Short-living supermassive magnetar model for the early X-ray flares following short GRBs | |
Gao, Wei-Hong; Fan, Yi-Zhong | |
刊名 | CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS |
2006 | |
卷号 | 6期号:5页码:513-516 |
关键词 | gamma-rays : bursts radiation mechanisms : nonthermal magnetic fields stars : neutron stars : rotation |
ISSN号 | 1009-9271 |
英文摘要 | We suggest a short-lived supermassive magnetar model to account for the X-ray flares following short gamma-ray bursts. In this model the central engine of the short gamma-ray bursts is a supermassive millisecond magnetar, formed in coalescence of double neutron stars. The X-ray flares are powered by the dipole radiation of the magnetar. When the magnetar has lost a significant part of its angular momentum, it collapses to a black hole and the X-ray flares cease abruptly. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | HIGH-RESOLUTION CALCULATIONS ; MERGING NEUTRON-STARS ; GENERAL-RELATIVITY ; BURST AFTERGLOWS ; ACCRETION DISK ; GRB-050709 ; ORIGIN ; STATE |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000241487800001 |
公开日期 | 2012-02-07 |
内容类型 | 期刊论文 |
源URL | [http://159.226.72.40/handle/332002/3616] |
专题 | 紫金山天文台_宇宙伽马暴、中子星及相关物理研究团组 |
作者单位 | 1.Nanjing Normal Univ, Dept Phys, Nanjing 210008, Peoples R China 2.Nanjing Normal Univ, Inst Theoret Phys, Nanjing 210008, Peoples R China 3.Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel 4.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China |
推荐引用方式 GB/T 7714 | Gao, Wei-Hong,Fan, Yi-Zhong. Short-living supermassive magnetar model for the early X-ray flares following short GRBs[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2006,6(5):513-516. |
APA | Gao, Wei-Hong,&Fan, Yi-Zhong.(2006).Short-living supermassive magnetar model for the early X-ray flares following short GRBs.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,6(5),513-516. |
MLA | Gao, Wei-Hong,et al."Short-living supermassive magnetar model for the early X-ray flares following short GRBs".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 6.5(2006):513-516. |
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