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| molecules:ism:glykolamid [2023/08/24 12:22] – mueller | molecules:ism:glykolamid [2023/08/24 12:45] (current) – mueller |
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| **[[https://doi.org/10.3847/2041-8213/ace977|First Glycine Isomer Detected in the Interstellar Medium: Glycolamide (NH2C(O)CH2OH)]]**\\ | **[[https://doi.org/10.3847/2041-8213/ace977|First Glycine Isomer Detected in the Interstellar Medium: Glycolamide (NH2C(O)CH2OH)]]**\\ |
| //Astrophys. J. Lett.// **953**, Art. No. L20 (2023).\\ | //Astrophys. J. Lett.// **953**, Art. No. L20 (2023).\\ |
| | The molecule was detected in the course of a molecular line survey of the Galactic Center molecular cloud G+0.693–0.027 employing the Yebes 40 m and IRAM 30 m radio telecopes. The transitions cover 31 to 98 GHz with 1 ≤ //J// ≤ 7 and //K<sub>a</sub>// ≤ 5. Some lines are unblended, slightly blended, or the peak of the line is at most slightly blended. Some further lines are blended more substantially. The glycolaldehyde/glycolamide ratio is ∼15, while the ethanol/ethanolamine ratio is ∼40.\\ |
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