Institutional Repository of Radio Astronomy Research Laboratory
| The physical fundamental plane of black hole activity: revisited | |
Liu, Xiang1,2 ; Han, Zhenhua1,3; Zhang, Zhen1
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| 2016 | |
| Source Publication | ASTROPHYSICS AND SPACE SCIENCE
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| Volume | 361Issue:1Pages:9 |
| Contribution Rank | 1 |
| Abstract | The correlation between the jet power and accretion disk luminosity is investigated for active galactic nuclei (AGNs) and black hole X-ray binaries (BHXBs) from the literature. The power-law correlation index is steep (mu similar to 1.0-1.4) for radio loud quasars and the 'outliers' of BHXBs, and it is flatter (mu similar to 0.3-0.6) for radio loud galaxies and the standard BHXBs. The steep-index groups are mostly at higher accretion rates (peaked at Eddington ratio > 0.01) and the flatter-index groups are at relatively low accretion rates (peaked at Eddington ratio < 0.01), implying that the former groups could be dominated by the inner disk accretion of black hole, while the jet in latter groups would be a hybrid production of the accretion and black hole spin. We could still have a fundamental plane of black hole activity for the BHXBs and AGNs with diverse (maybe two kinds of) correlation indices. It is noted that the fundamental plane of black hole activity should be referred to the correlation between the jet power and disk luminosity or equivalently to the correlation between jet power, Eddington ratio and black hole mass, rather than the jet power, disk luminosity and black hole mass. |
| Keyword | Black Hole Physics Galaxies: Jets Quasars: General Accretion Accretion Disks |
| Subtype | Article |
| DOI | 10.1007/s10509-015-2601-3 |
| WOS Headings | Science & Technology ; Physical Sciences |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | RADIO/X-RAY CORRELATION ; HOT ACCRETION FLOWS ; SEYFERT 1 GALAXIES ; GALACTIC NUCLEI ; JETS ; BINARIES ; EMISSION ; DISKS ; POWER ; POPULATION |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000367516500009 |
| Funding Organization | 973 Program(2015CB857100) ; Key Laboratory of Radio Astronomy, Chinese Academy of Sciences ; National Natural Science Foundation of China(11273050) |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/911 |
| Collection | 射电天文研究室_星系宇宙学研究团组 射电天文研究室 110米口径全可动射电望远镜（QTT）_110米大口径全可动射电望远镜关键技术研究（973项目）_课题1：大样本射电天体的观测和前沿问题研究 |
| Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 2.Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Peoples R China 3.Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China |
| First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Recommended Citation GB/T 7714 | Liu, Xiang,Han, Zhenhua,Zhang, Zhen. The physical fundamental plane of black hole activity: revisited[J]. ASTROPHYSICS AND SPACE SCIENCE,2016,361(1):9. |
| APA | Liu, Xiang,Han, Zhenhua,&Zhang, Zhen.(2016).The physical fundamental plane of black hole activity: revisited.ASTROPHYSICS AND SPACE SCIENCE,361(1),9. |
| MLA | Liu, Xiang,et al."The physical fundamental plane of black hole activity: revisited".ASTROPHYSICS AND SPACE SCIENCE 361.1(2016):9. |
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| The physical fundame（828KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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