Rotation curves of spiral galaxies

被引：697

作者：

Sofue, Y ^{[1
]}

Rubin, V

机构：

[1] Univ Tokyo, Inst Astron, Mitaka, Tokyo 1810015, Japan

[2] Carnegie Inst Sci, Dept Terr Magnetism, Washington, DC 20015 USA

来源：

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS | 2001年 / 39卷

关键词：

D O I：

10.1146/annurev.astro.39.1.137

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Rotation curves of spiral galaxies are the major tool for determining the distribution of mass in spiral galaxies. They provide fundamental information for understanding the dynamics, evolution, and formation of spiral galaxies. We describe various methods to derive rotation curves and review the results obtained. We discuss the basic characteristics of observed rotation curves in relation to various galaxy properties, such as Hubble type, structure, activity, and environment.

引用

页码：137 / 174

页数：38

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