| タイトル | X-ray sources in stellar winds |
| 著者（英） | Hatchett, S.; Mccray, R. |
| 著者所属（英） | Colorado Univ. |
| 発行日 | 1977-01-15 |
| 言語 | eng |
| 内容記述 | A model of a binary X-ray source immersed in a stellar wind from its companion star is considered. The geometry of the constant ionization and temperature contours in the model is discussed, and X-ray radiative transfer through the wind is described. The results are applied to make predictions about the presence and variability of iron K-shell fluorescence lines, to explain the light curve of Cen X-3 during a 'low' to 'high' state transition in July 1972, and to predict variability with orbital phase of resonance ultraviolet lines such as N V at 1238 and 1242 A from the binary system. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 77A21071 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/439340 |
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