タイトル | Star formation in the cooling flows of M87/Virgo and NGC 1275/Perseus |
著者(英) | Sarazin, Craig L.; White, Raymond E., III |
著者所属(英) | Alabama Univ.|Virginia Univ.|Cambridge Univ. |
発行日 | 1988-12-15 |
言語 | eng |
内容記述 | X-ray observations indicate that M87/Virgo and NGC 1275/Perseus have cooling flows that are associated with accretion rates of 20-30 and 300-500 solar masses/year, respectively. An assessment is made as to whether star formation is necessarily occurring in these cooling flows by calculating constant mass-flux models for all reasonable parameter space. No constant-mass-flux models that are consistent with all of the relevant observations are found; hence, it is concluded that mass is dropping out of these cooling flows. |
NASA分類 | ASTROPHYSICS |
レポートNO | 89A20364 |
権利 | Copyright |
URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/366288 |