Differences
This shows you the differences between two versions of the page.
molecules:extragalactic:menh2_extragalactic [2019/02/25 22:38] 127.0.0.1 external edit |
molecules:extragalactic:menh2_extragalactic [2019/10/22 16:31] (current) 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 | ||
- | |||
---- | ---- | ||