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| molecules:ism:sih3cn [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:sih3cn [2019/05/09 12:42] (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).\\ |
| 6 sets of silyl cyanide, SiH<sub>3</sub>CN, transitions with //J'// between 9 and 17 (between 89 and 170 GHz) were detected with the IRAM 30 m telescope in emission toward the late-type C-rich star CW Leonis. The //K// level structure is partly resolved. At least some degree of blending by emission lines of other molecules is present. | 6 sets of silyl cyanide, SiH<sub>3</sub>CN, transitions with //J'// between 9 and 17 (between 89 and 170 GHz) were detected with the IRAM 30 m telescope in emission toward the late-type C-rich star CW Leonis. The //K// level structure is partly resolved. At least some degree of blending by emission lines of other molecules is present. |
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