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What can Fermi tell us about magnetars?
Tong,H.1; Xu,R.X.2
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
通讯作者邮箱tonghao@xao.ac.cn ; r.x.xu@pku.edu.cn
会议地点Beijing, China
关键词pulsars: general stars: magnetars stars: neutron
卷号291
页码521-523
通讯作者Tong, H. ; Xu, R. X.
英文摘要We have analyzed the physical implications of Fermi observations of magnetars. Observationally, no significant detection is reported in Fermi observations of all magnetars. Then there are conflicts between outer gap model in the case of magnetars and Fermi observations. One possible explanation is that magnetars are wind braking instead of magnetic dipole braking. In the wind braking scenario, magnetars are neutron stars with strong multipole field. A strong dipole field is no longer required. A magnetism-powered pulsar wind nebula and a braking index smaller than three are the two predictions of wind braking of magnetars. Future deeper Fermi observations will help us make clear whether they are wind braking or magnetic dipole braking. It will also help us to distinguish between the magnetar model and the accretion model for AXPs and SGRs.
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
会议录出版者Cambridge University Press
语种英语
ISBN号978-1-107-03380-1
内容类型会议论文
源URL[http://ir.xao.ac.cn/handle/45760611-7/1005]  
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.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, Xinjiang 830011, China
2.School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China
推荐引用方式
GB/T 7714
Tong,H.,Xu,R.X.. What can Fermi tell us about magnetars?[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/.
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