Neutron Star Motion in the Disk Galaxy

	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
刊名	CHINESE PHYSICS LETTERS
	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
内容类型	期刊论文
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).