| Be／X射线双星的多波段观测 |
| |
| 引用本文： | 刘庆忠,杭恒荣.Be／X射线双星的多波段观测[J].天文学进展,1997,15(2):137-144. |
| |
| 作者姓名： | 刘庆忠 杭恒荣 |
| |
| 作者单位： | 中国科学院紫金山天山台!南京，210008，中国科学院紫金山天山台!南京，210008 |
| |
| 基金项目： | 国家自然科学基金，中国科学院天文委员会资助 |
| |
| 摘 要： | 简要地回顾了Ｂｅ／Ｘ射线双星２０多年来在红外、可见光、紫外和Ｘ射线波段所取得的观测结果，着重介绍了多波段联合观测对探讨双星间的相互作用如中子星的吸积方式和Ｘ射线产生的原因等方面的意义，对这些观测结果的分析研究，将是人们了解Ｂｅ／Ｘ射线双星的轨道参数和双星的物理参数、建立理论模型的基础。
|
| 关 键 词： | 双星 X射线 紫外线 多波段观测 |
Multiwaveband Study of Be/X-ray Binaries |
| |
| Liu Qingzhong, Hang Hengrong.Multiwaveband Study of Be/X-ray Binaries[J].Progress In Astronomy,1997,15(2):137-144. |
| |
| Authors: | Liu Qingzhong Hang Hengrong |
| |
| Abstract: | The multiwaveband observational results of Be/X-ray binaries, obtained both on groundbased optical and IR observation and on the satellite UV and X-ray observation for about twentyyearsj are briefly illtroduced, from which the interaction b~en Be and neutron stars can bededuced, such as the accretion mode of neutron star and the mechanism for X-ray burst. Themultiwaveband study can also provide us with the physical parameters of both orbit and binary,and also provide observational evidences for establishing theoretical models. |
| |
| Keywords: | binaries: spectroscopic-X mys: stars-ultravoilet: stars-infrared: stars |
| 本文献已被 CNKI 维普 等数据库收录！ |
