Dust formation in nova winds

被引：0
作者：
A. Evans
机构：
[1] Keele University,Department of Physics
来源：
Astrophysics and Space Science | 2001年 / 275卷
关键词：
Oxygen; Dust; Dust Formation; Classical Nova; Abundance Effect;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
We review the properties of classical novae, with particular emphasison their dust formation. Recent observational and theoretical workindicates that CO formation in nova winds does not go to saturation,so that both oxygen- and carbon-rich condensates can appearsimultaneously in the ejected material. The UIR carrier in novaeappears to be near-unique to novae, although whether this is due toenvironmental, excitation or abundance effects is not yet clear.
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页码：131 / 141
页数：10
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