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Neutron Star Motion in the Disk Galaxy
Wei Ying-Chun; Taani, A.; Pan Yuan-Yue; Wang Jing; Cai Yan; Liu Gao-Chao; Luo A-Li; Zhang Hong-Bo; Zhao Yong-Heng
2010-11-01
发表期刊CHINESE PHYSICS LETTERS
卷号27期号:11
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.
DOI10.1088/0256-307X/27/11/119801
收录类别SCI
语种英语
WOS记录号WOS:000283725100059
引用统计
被引频次:2[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/7727
专题光学天文研究部
作者单位Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
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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).
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