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| molecules:extragalactic:ch2nh_extragalactic [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:extragalactic:ch2nh_extragalactic [2019/10/22 16:24] (current) – mueller |
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| S. Martín, R. Mauersberger, J. Martín-Pintado, C. Henkel, and S. García-Burillo\\ | S. Martín, R. Mauersberger, J. Martín-Pintado, C. Henkel, and S. García-Burillo\\ |
| used the IRAM 30 m telecope to carry out\\ | used the IRAM 30 m telecope to carry out\\ |
| **[[http://dx.doi.org/10.1086/503297|A 2 Millimeter Spectral Line Survey of the Starburst Galaxy NGC 253]]**\\ | **[[https://doi.org/10.1086/503297|A 2 Millimeter Spectral Line Survey of the Starburst Galaxy NGC 253]]**\\ |
| //Astrophys. J. Suppl. ser.// **164**, (2006) 450 – 476.\\ | //Astrophys. J. Suppl. ser.// **164**, (2006) 450 – 476.\\ |
| Methanimine, H<sub>2</sub>CNH, was identified by the //J<sub>K<sub>a</sub>,K<sub>c</sub></sub>// = 2<sub>1,1</sub> – 1<sub>1,0</sub> transition in emission near 133.27 GHz. A feature near the noise level is present at the 1<sub>1,0</sub> – 1<sub>0,1</sub> transition with rest frequencies near 166.85 GHz. | Methanimine, H<sub>2</sub>CNH, was identified by the //J<sub>K<sub>a</sub>,K<sub>c</sub></sub>// = 2<sub>1,1</sub> – 1<sub>1,0</sub> transition in emission near 133.27 GHz. A feature near the noise level is present at the 1<sub>1,0</sub> – 1<sub>0,1</sub> transition with rest frequencies near 166.85 GHz. |
| 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 1<sub>0,1</sub> – 0<sub>0,0</sub> ground state transition was detected prominently in absorption near 33.9 GHz, corresponding to a rest frequency of about 64.0 GHz. | The 1<sub>0,1</sub> – 0<sub>0,0</sub> ground state transition was detected prominently in absorption near 33.9 GHz, corresponding to a rest frequency of about 64.0 GHz. |
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| Contributor(s): H. S. P. Müller; 08, 2017 | Contributor(s): H. S. P. Müller; 08, 2017 |
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