The radio spectrum of Si3

被引:5
|
作者
McCarthy, MC
Thaddeus, P
机构
[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[2] Harvard Univ, Div Engn & Appl Sci, Cambridge, MA 02138 USA
来源
ASTROPHYSICAL JOURNAL | 2003年 / 592卷 / 02期
关键词
ISM : molecules; line : identification; molecular data; molecular processes; radio lines : ISM;
D O I
10.1086/375728
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The silicon trimer Si-3 and several of its rare isotopic species have been detected in the laboratory, and the frequencies of 66 rotational transitions in the range 5 - 42 GHz have been measured to a few parts in 10(7). The most intense radio lines can be calculated from the derived spectroscopic constants to better than 3 km s(-1) in equivalent radial velocity up to frequencies of 50 GHz, adequate for a deep search in the best astronomical sources; above that frequency the uncertainties increase to of the order of 20 km s(-1) at 160 GHz, which is still sufficient for a deep search in a wide-line source such as IRC + 10216.
引用
收藏
页码:L91 / L93
页数:3
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