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题名: THE CRUST SCREEN MODEL FOR THE MAGNETIC-FIELD OF BINARY-X-RAY SOURCES
作者: ZHANG, CM ;  WU, XJ ;  YANG, GC
刊名: ASTRONOMY AND ASTROPHYSICS
出版日期: 1994
卷号: 283, 期号:3, 页码:889-892
关键词: NEUTRON-STAR ;  PULSAR ;  DECAY ;  ACCRETION ;  EVOLUTION ;  ORIGIN ;  PERIOD
学科分类: Physics
通讯作者: ZHANG, CM , HEBEI INST TECHNOL,DEPT PHYS,BOX 146,TIANJIN 300130,PEOPLES R CHINA.
部门归属: ACAD SINICA,INST THEORET PHYS,BEIJING 100080,PEOPLES R CHINA; CCAST WORLD LAB,CTR ASTRON & ASTROPHYS,BEIJING 100080,PEOPLES R CHINA; BEIJING UNIV,DEPT GEOPHYS,BEIJING 100080,PEOPLES R CHINA
英文摘要: It is assumed that the compressed accretion matter on the crust of a neutron star with magnetic field has ferromagnetic permeability. The observed inverse correlation between field strength and accreted mass can be deduced, by means of the analytic calculation of a proposed crust screen model. The field-period relation P = 2.7 ms B-9(5/7) is also presented, which fits for the equilibrium period line of X-ray binary sources.
收录类别: SCI
原文出处: 查看原文
WOS记录号: WOS:A1994NC57600024
Citation statistics: 
内容类型: 期刊论文
URI标识: http://ir.itp.ac.cn/handle/311006/11946
Appears in Collections:理论物理所1978-2010年知识产出_期刊论文

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Recommended Citation:
ZHANG, CM,WU, XJ,YANG, GC. THE CRUST SCREEN MODEL FOR THE MAGNETIC-FIELD OF BINARY-X-RAY SOURCES[J]. ASTRONOMY AND ASTROPHYSICS,1994,283(3):889-892.
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