KMS of Xinjiang Astronomical Observatory, CAS
Determining the neutron star surface magnetic field strength of two Z sources | |
Ding, Guoqiang1![]() ![]() ![]() | |
2013-02-21 | |
Conference Name | IAU Symposium 290:Feeding Compact Objects: Accretion on All Scales |
Source Publication | Feeding Compact Objects: Accretion on All Scales, Proceedings of the International Astronomical Union, IAU Symposium 290 |
Volume | 290 |
Pages | 203-204 |
Conference Date | 20 - 24 August 2012 |
Correspondent Email | dinggq@gmail.com |
Conference Place | Beijing, China |
Publisher | Cambridge University Press |
Project Number | 2009CB824800 ; 11143013 |
Contribution Rank | 1 |
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 Organization | 973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 |
Keyword | Compact Object Neutron Star Accretion Disk |
DOI | 10.1017/S174392131201962X |
URL | 查看原文 |
Language | 英语 |
ISBN | 978-1-107-03379-5 |
Citation statistics | |
Document Type | 会议论文 |
Identifier | http://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 Author | Ding, Guoqiang |
Affiliation | 1.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 Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
Corresponding Author Affilication | Xinjiang 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. |
Files in This Item: | ||||||
File Name/Size | DocType | Version | Access | License | ||
Determining the neut(61KB) | 会议论文 | 开放获取 | CC BY-NC-SA | View Application Full Text |
Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Edit Comment