Enigmatic emission

被引:0
|
作者
Takeshi Oka
机构
[1] Enrico Fermi Institute,Department of Astronomy and Astrophysics and the Department of Chemistry
[2] University of Chicago,undefined
来源
Nature | 2002年 / 418卷
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D O I
暂无
中图分类号
学科分类号
摘要
The detection of infrared emission from the dusty disk around a distant star signals the presence of the H3+ ion. The finding may provide a vital clue to how hydrogen and helium condense into gas-giant planets.
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页码:31 / 33
页数:2
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