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Determining the neutron star surface magnetic field strength of two Z sources
Ding, Guoqiang1; Huang, Chunping1,2; Wang, Yanan1,2
2013-02-21
Conference NameIAU Symposium 290:Feeding Compact Objects: Accretion on All Scales
Source PublicationFeeding Compact Objects: Accretion on All Scales, Proceedings of the International Astronomical Union, IAU Symposium 290
Volume290
Pages203-204
Conference Date20 - 24 August 2012
Correspondent Emaildinggq@gmail.com
Conference PlaceBeijing, China
PublisherCambridge University Press
Project Number2009CB824800 ; 11143013
Contribution Rank1
Abstract

From the extreme position of disk motion, we infer the neutron star (NS) surface magnetic field strength (B 0) of Z-source GX 17+2 and Cyg X-2. The inferred B 0 of GX 17+2 and Cyg X-2 are ~(1-5)¡Á108 G and ~(1-3)¡Á108 G, respectively, which are not inferior to that of millisecond X-ray pulsars or atoll sources. It is likely that the NS magnetic axis of Z sources is parallel to the axis of rotation, which could result in the lack of pulsations in these sources.

Funding Organization973项目 ; IAU ; 973项目 ; IAU ; 973项目 ; IAU ; 973项目 ; IAU ; 国家自然科学基金 ; 国家自然科学基金 ; 国家自然科学基金 ; 国家自然科学基金
KeywordCompact Object Neutron Star Accretion Disk
DOI10.1017/S174392131201962X
URL查看原文
Language英语
ISBN978-1-107-03379-5
Citation statistics
Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/978
Collection已撤销研究室/团组_高能天体物理研究团组
Corresponding AuthorDing, Guoqiang
Affiliation1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences,150, Science 1-Street, Urumqi, Xinjiang 830011, China
2.University of Chinese Academy of Sciences,China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Ding, Guoqiang,Huang, Chunping,Wang, Yanan. Determining the neutron star surface magnetic field strength of two Z sources[C]:Cambridge University Press,2013:203-204.
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