Suzaku observations of non-thermal X-ray emission from galaxy clusters

被引：0
|
作者：
Kawano, N. [1 ]
Fukazawa, Y. [1 ]
Nakazawa, K. [2 ]
机构：
[1] Hiroshima Univ, Hiroshima 730, Japan
[2] USAS JAXA, Houston, TX USA
来源：
FIRST GLAST SYMPOSIUM | 2007年 / 921卷
关键词：
clusters of galaxies; non-thermal hard X-ray emission;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Clusters of galaxies are the largest gravitationally- bound system in the universe, and possible candidates of particle accelerator. The detection of diffuse radio emission, which is synchrotron emission caused by relativistic electrons, supports the scenario. The direct measurements by X-ray/Gamma-ray are important to clarify the non-thermal view of clusters. We present the initial hard X-ray research of galaxy clusters (especially for A3376) with Suzaku, which has excellent sensitivity in a few tens keV GLAST will make X-ray results be more valuable to discuss particle acceleration in galaxy clusters.
引用
收藏
页码：488 / +
页数：2
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