X-ray lines in gamma-ray bursts and Cerenkov line emissions

被引：0

作者：

Wang, W ^{[1
]}

机构：

[1] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China

来源：

1604-2004: SUPERNOVAE AS COSMOLOGICAL LIGHTHOUSES | 2005年 / 342卷

关键词：

DISCOVERY; AFTERGLOW; SUPERNOVA;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

X-ray emission and absorption features are of great importance in our understanding the nature and environment of gamma-ray bursts (GRBs). Iron emission lilies have been detected in at least four GRB afterglows, which provides the new evidence for the connection between supernovae (SNe) and GRBs. In this paper, we will specially concentrate on the Cerenkov line mechanism, in which broad iron lines are expected, and a small mass of Fe is required to produce the large line luminosity. In addition, our interpretation can favor the recent jet unified model for different classes of gamma-ray bursts with a standard energy reservoir.

引用

页码：346 / 348

页数：3

共 12 条

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