neutronstarmotioninthediskgalaxy
文献类型：期刊论文
| 作者 | Wei Yingchun; A Taani; Pan Yuanyue; Wang Jing; Cai Yan ; Liu Gaochao; Luo Ali; Zhang Hongbo; Zhao Yongheng
|
| 刊名 | chinesephysicsletters
 |
| 出版日期 | 2010 |
| 卷号 | 027期号:011页码:119801 |
| ISSN号 | 0256-307X |
| 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 Poineare 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. |
| 语种 | 英语 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/41692]  |
| 专题 | 光学部_LAMOST运行和发展中心 |
| 作者单位 | 中国科学院国家天文台 |
| 推荐引用方式 GB/T 7714 | Wei Yingchun,A Taani,Pan Yuanyue,et al. neutronstarmotioninthediskgalaxy[J]. chinesephysicsletters,2010,027(011):119801. |
| APA | Wei Yingchun.,A Taani.,Pan Yuanyue.,Wang Jing.,Cai Yan.,...&Zhao Yongheng.(2010).neutronstarmotioninthediskgalaxy.chinesephysicsletters,027(011),119801. |
| MLA | Wei Yingchun,et al."neutronstarmotioninthediskgalaxy".chinesephysicsletters 027.011(2010):119801. |
入库方式： OAI收割
来源：国家天文台
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