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Is magnetar a fact or fiction to us?
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518-520
通讯作者Tong, H. ; Xu, R. X.
英文摘要The key point of studying AXPs/SGRs (anomalous X-ray pulsars/soft gamma-ray repeaters) is relevant to the energy budget. Historically, rotation was thought to be the only free energy of pulsar until the discovery of accretion power in X-ray binaries. AXPs/SGRs could be magnetars if they are magnetism-powered, but would alternatively be quark-star/fallback-disk systems if more and more observations would hardly be understood in the magnetar scenario.
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/45760611-7/1006]  
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.. Is magnetar a fact or fiction to us?[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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