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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