中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Merger Dynamics of the Pair of Galaxy Clusters--A399 and A401

文献类型:期刊论文

作者Yuan Qirong3; Yan Pengfei2; Yang Yanbin1; Xu Zhou1
刊名Chinese Journal of Astronomy and Astrophysics
出版日期2005
卷号5期号:2页码:126
ISSN号1009-9271
英文摘要Convincing evidence for a past interaction between the two rich clusters A399 and A401 was recently found in the X-ray imaging observations. We examine the structure and dynamics of this pair of galaxy clusters. A mixture-modeling algorithm was applied to obtain a robust partition into two clusters, which allowed us to discuss the virial mass and velocity distribution of each cluster. Assuming that these two clusters follow a linear orbit and they have once experienced a close encounter, we model the binary cluster as a two-body system. As a result, four gravitationally bound solutions are obtained. The recent X-ray observations seem to favor a scenario in which the two clusters with a true separation of 5.4h-1 Mpc are currently expanding at 583 km s-1along a direction with a projection angle of 67.5°, and they will reach a maximum extent of 5.65 h-1 Mpc in about 1.0 h-1 Gyr.
语种英语
源URL[http://ir.bao.ac.cn/handle/114a11/45876]  
专题中国科学院国家天文台
作者单位1.中国科学院国家天文台
2.青岛科技大学
3.南京师范大学
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GB/T 7714
Yuan Qirong,Yan Pengfei,Yang Yanbin,et al. Merger Dynamics of the Pair of Galaxy Clusters--A399 and A401[J]. Chinese Journal of Astronomy and Astrophysics,2005,5(2):126.
APA Yuan Qirong,Yan Pengfei,Yang Yanbin,&Xu Zhou.(2005).Merger Dynamics of the Pair of Galaxy Clusters--A399 and A401.Chinese Journal of Astronomy and Astrophysics,5(2),126.
MLA Yuan Qirong,et al."Merger Dynamics of the Pair of Galaxy Clusters--A399 and A401".Chinese Journal of Astronomy and Astrophysics 5.2(2005):126.

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来源:国家天文台

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