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| molecules:ism:c10h [2023/02/27 13:11] – created mueller | molecules:ism:c10h [2023/02/27 13:26] – mueller |
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| **[[https://doi.org/10.3847/2041-8213/acb648|Astronomical Detection of the Interstellar Anion C<sub>10</sub>H<sup>–</sup> toward TMC-1 from the GOTHAM Large Program on the Green Bank Telescope]]**\\ | **[[https://doi.org/10.3847/2041-8213/acb648|Astronomical Detection of the Interstellar Anion C<sub>10</sub>H<sup>–</sup> toward TMC-1 from the GOTHAM Large Program on the Green Bank Telescope]]**\\ |
| //Astrophys. J. Lett.// **944**, Art. No. L45 (2023).\\ | //Astrophys. J. Lett.// **944**, Art. No. L45 (2023).\\ |
| | The identification was made by stacking data from the line survey up to 30 GHz; most signal-contribution came from the 13.1 to 19.2 GHz region. The authors also report a tentative detection of C<sub>10</sub>H with a C<sub>10</sub>H<sup>–</sup> to C<sub>10</sub>H of roughly 2. In addition, C<sub>10</sub>H<sup>–</sup> is roughly 5 times more abundant than C<sub>8</sub>H<sup>–</sup> and about one third more abundant than C<sub>6</sub>H<sup>–</sup>.\\ |
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| | Contributor(s): H. S. P. Müller; 2, 2023 |
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