AXPs & SGRs: Magnetar or Quarctar?
文献类型：会议论文
| 作者 | Qiao, Guojun1; Liu, Xionwei1; Xu, Renxin1; Du, Yuanjie2; Han, Jinlin3; Tong, Hao4 ; Wang, Hongguang5
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| 出版日期 | 2013-02-21 |
| 会议名称 | IAU Symposium 291： Neutron Stars and Pulsars: Challenges and Opportunities after 80 years |
| 会议日期 | 20-31 August 2012 |
| 会议地点 | Beijing, China |
| 通讯作者邮箱 | 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 |
| 卷号 | 291 |
| 页码 | 474-476 |
| 通讯作者 | Qiao, Guojun ; Liu, Xionwei ; Xu, Renxin ; Du, Yuanjie ; Han, Jinlin ; Tong, Hao ; Wang, Hongguang |
| 英文摘要 | 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. |
| 会议主办者 | IAU |
| 会议网址 | http://www.pulsarastronomy.net/IAUS291/ |
| 会议录 | Neutron Stars and Pulsars: Challenges and Opportunities after 80 years, Proceedings of the International Astronomical Union, IAU Symposium 291
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| 会议录出版者 | Cambridge University Press |
| 语种 | 英语 |
| ISBN号 | 978-1-107-03380-1 |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/1007]  |
| 专题 | 脉冲星研究团组 新疆天文台_射电天文研究室 |
| 作者单位 | 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 |
| 推荐引用方式 GB/T 7714 | Qiao, Guojun,Liu, Xionwei,Xu, Renxin,et al. AXPs & SGRs: Magnetar or Quarctar?[C]. 见:IAU Symposium 291： Neutron Stars and Pulsars: Challenges and Opportunities after 80 years. Beijing, China. 20-31 August 2012.http://www.pulsarastronomy.net/IAUS291/. |
入库方式： OAI收割
来源：新疆天文台
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