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THE SPIN-UP OF ACCRETING NEUTRON STARS IN BINARY SYSTEMS
Wang, J.; Zhang, C. M.; Zhao, Y. H.
2011-09-01
发表期刊INTERNATIONAL JOURNAL OF MODERN PHYSICS D
卷号20期号:10页码:2019-2022
摘要In binary systems, the rotation of neutron stars can be spun up by the accreted material, and at the same time the decay of their magnetic fields occur in the accretion phase. As a result, the spin period may arrive at a minimum of about 1.5 ms, corresponding to a bottom value of the magnetic field similar to 10(8) G. Taking the conditions: (i) initial magnetic field varying from 10(11) G to 10(13) G while setting period as 100 s, (ii) initial period as 1-100 s at B = 5 x 10(12) G, we find that this minimum of spin period seems independent of these initial conditions.
关键词Neutron Stars Pulsars Magnetic Field Spin Period Binary
DOI10.1142/S021827181102010X
收录类别SCI
语种英语
WOS记录号WOS:000295277300033
引用统计
文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/7908
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
Wang, J.,Zhang, C. M.,Zhao, Y. H.. THE SPIN-UP OF ACCRETING NEUTRON STARS IN BINARY SYSTEMS[J]. INTERNATIONAL JOURNAL OF MODERN PHYSICS D,2011,20(10):2019-2022.
APA Wang, J.,Zhang, C. M.,&Zhao, Y. H..(2011).THE SPIN-UP OF ACCRETING NEUTRON STARS IN BINARY SYSTEMS.INTERNATIONAL JOURNAL OF MODERN PHYSICS D,20(10),2019-2022.
MLA Wang, J.,et al."THE SPIN-UP OF ACCRETING NEUTRON STARS IN BINARY SYSTEMS".INTERNATIONAL JOURNAL OF MODERN PHYSICS D 20.10(2011):2019-2022.
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