achandrastudyofthemassivedistantgalaxyclustersdssj01501005
文献类型:期刊论文
作者 | Qin Zhenzhen2; Xu Haiguang2; Wang Jingying2; Gu Junhua1![]() |
刊名 | researchinastronomyandastrophysics
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出版日期 | 2013 |
卷号 | 13期号:10页码:1155 |
ISSN号 | 1674-4527 |
英文摘要 | We present a study of a fossil cluster, SDSS J0150–1005 (z ? 0.364), with high spatial resolution based on the imaging spectroscopic analysis of Chandra observations. The Chandra X-ray image shows a relaxed and symmetric morphology, which indicates that SDSS J0150–1005 is a well-developed galaxy cluster with no sign of a recent merger. According to the isothermal model, its global gas temperature is 5.73 ± 0.80 keV, and the virial mass is 6.23 ± 1.34 × 10~(14)M_⊙. Compared with the polytropic temperature model, the mass calculated based on the isothermal model is overestimated by 49%±11. The central gas entropy, S_(0.1r200) = 143.9 ± 18.3 keV cm~2, is significantly lower than the average value of normal galaxy clusters with similar temperatures. Our results indicate that SDSS J0150–1005 formed during an early epoch. |
语种 | 英语 |
源URL | [http://ir.bao.ac.cn/handle/114a11/41871] ![]() |
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.上海交通大学 |
推荐引用方式 GB/T 7714 | Qin Zhenzhen,Xu Haiguang,Wang Jingying,et al. achandrastudyofthemassivedistantgalaxyclustersdssj01501005[J]. researchinastronomyandastrophysics,2013,13(10):1155. |
APA | Qin Zhenzhen,Xu Haiguang,Wang Jingying,&Gu Junhua.(2013).achandrastudyofthemassivedistantgalaxyclustersdssj01501005.researchinastronomyandastrophysics,13(10),1155. |
MLA | Qin Zhenzhen,et al."achandrastudyofthemassivedistantgalaxyclustersdssj01501005".researchinastronomyandastrophysics 13.10(2013):1155. |
入库方式: OAI收割
来源:国家天文台
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