How to detect supermassive binary black holes at parsec scales
Liu, Xiang
2016-02-01
会议日期2016-02-01
会议地点Beijing, China
关键词Black Hole Physics: Binary Galaxies: Jets Quasars: General Radio Continuum
卷号312
DOI10.1017/S1743921315007553
页码77-78
英文摘要

It is difficult to find or identifying the binary black holes in parsec scales, since the dual AGN may be merged quickly. It is required to explore more possibilities to identifying binary black holes in parsec scales, we give some discussions, especially with the VLBI methods.

产权排序1
会议录IAUS 312: Star Clusters and Black Holes in Galaxies across Cosmic Time
资助机构International Astronomical Union ; State Key Lab of Computational Astrophysics, NAOC, CAS ; State Key Laboratory of Theoretical Physics, ITP, CAS ; Thousand Talents Program - Recruitment of Global Experts ; Chile-China Joint Center for Astronomy ; SUGON Company ; International Astronomical Union ; State Key Lab of Computational Astrophysics, NAOC, CAS ; State Key Laboratory of Theoretical Physics, ITP, CAS ; Thousand Talents Program - Recruitment of Global Experts ; Chile-China Joint Center for Astronomy ; SUGON Company
会议录出版者Cambridge University Press
语种英语
URL标识查看原文
ISSN号1743-9221
ISBN号978-1107078727
内容类型会议论文
源URL[http://ir.xao.ac.cn/handle/45760611-7/1771]  
专题星系宇宙学研究团组
新疆天文台_射电天文研究室
通讯作者Liu, Xiang
作者单位Xinjiang Astronomical Observatory of CAS, 150 Science 1-Street, Urumqi 830011, China
推荐引用方式
GB/T 7714
Liu, Xiang. How to detect supermassive binary black holes at parsec scales[C]. 见:. Beijing, China. 2016-02-01.
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