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| molecules:ism:oxiran [2022/11/17 14:30] – mueller | molecules:ism:oxiran [2023/06/09 13:56] (current) – mueller | ||
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| //Mon. Not. R. Astron. Soc.// **518**, 185 (2023).\\ | //Mon. Not. R. Astron. Soc.// **518**, 185 (2023).\\ | ||
| 17 lines, corresponging to 19 transitions with 4 ≤ //J// ≤ 13 with diverse values of // | 17 lines, corresponging to 19 transitions with 4 ≤ //J// ≤ 13 with diverse values of // | ||
| + | \\ | ||
| + | |||
| + | H. S. P. Müller, J. K. Jørgensen, J.-C. Guillemin, F. Lewen, and S. Schlemmer\\ | ||
| + | presented more recently the\\ | ||
| + | **[[https:// | ||
| + | //J. Mol. Spectrosc.// | ||
| + | As in the case of the mono-deuterated oxirane above, lines were identifies in the PILS data. | ||
| + | Five or six lines are essentially unblended and have a sufficient signal-to-noise ratio, | ||
| + | two more lines are blended, and the combination of the contributions account nicely for the emission lines. | ||
| + | So the identification was deemed to be somewhat tentative in this line-rich survey. | ||
| + | From the estimate of the column density, one can derive a degree of deuteration per H atom of ~0.16, | ||
| + | compared to ~0.036 per H atom in the case of // | ||
| + | Such an enhancement of the degree of deuteration per H atom has also been seen for other | ||
| + | doubly deuterated molecules compared to their mono-deuerated variants, such as CHD< | ||
| + | CHD< | ||
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| - | Contributor(s): | + | Contributor(s): |
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