LLAGN and jet-scaling probed with the EVN
文献类型:会议论文
作者 | Paragi, Zsolt1; Shen, Zhi-Qiang2,3; De Gasperin, Francesco4; Yang, Jun1; Merloni, Andrea5,6; Li ZX(李志玄)7 |
出版日期 | 2012 |
会议日期 | 2012-10-09 |
会议地点 | Bordeaux, France |
卷号 | 178 |
DOI | 10.22323/1.178.0008 |
页码 | 1-6 |
英文摘要 | Accreting black holes (BH) on all mass scales (from stellar to supermassive) appear to follow a nonlinear relation between X-ray luminosity, radio luminosity and BH mass, indicating that similar physical processes drive the central engines in X-ray binaries and active galactic nuclei (AGN). However, in recent years an increasing number of BH systems have been identified that do not fit into this scheme. These outliers may be the key to understand how BH systems are powered by accretion. Here we present results from EVN observations of a sample of low-luminosity AGN (LLAGN) with known mass that have unusually high radio powers when compared with their X-ray luminosity. |
产权排序 | 第7完成单位 |
资助机构 | N/A |
会议录 | Proceedings of Science - 11th European VLBI Network Symposium and Users Meeting, EVN Symposium 2012 |
会议录出版者 | Sissa Medialab Srl |
文献子类 | Conference article (CA) |
学科主题 | 射电天文学 |
语种 | 英语 |
URL标识 | 查看原文 |
资助项目 | N/A |
ISSN号 | E-ISSN: 18248039 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/17395] |
专题 | 云南天文台_射电天文研究组 |
通讯作者 | Paragi, Zsolt |
作者单位 | 1.Joint Institute for VLBI in Europe (JIVE), Postbus 2, 7990 AA Dwingeloo, The Netherlands 2.Shanghai Astronomical Observatory, CAS, 80 Nandan Road, Shanghai 200030, P.R. China 3.Key Laboratory of Radio Astronomy, CAS, P.R. China 4.University of Hamburg, Gojenbergsweg 112, D-21029, Hamburg, Germany 5.Max-Planck-Institut für Extraterrestrische Physik, Gießenbachstr. 85741 Garching, Germany 6.Exzellenzcluster Universe, Boltzmann Str. 2, 85748 Garching, Germany 7.Yunnan Astronomical Observatory, NAOC, 650011 Kunming, P.R. China |
推荐引用方式 GB/T 7714 | Paragi, Zsolt,Shen, Zhi-Qiang,De Gasperin, Francesco,et al. LLAGN and jet-scaling probed with the EVN[C]. 见:. Bordeaux, France. 2012-10-09. |
入库方式: OAI收割
来源:云南天文台
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