中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Coronae above accretion disks around black holes: the effect of Compton cooling

文献类型:期刊论文

作者Meyer-Hofmeister, E.1; Liu, B. F.2; Meyer, F.1
刊名ASTRONOMY & ASTROPHYSICS
出版日期2012-08-01
卷号544
关键词accretion, accretion disks X-rays: galaxies black hole physics galaxies: active magnetic fields galaxies: Seyfert
英文摘要Context. The geometry of the accretion flow around stellar mass and supermassive black holes depends on the accretion rate. Broad iron emission lines originating from the irradiation of cool matter can indicate that there is an inner disk below a hot coronal flow.
收录类别SCI
语种英语
WOS记录号WOS:000308290100087
源URL[http://ir.bao.ac.cn/handle/114a11/6142]  
专题国家天文台_空间科学研究部
作者单位1.Max Planck Inst Astrophys, D-85740 Garching, Germany
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
推荐引用方式
GB/T 7714
Meyer-Hofmeister, E.,Liu, B. F.,Meyer, F.. Coronae above accretion disks around black holes: the effect of Compton cooling[J]. ASTRONOMY & ASTROPHYSICS,2012,544.
APA Meyer-Hofmeister, E.,Liu, B. F.,&Meyer, F..(2012).Coronae above accretion disks around black holes: the effect of Compton cooling.ASTRONOMY & ASTROPHYSICS,544.
MLA Meyer-Hofmeister, E.,et al."Coronae above accretion disks around black holes: the effect of Compton cooling".ASTRONOMY & ASTROPHYSICS 544(2012).

入库方式: OAI收割

来源:国家天文台

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