Institutional Repository of Radio Astronomy Research Laboratory
AXPs & SGRs: Magnetar or Quarctar? | |
Qiao, Guojun1; Liu, Xionwei1; Xu, Renxin1; Du, Yuanjie2; Han, Jinlin3; Tong, Hao4![]() | |
2013-02-21 | |
Conference Name | IAU Symposium 291:Neutron Stars and Pulsars: Challenges and Opportunities after 80 years |
Source Publication | Neutron Stars and Pulsars: Challenges and Opportunities after 80 years, Proceedings of the International Astronomical Union, IAU Symposium 291 |
Volume | 291 |
Pages | 474-476 |
Conference Date | 20-31 August 2012 |
Correspondent Email | gjn@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 Place | Beijing, China |
Publisher | Cambridge University Press |
Project Number | 2009CB824800 ; 2012CB821800 ; 10935001 ; 10973002 ; 10833003 ; 11103021 ; 10821061 ; 10573002 ; 10778611 ; 10773016 ; 11073030 ; 305001 |
Contribution Rank | 4 |
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 Organization | 973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 |
DOI | 10.1017/S1743921312024568 |
URL | 查看原文 |
Language | 英语 |
ISBN | 978-1-107-03380-1 |
Citation statistics | |
Document Type | 会议论文 |
Identifier | http://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 Author | Qiao, Guojun; Liu, Xionwei; Xu, Renxin; Du, Yuanjie; Han, Jinlin; Tong, Hao; Wang, Hongguang |
Affiliation | 1.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. |
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AXPs & SGRs_ Magneta(149KB) | 会议论文 | 开放获取 | CC BY-NC-SA | View Application Full Text |
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