH<​sub>​3</​sub>​NH<​sub>​2</​sub>,​ is an asymmetric top rotor displaying considerable splitting caused by the internal rotation of the CH<​sub>​3</​sub>​ group and the inversion of the NH<​sub>​2</​sub>​ group. Three transitions with //K// = 1 – 0 have been identified; two with //​J'//​ = //​J"//​ = 1 at rest frequencies of 79008 and 89956 MHz, respectively,​ and one with //​J'//​ = //​J"//​ = 2 at 78135 MHz. Even though the number of lines is a bit small, the detection can probably be viewed as secure because of the moderate line number density. Methylamine,​ CH<​sub>​3</​sub>​NH<​sub>​2</​sub>,​ is an asymmetric top rotor displaying considerable splitting caused by the internal rotation of the CH<​sub>​3</​sub>​ group and the inversion of the NH<​sub>​2</​sub>​ group. Three transitions with //K// = 1 – 0 have been identified; two with //​J'//​ = //​J"//​ = 1 at rest frequencies of 79008 and 89956 MHz, respectively,​ and one with //​J'//​ = //​J"//​ = 2 at 78135 MHz. Even though the number of lines is a bit small, the detection can probably be viewed as secure because of the moderate line number density.
Line 11: Line 11:
  
 Contributor(s):​ H. S. P. Müller; 5, 2012 Contributor(s):​ H. S. P. Müller; 5, 2012
- 
  
 ---- ----
  
  
  • molecules/extragalactic/menh2_extragalactic.txt
  • Last modified: 2019/10/22 16:31
  • by mueller