| タイトル | X-ray emission from Be star binaries |
| 著者（英） | Apparao, K. M. V. |
| 著者所属（英） | NASA Marshall Space Flight Center|Tata Inst. of Fundamental Research |
| 発行日 | 1985-05-01 |
| 言語 | eng |
| 内容記述 | A model in which a neutron star in an eccentric inclined orbit around a Be star passes through a ring of matter around the Be star has been used to explain the recurrent flares of X-ray emission from these systems. The optical emission during X-ray flares is due to partial absorption and reprocessing of the X-rays in the ring. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 85A35430 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/391302 |
