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| Two predictions for the spin down behavior of magnetar SGR J1745-2900 | |
Tong, Hao
| |
| 2015-03-01 | |
| Conference Name | Quarks and Compact Stars 2014 |
| Source Publication | Proceedings of quarks and compact stars |
| Volume | 56 |
| Issue | Suppl. |
| Pages | 73-75 |
| Conference Date | Oct. 20-22, 2014 |
| Correspondent Email | tonghao@xao.ac.cn |
| Conference Place | KIAA at Peking University, Beijing, China |
| Publisher | Acta Astronomica Sinica |
| Project Number | LHXZ201201 ; 2015CB857100 |
| Contribution Rank | 1 |
| Abstract | The basic concepts of wind braking of magnetars, and its applications to various timing events of magnetars are outlined. The case of the Galactic centre magnetar SGR J1745-2900 is especially discussed. Two predictions for SGR J1745-2900 are made (the period derivative will first increase then decrease; and possible outbursts in the near future). |
| Funding Organization | Xinjiang Bairen project ; Xinjiang Bairen project ; West Light Foundation of CAS (LHXZ201201) ; West Light Foundation of CAS (LHXZ201201) ; Qing Cu Hui of CAS ; Qing Cu Hui of CAS ; 973 Program(2015CB857100) ; 973 Program(2015CB857100) |
| Keyword | Pulsars Individual: (Sgr J1745−2900) Stars: Magnetar Wind |
| URL | 查看原文 |
| Indexed By | 其他 |
| Language | 英语 |
| Document Type | 会议论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/1731 |
| Collection | 射电天文研究室_脉冲星研究团组 射电天文研究室 |
| Corresponding Author | Tong, Hao |
| Affiliation | Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, 830011, China |
| First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Recommended Citation GB/T 7714 | Tong, Hao. Two predictions for the spin down behavior of magnetar SGR J1745-2900[C]:Acta Astronomica Sinica,2015:73-75. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| Tong-2015-Two predic（144KB） | 会议论文 | 开放获取 | CC BY-NC-SA | View Application Full Text | ||
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