| |
| molecules:extragalactic:c2s_extragalactic [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:extragalactic:c2s_extragalactic [2019/10/22 13:48] (current) – mueller |
|---|
| 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.\\ |
| Thioethenylidene, C<sub>2</sub>S, was identified by its four //N<sub>J</sub>// = 10<sub>11</sub> – 9<sub>10</sub> to 11<sub>12</sub> – 10<sub>14</sub> transitions with rest frequencies between 131.5 and 144.3 GHz. | Thioethenylidene, C<sub>2</sub>S, was identified by its four //N<sub>J</sub>// = 10<sub>11</sub> – 9<sub>10</sub> to 11<sub>12</sub> – 10<sub>14</sub> transitions with rest frequencies between 131.5 and 144.3 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 low energy fine structure lines //N<sub>J</sub>// = 5<sub>5</sub> – 4<sub>3</sub>, 6<sub>5</sub> – 5<sub>4</sub>, and 7<sub>6</sub> – 6<sub>5</sub> with rest frequencies near 57.2, 69.3, and 81.5 GHz, respectively, were detected in absorption. | The low energy fine structure lines //N<sub>J</sub>// = 5<sub>5</sub> – 4<sub>3</sub>, 6<sub>5</sub> – 5<sub>4</sub>, and 7<sub>6</sub> – 6<sub>5</sub> with rest frequencies near 57.2, 69.3, and 81.5 GHz, respectively, were detected in absorption. |
| |
| Contributor(s): H. S. P. Müller; 08, 2017 | Contributor(s): H. S. P. Müller; 08, 2017 |
| |
| |
| ---- | ---- |
| |
| |