Short-living supermassive magnetar model for the early X-ray flares following short GRBs

被引：104

作者：

Gao, Wei-Hong ^{[1
]}

Fan, Yi-Zhong

机构：

[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

来源：

CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS | 2006年 / 6卷 / 05期

关键词：

gamma-rays : bursts; radiation mechanisms : nonthermal; magnetic fields; stars : neutron; stars : rotation;

D O I：

10.1088/1009-9271/6/5/01

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

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.

引用

页码：513 / 516

页数：4

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