Metal hydrides in astronomy

被引：0
|
作者：
Bernath, Peter [1 ]
机构：
[1] Univ Waterloo, Dept Chem, Waterloo, ON N2L 3G1, Canada
来源：
Astrochemistry: From Laboratory Studies to Astronomical Observations | 2006年 / 855卷
关键词：
stellar atmospheres; molecular opacities; metal hydrides;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Metal hydride molecules are important in astronomy: they are found in sunspots, cool stellar atmospheres and in substellar objects called brown dwarfs. Molecular opacities needed to simulate the spectral energy distributions emitted by these objects. The astronomical observation of metal hydrides is reviewed and the calculation of opacities is discussed for CrH, FeH and TiH.
引用
收藏
页码：143 / 148
页数：6
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