Is magnetar a fact or fiction to us?
文献类型:会议论文
作者 | Tong,H.1; Xu,R.X.2 |
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 | tonghao@xao.ac.cn ; r.x.xu@pku.edu.cn |
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 |
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/. |
入库方式: OAI收割
来源:新疆天文台
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