This shows you the differences between two versions of the page.
| Both sides previous revision Previous revision Next revision | Previous revision |
| molecules:ism:hnc3 [2024/04/08 17:52] – mueller | molecules:ism:hnc3 [2024/04/08 17:59] (current) – mueller |
|---|
| //Astron. Astrophys.// **642**, Art. No. L8 (2020).\\ | //Astron. Astrophys.// **642**, Art. No. L8 (2020).\\ |
| The authors report the detection of DNC<sub>3</sub>. The observations were obtained with the Yebes 40m radio telescope in the course of a line survey covering 31.0–50.3 GHz.\\ | The authors report the detection of DNC<sub>3</sub>. The observations were obtained with the Yebes 40m radio telescope in the course of a line survey covering 31.0–50.3 GHz.\\ |
| | \\ |
| | |
| | J. Cernicharo, B. Tercero, C. Cabezas, M. Agúndez, E. Roueff, R. Fuentetaja, N. Marcelino, and P. de Vicente\\ |
| | carried out more recently a\\ |
| | **[[https://doi.org/10.1051/0004-6361/202348822|Study of the HCCNC and HNCCC isotopologs in TMC-1]]**\\ |
| | //Astron. Astrophys.// **682**, Art. No. L13 (2024).\\ |
| | They reported in the framework of improved data of the above survey the detection of the three HNC<sub>3</sub> <sup>13</sup>C isotopomers. They determined the <sup>12</sup>C/<sup>13</sup>C ratios of ~90 with scatter that is insignificant with respect to the uncertainties. These values are somewhat lower than ~65 usually found in the the local ISM, but very similar to values of HCCNC <sup>13</sup>C isotopomers and to two of the three HC<sub>3</sub>N <sup>13</sup>C isotopomers. In addition, an H/D ratio of ~53 was reported, similar to the value of 57 ± 2 of HC<sub>3</sub>N.\\ |
| \\ | \\ |
| |