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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
AbstractThe 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.
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WOS IDWOS:000283725100059
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Cited Times:2[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
AffiliationChinese 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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