The effect of the stellar wind velocity on the eccentric-orbit binary model |
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| Authors: | Toru Okuda Shiro Sakashita |
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| Affiliation: | (1) Institute of Earth Science, Hokkaido University of Education, Hakodate, Japan;(2) Dept. of Physics, Hokkaido University, Sapporo, Japan |
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| Abstract: | The previous eccentric-orbit binary model for the recurrent X-ray sources is modified by taking account of the velocity field of the stellar wind. The resultant formula of the light curves for the X-ray sources may have an useful application to the observed X-ray sources. |
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