GLAST simulation study of an extended TeV-emitting supernova remnant for the origin of cosmic-ray nuclei

被引：0
|
作者：
Katagiri, H. [1 ]
Yoshida, H. [1 ]
Mizuno, T. [1 ]
Takahashi, H. [1 ]
Fukazawa, Y. [1 ]
Ohsugi, T. [1 ]
机构：
[1] Hiroshima Univ, Grad Sch Sci, Dept Phys Sci, 1-3-1 Kagamiyama, Higashihiroshima 7398526, Japan
来源：
FIRST GLAST SYMPOSIUM | 2007年 / 921卷
关键词：
GLAST; gamma-ray; cosmic ray; supernova remnant; TeV;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We extracted the gamma-ray emission of the pi(0)-decay, which will be a decisive evidence of cosmic-ray proton acceleration, from the one-year data of an extended TeV-emitting supemova remnant, generated by the GLAST full detector simulation, although many assumptions were oversimplified.
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页码：397 / +
页数：2
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