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| molecules:ism:mesih3 [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:mesih3 [2019/04/26 15:31] (current) – mueller |
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| reported on the\\ | reported on the\\ |
| **[[https://doi.org/10.1051/0004-6361/201731672|Discovery of Methyl Silane and Confirmation of Silyl Cyanide in IRC +10216]]**\\ | **[[https://doi.org/10.1051/0004-6361/201731672|Discovery of Methyl Silane and Confirmation of Silyl Cyanide in IRC +10216]]**\\ |
| //Astron. Astrophys.// **606**, LL5 (2017).\\ | //Astron. Astrophys.// **606**, Art. No. L5 (2017).\\ |
| 8 sets of methyl silane, CH<sub>3</sub>SiH<sub>3</sub> transitions with //J'// between 4 and 16 (between 87 and 351 GHz) were detected with the IRAM 30 m telescope in emission toward the late-type C-rich star CW Leonis. The //K// levels are blended at low //J//, but partly resolved //K// level structure is seen at higher //J//. Some sets of transitions are slightly or strongly blended with emission lines of other molecules, but in all instances there are features not entirely blended. | 8 sets of methyl silane, CH<sub>3</sub>SiH<sub>3</sub> transitions with //J'// between 4 and 16 (between 87 and 351 GHz) were detected with the IRAM 30 m telescope in emission toward the late-type C-rich star CW Leonis. The //K// levels are blended at low //J//, but partly resolved //K// level structure is seen at higher //J//. Some sets of transitions are slightly or strongly blended with emission lines of other molecules, but in all instances there are features not entirely blended. |
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