Magnetic field and spin frequency of X-ray neutron star associated with the kHz QPOs
文献类型:期刊论文
作者 | Zhang, Chengmin![]() |
刊名 | ADVANCES IN SPACE RESEARCH
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出版日期 | 2007 |
卷号 | 40期号:10页码:1480-1484 |
关键词 | magnetic field of neutron star spin frequency of pulsar kHz QPOs binary system |
英文摘要 | By means of the accretion induced magnetic field evolution model of neutron star in low mass X-ray binary, the star spin frequency evolution has been studied, and we find that the star spin frequency is almost independent of the mass accretion rate, initial magnetic field and initial period, when the star magnetosphere evolves less than about five star radii with the spin frequency of about 100 Hz. However, the similar distributions of kHz QPOs in the bright Z sources (similar to Eddington accretion rate) and in the less luminous Atoll ones (-1% Eddington accretion rate) imply that both sources share the similar magnetosphere radii and spin frequencies, which is consistent with our theoretical model. (C) 2007 Published by Elsevier Ltd on behalf of COSPAR. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000253590100009 |
源URL | [http://ir.bao.ac.cn/handle/114a11/7244] ![]() |
专题 | 国家天文台_射电天文研究部 |
作者单位 | Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Zhang, Chengmin. Magnetic field and spin frequency of X-ray neutron star associated with the kHz QPOs[J]. ADVANCES IN SPACE RESEARCH,2007,40(10):1480-1484. |
APA | Zhang, Chengmin.(2007).Magnetic field and spin frequency of X-ray neutron star associated with the kHz QPOs.ADVANCES IN SPACE RESEARCH,40(10),1480-1484. |
MLA | Zhang, Chengmin."Magnetic field and spin frequency of X-ray neutron star associated with the kHz QPOs".ADVANCES IN SPACE RESEARCH 40.10(2007):1480-1484. |
入库方式: OAI收割
来源:国家天文台
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