Position Measurements of the Core in 3C 66B

摘要：

It was argued that 3C 66B, a nearby radio galaxy, harbors a supermassive black hole binary (SMBHB). To investigate this, a 4-epoch VLBA phase referencing imaging observation was performed in 2004-2005. Here we present some preliminary results of this project. We found a large position difference compared to previous results.

作者: G.-Y.Zhao Y.-J.Chen Z.-Q.Shen H.Sudou S.Iguchi Y.Murata Y.Taniguchi

作者单位: Shanghai Astronomical Observatory,Chinese Academy of Sciences,Shanghai 200030,China Graduate School Shanghai Astronomical Observatory,Chinese Academy of Sciences,Shanghai 200030,China Faculty of Engineering,Gifu University,Gifu 501-1193,Japan National Astronomical Observatory of Japan,Tokyo 181-8588,Japan The Institute of Space and Astronautical Science,JAXA,Kanagawa 229-8510,Japan Research Center for Space and Cosmic Evolution,Ehime University,Matsuyama 790-8577,Japan

会议类型: 国际会议

会议名称: International Conference of Multiwavelength Variability of Blazars(Blazar多波段光变国际学术会议)

会议地点: 广州

会议语种:英文

页码: 61-63

在线出版日期: 2010-09-20（万方平台首次上网日期，不代表论文的发表时间）