Diffuse interstellar absorption bands

被引:2
作者
Xiang FuYun [1 ,2 ]
Liang ShunLin [1 ]
Li AiGen [1 ,3 ]
机构
[1] Univ Missouri, Dept Phys & Astron, Columbia, MO 65211 USA
[2] Xiangtan Univ, Fac Mat Photoelect & Phys, Xiangtan 411105, Peoples R China
[3] Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
来源
SCIENCE IN CHINA SERIES G-PHYSICS MECHANICS & ASTRONOMY | 2009年 / 52卷 / 04期
基金
中国国家自然科学基金; 美国国家科学基金会;
关键词
astrophysics; interstellar matter; interstellar extinction; diffuse interstellar band; circumstellar environment; POLYCYCLIC AROMATIC-HYDROCARBONS; HIGH-RESOLUTION PROFILES; HIGHLY UNSATURATED-HYDROCARBONS; ULTRAVIOLET EXTINCTION; INFRARED-EMISSION; UV EXTINCTION; ISO-SWS; FEATURES; DUST; SPECTRA;
D O I
10.1007/s11433-009-0082-5
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The diffuse interstellar bands (DIBs) are a large number of absorption bands that are superposed on the interstellar extinction curve and are of interstellar origin. Since the discovery of the first two DIBs in the 1920s, the exact nature of DIBs still remains unclear. This article reviews the history of the detections of DIBs in the Milky Way and external galaxies, the major observational characteristics of DIBs, the correlations or anti-correlations among DIBs or between DIBs and other interstellar features (e.g. the prominent 2175 Angstrom extinction bump and the far-ultraviolet extinction rise), and the proposed candidate carriers. Whether they are also present in circumstellar environments is also discussed.
引用
收藏
页码:489 / 501
页数:13
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