Neutron Star Motion in the Disk Galaxy
文献类型：期刊论文
| 作者 | Wei Ying-Chun; Taani, A.; Pan Yuan-Yue; Wang Jing ; Cai Yan; Liu Gao-Chao; Luo A-Li; Zhang Hong-Bo; Zhao Yong-Heng
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| 刊名 | CHINESE PHYSICS LETTERS
 |
| 出版日期 | 2010-11-01 |
| 卷号 | 27期号:11 |
| 英文摘要 | The neutron star motions are based on the undisturbed finitely thick galactic disk gravitational potential model. Two initial conditions, i.e. the locations and velocities, are considered. The Monte Carlo method is employed to separate rich diversities of the orbits of neutron stars into several sorts. The Poincare section has the potential to play an important role in the diagnosis of the neutron star motion. It has been observed that the increasing ratio of the motion range vertical to the galactic plane to that parallel to the galactic plane results in the irregularity of neutron star motion. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000283725100059 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/7727]  |
| 专题 | 国家天文台_光学天文研究部 |
| 作者单位 | Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
| 推荐引用方式 GB/T 7714 | Wei Ying-Chun,Taani, A.,Pan Yuan-Yue,et al. Neutron Star Motion in the Disk Galaxy[J]. CHINESE PHYSICS LETTERS,2010,27(11). |
| APA | Wei Ying-Chun.,Taani, A..,Pan Yuan-Yue.,Wang Jing.,Cai Yan.,...&Zhao Yong-Heng.(2010).Neutron Star Motion in the Disk Galaxy.CHINESE PHYSICS LETTERS,27(11). |
| MLA | Wei Ying-Chun,et al."Neutron Star Motion in the Disk Galaxy".CHINESE PHYSICS LETTERS 27.11(2010). |
入库方式： OAI收割
来源：国家天文台
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