molecules:extragalactic:h2ccn_extragalactic

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molecules:extragalactic:h2ccn_extragalactic [2019/02/25 22:38] – external edit 127.0.0.1molecules:extragalactic:h2ccn_extragalactic [2019/10/22 16:25] (current) – mueller
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 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.\\
 The cyanomethyl radical shows at low quantum numbers complicated pattern caused by fine structure (FS) and hyperfine structure (HFS) of the N nucleus; at even //K<sub>a</sub>//, HFS of the two equivalent H nuclei occurs. Two //K<sub>a</sub>// = 0 transitions with //J"// = 2 and 3 were detected. The lines were broadened because of FS and HFS. The cyanomethyl radical shows at low quantum numbers complicated pattern caused by fine structure (FS) and hyperfine structure (HFS) of the N nucleus; at even //K<sub>a</sub>//, HFS of the two equivalent H nuclei occurs. Two //K<sub>a</sub>// = 0 transitions with //J"// = 2 and 3 were detected. The lines were broadened because of FS and HFS.
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 Contributor(s): H. S. P. Müller; 5, 2012 Contributor(s): H. S. P. Müller; 5, 2012
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