| タイトル | The prevalence of cooling flows in clusters of galaxies |
| 著者（英） | Forman, W.; Stewart, G. C.; Jones, C.; Fabian, A. C. |
| 著者所属（英） | Harvard-Smithsonian Center for Astrophysics|Cambridge Univ. |
| 発行日 | 1984-10-01 |
| 言語 | eng |
| 内容記述 | The central density and temperature of the intracluster gas in 36 clusters of galaxies have been determined by deprojection of the X-ray surface brightness distribution. The cooling time of the gas in half of these clusters is less than a Hubble time (50 km/s per Mpc). For these clusters mass inflow rates between 2 and 400 solar mass per year are derived. These cooling flows may provide a significant fraction of the mass of the central cD galaxies. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 85A13826 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/394271 |
