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| molecules:ism:sih [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:sih [2019/10/18 13:02] (current) – mueller |
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| The tentative identification of silylidyne, SiH, toward Orion KL was reported by\\ | The tentative identification of silylidyne, SiH, toward Orion KL was reported by\\ |
| P. Schilke, D. J. Benford, T. R. Hunter, D. C. Lis, and T. G. Philips,\\ | P. Schilke, D. J. Benford, T. R. Hunter, D. C. Lis, and T. G. Philips,\\ |
| **[[http://dx.doi.org/10.1086/318951|A Line Survey of Orion-KL from 607 to 725 GHz]]**\\ | **[[https://doi.org/10.1086/318951|A Line Survey of Orion-KL from 607 to 725 GHz]]**\\ |
| //Astrophys. J. Suppl. Ser.// **132**, 281–364 (2001).\\ | //Astrophys. J. Suppl. Ser.// **132**, 281–364 (2001).\\ |
| The two λ components of the //J// = 1.5 – 0.5 transition pertaining to the energetically lower lying Π<sub>1/2</sub> spin-state near 624.9 and 627.7 GHz were detected. However, they were at least partially overlapped. As the source is rather line rich, the detection was viewed as tentative. | The two λ components of the //J// = 1.5 – 0.5 transition pertaining to the energetically lower lying Π<sub>1/2</sub> spin-state near 624.9 and 627.7 GHz were detected. However, they were at least partially overlapped. As the source is rather line rich, the detection was viewed as tentative. |
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| Contributor(s): H. S. P. Müller; 06, 2006 | Contributor(s): H. S. P. Müller; 06, 2006 |
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