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Interstellar dust grains

被引：1863
作者：
Draine, BT [1 ]
机构：
[1] Princeton Univ Observ, Princeton, NJ 08544 USA
来源：
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS | 2003年 / 41卷
关键词：
infrared astronomy; interstellar medium; interstellar grains; light scattering; molecular clouds;
D O I：
10.1146/annurev.astro.41.011802.094840
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
This review surveys the observed properties of interstellar dust grains: the wavelength-dependent extinction of starlight, including absorption features, from UV to infrared; optical luminescence; infrared emission; microwave emission; optical, UV, and X-ray scattering by dust; and polarization of starlight and of infrared emission. The relationship between presolar grains in meteorites and the interstellar grain population is discussed. Candidate grain materials and abundance constraints are considered. A dust model consisting of amorphous silicate grains, graphite grains, and polycyclic aromatic hydrocarbons is compared with observed emission and scattering. Some issues concerning evolution of interstellar dust are discussed.
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收藏
页码：241 / 289
页数：49
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