XAO OpenIR  > 射电天文研究室  > 脉冲星研究团组
AXPs & SGRs: Magnetar or Quarctar?
Qiao, Guojun1; Liu, Xionwei1; Xu, Renxin1; Du, Yuanjie2; Han, Jinlin3; Tong, Hao4; Wang, Hongguang5
2013-02-21
Conference NameIAU Symposium 291:Neutron Stars and Pulsars: Challenges and Opportunities after 80 years
Source PublicationNeutron Stars and Pulsars: Challenges and Opportunities after 80 years, Proceedings of the International Astronomical Union, IAU Symposium 291
Volume291
Pages474-476
Conference Date20-31 August 2012
Correspondent Emailgjn@pku.edu.cn ; xiongwliu@163.com ; r.x.xu@pku.edu.cn ; duyj@nssc.ac.cn ; hjl@nao.cas.cn ; tonghao@xao.ac.cn ; cosmic008@yahoo.com.cn
Conference PlaceBeijing, China
PublisherCambridge University Press
Project Number2009CB824800 ; 2012CB821800 ; 10935001 ; 10973002 ; 10833003 ; 11103021 ; 10821061 ; 10573002 ; 10778611 ; 10773016 ; 11073030 ; 305001
Contribution Rank4
Abstract

The concept of a "magnetar" was proposed mainly because of two factors. First, the X-ray luminosity of Anomalous X-ray Pulsars (AXPs) and Soft Gamma-Ray Repeaters (SGRs) is larger than the rotational energy loss rate (Lx > E rot ), and second, the magnetic field strength calculated from "normal method" is super strong. It is proposed that the radiation energy of magnetar comes from its magnetic fields. Here it is argued that the magnetic field strength calculated through the normal method is incorrect at the situation Lx > E rot , because the wind braking is not taken into account. Besides, the "anti-magnetar" and some other X-ray and radio observations are difficult to understand with a magnetar model.

Funding Organization973项目 ; IAU ; 973项目 ; IAU ; 国家自然科学基金 ; 国家自然科学基金 ; 教育部科学技术研究重点项目 ; 教育部科学技术研究重点项目
DOI10.1017/S1743921312024568
URL查看原文
Language英语
ISBN978-1-107-03380-1
Citation statistics
Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/1007
Collection射电天文研究室_脉冲星研究团组
射电天文研究室
Corresponding AuthorQiao, Guojun; Liu, Xionwei; Xu, Renxin; Du, Yuanjie; Han, Jinlin; Tong, Hao; Wang, Hongguang
Affiliation1.Department of Astronomy, Peking University, Beijing 100871, China
2.Center for Space Science and Applied Research, CAS, Beijing, 100190, China
3.National Astronomical Observatories, CAS, Beijing 100012, China
4.Xinjiang Astronomical Observatory, CAS, Urumqi, Xinjiang 830011, China
5.Center for Astrophysics, Guangzhou University, Guangzhou 510400, China
Recommended Citation
GB/T 7714
Qiao, Guojun,Liu, Xionwei,Xu, Renxin,et al. AXPs & SGRs: Magnetar or Quarctar?[C]:Cambridge University Press,2013:474-476.
Files in This Item:
File Name/Size DocType Version Access License
AXPs & SGRs_ Magneta(149KB)会议论文 开放获取CC BY-NC-SAView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Qiao, Guojun]'s Articles
[Liu, Xionwei]'s Articles
[Xu, Renxin]'s Articles
Baidu academic
Similar articles in Baidu academic
[Qiao, Guojun]'s Articles
[Liu, Xionwei]'s Articles
[Xu, Renxin]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Qiao, Guojun]'s Articles
[Liu, Xionwei]'s Articles
[Xu, Renxin]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: AXPs & SGRs_ Magnetar or Quarctar_.pdf
Format: Adobe PDF
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.