Suzaku Observation of Nearby On-Going Merger Cluster Abell 3627

被引:8
|
作者
Nishino, Sho [1 ]
Fukazawa, Yasushi [1 ]
Hayashi, Katsuhiro [1 ]
机构
[1] Hiroshima Univ, Dept Phys Sci, Hiroshima 7398526, Japan
基金
日本学术振兴会;
关键词
galaxies: clusters: individual (Abell 3627); X-rays: galaxies: clusters; MASSIVE GALAXY CLUSTER; X-RAY-DETECTOR; BOARD SUZAKU; TEMPERATURE MAP; GREAT ATTRACTOR; MILKY-WAY; ASCA; REPRODUCIBILITY; A3627; TAIL;
D O I
10.1093/pasj/64.1.16
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of the Suzaku observation of a nearby (z = 0.016), on-going merger cluster, Abell 3627. The overall temperature of the ICM is around 7 keV, and we found a cool region with k(T) similar to 4-5 keV at the position corresponding to the brightness excess from a spherically symmetrical beta-model found by ROSAT. This structure seems to be a subcluster colliding into the main body. In the temperature and density profiles, no apparent jump associated with a shock is confirmed at the colliding position; therefore, the velocity of the subcluster seems to be subsonic. On the other hand, the line-of-sight velocity of the subcluster is strictly restricted to be less than 800 km s(-1) using the Doppler shift of the Fe-K lines. Moreover, our ICM temperature map also suggests the possibility of another merging subcluster in the north-west region. A 3627 is now in the process of an aggressive cluster merger, associated with the formation of a large-scale structure.
引用
收藏
页数:10
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