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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.
引用
收藏
页码：241 / 289
页数：49
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