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| molecules:extragalactic:nh2_extragalactic [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:extragalactic:nh2_extragalactic [2019/10/22 13:50] (current) – mueller |
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| Amidogen was detected with ALMA within cycle 0 observations in the unnamed foreground galaxy at //z// ≈ 0.89 toward the blazar PKS 1830–211 by\\ | Amidogen was detected with ALMA within cycle 0 observations in the unnamed foreground galaxy at //z// ≈ 0.89 toward the blazar PKS 1830–211 by\\ |
| S. Muller, F. Combes, M. Guélin, et al.,\\ | S. Muller, F. Combes, M. Guélin, et al.,\\ |
| **[[http://dx.doi.org/10.1051/0004-6361/201423646|An ALMA Early Science survey of molecular absorption lines toward PKS 1830–211 – Analysis of the absorption profiles]]**\\ | **[[https://doi.org/10.1051/0004-6361/201423646|An ALMA Early Science survey of molecular absorption lines toward PKS 1830–211 – Analysis of the absorption profiles]]**\\ |
| //Astron. Astrophys.// **566**, (2014) Art. No. A112.\\ | //Astron. Astrophys.// **566**, (2014) Art. No. A112.\\ |
| The strongest //J// = 1.5 – 1.5 and the weaker 1.5 – 0.5 fine structure components of the 1<sub>10</sub> – 1<sub>01</sub> transition of //para//-amidogen at 462446.5 and around 461440 MHz were detected in absorption, the latter with partially resolved <sup>14</sup>N hyperfine splitting. | The strongest //J// = 1.5 – 1.5 and the weaker 1.5 – 0.5 fine structure components of the 1<sub>10</sub> – 1<sub>01</sub> transition of //para//-amidogen at 462446.5 and around 461440 MHz were detected in absorption, the latter with partially resolved <sup>14</sup>N hyperfine splitting. |