Orbital motion of the radio core in the radio galaxy 3C 66B

被引：0

作者：

Sudou, H ^{[1
]}

Iguchi, S ^{[1
]}

Murata, Y ^{[1
]}

Taniguchi, Y ^{[1
]}

机构：

[1] Gifu Univ, Fac Engn, Gifu 5011193, Japan

来源：

Future Directions in High Resolution Astronomy: The 10th Anniversary of the VLBA | 2005年 / 340卷

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D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Supermassive black hole binaries may exist in the centers of active galactic nuclei like radio galaxies. We imaged the radio galaxy 3C 66B at radio frequencies using the Very Long Baseline Interferometer and found that the unresolved radio core of 3C 66B shows well-defined elliptical motions with a period of 1.05 +/- 0.03 years. This result strongly suggests the orbital motion of a supermassive black hole binary.

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页码：541 / 543

页数：3

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