Major Dry-Merger Rate and Extremely Massive Dry-Mergers of BCGs
被引:0
作者:
Liu, F. S.
论文数: 0引用数: 0
h-index: 0
机构:
Shenyang Normal Univ, Coll Phys Sci & Technol, Shenyang 110034, Peoples R ChinaShenyang Normal Univ, Coll Phys Sci & Technol, Shenyang 110034, Peoples R China
Liu, F. S.
[1
]
Deng, Z. G.
论文数: 0引用数: 0
h-index: 0
机构:
Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R ChinaShenyang Normal Univ, Coll Phys Sci & Technol, Shenyang 110034, Peoples R China
Deng, Z. G.
[3
]
Xia, X. Y.
论文数: 0引用数: 0
h-index: 0
机构:
Tianjin Normal Univ, Dept Phys, Tianjin, Peoples R ChinaShenyang Normal Univ, Coll Phys Sci & Technol, Shenyang 110034, Peoples R China
Xia, X. Y.
[2
]
机构:
[1] Shenyang Normal Univ, Coll Phys Sci & Technol, Shenyang 110034, Peoples R China
[2] Tianjin Normal Univ, Dept Phys, Tianjin, Peoples R China
[3] Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China
来源:
RELATIVISTIC ASTROPHYSICS
|
2008年
/
1059卷
关键词:
galaxies: cD;
galaxies:cluster of galaxies;
galaxies:merger;
galaxies:photometry;
D O I:
暂无
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Possible ongoing dry merger pairs of the early type Brightest Cluster Galaxies (BCGs) have been searched from a sample of 515 BCGs with redshifts between 0.03 to 0.12 selected from the C4 cluster catalogue. The results are compared with those of GEMS (Galaxy Evolution from Morphology and SEDs Survey) [1]. We find that BCGs have much higher ongoing merger fraction than that of luminous early-type galaxies from GEMS. This may infer that BCGs have higher dry-merger rate. We also found the trendence that the BCGs in richer clusters tend to have higher merger fraction than that in poorer clusters. With careful inspection, we find that extremely massive major dry mergers do exist in the BCGs sample which shows that they are not rare locally and may have important implication on the evolution of BCGs.
机构:
Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Chinese Acad Sci, Grad Sch, Beijing 100049, Peoples R China
Tianjin Normal Univ, Dept Phys, Tianjin 300074, Peoples R ChinaChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Liu, F. S.
;
Xia, X. Y.
论文数: 0引用数: 0
h-index: 0
机构:
Tianjin Normal Univ, Dept Phys, Tianjin 300074, Peoples R ChinaChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Xia, X. Y.
;
Mao, Shude
论文数: 0引用数: 0
h-index: 0
机构:
Tianjin Normal Univ, Dept Phys, Tianjin 300074, Peoples R China
Univ Manchester, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, EnglandChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Mao, Shude
;
Wul, Hong
论文数: 0引用数: 0
h-index: 0
机构:
Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R ChinaChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Wul, Hong
;
Deng, Z. G.
论文数: 0引用数: 0
h-index: 0
机构:
Chinese Acad Sci, Grad Sch, Beijing 100049, Peoples R ChinaChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
机构:
Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Chinese Acad Sci, Grad Sch, Beijing 100049, Peoples R China
Tianjin Normal Univ, Dept Phys, Tianjin 300074, Peoples R ChinaChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Liu, F. S.
;
Xia, X. Y.
论文数: 0引用数: 0
h-index: 0
机构:
Tianjin Normal Univ, Dept Phys, Tianjin 300074, Peoples R ChinaChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Xia, X. Y.
;
Mao, Shude
论文数: 0引用数: 0
h-index: 0
机构:
Tianjin Normal Univ, Dept Phys, Tianjin 300074, Peoples R China
Univ Manchester, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, EnglandChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Mao, Shude
;
Wul, Hong
论文数: 0引用数: 0
h-index: 0
机构:
Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R ChinaChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Wul, Hong
;
Deng, Z. G.
论文数: 0引用数: 0
h-index: 0
机构:
Chinese Acad Sci, Grad Sch, Beijing 100049, Peoples R ChinaChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China