| Автор | Sofue, Yoshiaki |
| Автор | Rubin, Vera |
| Дата выпуска | 2001 |
| dc.description | ▪ Abstract 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. |
| Формат | application.pdf |
| Издатель | Annual Reviews |
| Копирайт | Annual Reviews |
| Название | ROTATION CURVES OF SPIRAL GALAXIES |
| DOI | 10.1146/annurev.astro.39.1.137 |
| Print ISSN | 0066-4146 |
| Журнал | Annual Review of Astronomy and Astrophysics |
| Том | 39 |
| Первая страница | 137 |
| Последняя страница | 174 |
| Аффилиация | Sofue, Yoshiaki; Institute of Astronomy, University of Tokyo, Mitaka Tokyo 181-0015, Japan, e-mail: sofue@ioa.s.u-tokyo.ac.jp |
