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molecules:ism:mesh [2019/10/23 22:01] – mueller | molecules:ism:mesh [2021/05/07 15:54] (current) – mueller | ||
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- | 6 features belonging to several more //J// = 3 –2 and 4 –3 were observed near 75.9 and near 101 GHz. The derived rotational temperature in that source was about 9 K. | + | 6 features belonging to several more //J// = 3 –2 and 4 –3 were observed near 75.9 and near 101 GHz. The derived rotational temperature in that source was about 9 K.\\ |
Much higher rotational temperatures (about 70 K) were derived in a 3, 2, and 1 mm line survey carried out with SEST:\\ | Much higher rotational temperatures (about 70 K) were derived in a 3, 2, and 1 mm line survey carried out with SEST:\\ | ||
E. Gibb, A. Nummelin, W. M. Irvine, D. C. B. Whittet, and P. Bergman,\\ | E. Gibb, A. Nummelin, W. M. Irvine, D. C. B. Whittet, and P. Bergman,\\ | ||
**[[https:// | **[[https:// | ||
- | // | + | // |
L. Majumdar, P. Gratier, T. Vidal, V. Wakelam, J.-C. Loison, K. M. Hickson, and E. Caux,\\ | L. Majumdar, P. Gratier, T. Vidal, V. Wakelam, J.-C. Loison, K. M. Hickson, and E. Caux,\\ | ||
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//Mon. Not. R. Astron. Soc.// **458**, 1859–1865 (2016).\\ | //Mon. Not. R. Astron. Soc.// **458**, 1859–1865 (2016).\\ | ||
- | The IRAM 30 m telescope was used to study this solar-type pair of proto-stars at 3 mm. Here, an excitation temperature of 32 ± 4 K was derived. | + | The IRAM 30 m telescope was used to study this solar-type pair of proto-stars at 3 mm. Here, an excitation temperature of 32 ± 4 K was derived.\\ |
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+ | L. F. Rodríguez-Almeida, | ||
+ | reported on\\ | ||
+ | **[[https:// | ||
+ | C< | ||
+ | // | ||
+ | This is the first unumbiguous detection of ethanethiol in the ISM. Ten lines with 2 ≤ //J// ≤ 6 and // | ||
H. S. P. Müller, A. Belloche, L.-H. Xu, R. M. Lees, R. T. Garrod, A. Walters, J. van Wijngaarden, | H. S. P. Müller, A. Belloche, L.-H. Xu, R. M. Lees, R. T. Garrod, A. Walters, J. van Wijngaarden, | ||
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- | Contributor(s): | + | Contributor(s): |
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