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Open AccessJournal ArticleDOI

Orbital motion in the radio galaxy 3C 66B: evidence for a supermassive black hole binary.

Hiroshi Sudou, +3 more
- 23 May 2003 - 
- Vol. 300, Iss: 5623, pp 1263-1265
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TLDR
Using the very-long-baseline interferometer, it is found that the unresolved radio core of 3C 66B shows well-defined elliptical motions with a period of 1.05 ± 0.03 years, which provides a direct detection of a supermassive black hole binary.
Abstract
Supermassive black hole binaries may exist in the centers of active galactic nuclei such as quasars and radio galaxies, and mergers between galaxies may result in the formation of supermassive binaries during the course of galactic evolution. Using the very-long-baseline interferometer, we imaged the radio galaxy 3C 66B at radio frequencies and found that the unresolved radio core of 3C 66B shows well-defined elliptical motions with a period of 1.05 ± 0.03 years, which provides a direct detection of a supermassive black hole binary.

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Citations
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Journal ArticleDOI

A super massive black hole binary in 3C 66B: Future observational perspectives

TL;DR: In this paper, the existence of a supermassive black hole binary in the radio galaxy 3C 66B has been investigated using VLBI observations, which suggests the presence of a couple of massive black holes in the center of the galaxy.
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Pulsar timing array observations of gravitational wave source timing parallax

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Proper motion of the sub-parsec-scale jet in the radio galaxy 3c 66b

TL;DR: In this paper, the proper motion of the sub-parsec-scale jet in a nearby elliptical galaxy 3C 66B was studied at 2.3 GHz and 8.4 GHz at 10 epochs over four years, using the Very Long Baseline Array for all epochs and the Effelsberg 100 m telescope for the last epoch.
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Determination of Central Engine Position and Accretion Disk Structure in NGC 4261 by Core Shift Measurements

TL;DR: In this paper, the authors measured radio core positions showing observing frequency dependences (known as "core shift") in both approaching jets and counter jets and obtained spectral index maps, which indicate that emission from the counter jet is affected by free-free absorption (FFA).
References
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Journal ArticleDOI

Inward Bound—The Search for Supermassive Black Holes in Galactic Nuclei

TL;DR: In this paper, the authors review dynamical search techniques, the robustness of the evidence, and BH demographics, and find that supermassive black holes are present in 20% of nearby E-Sbc galaxies.
Journal ArticleDOI

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TL;DR: In this article, ground-based observations of a complete sample of 10 of these infrared galaxies suggest that they represent the initial dust-enshrouded stages of quasars, and a second group of ultraluminous objects selected on the basis of warm infrared colors are found to be preferentially Seyfert galaxies.
Book

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TL;DR: In this paper, a theory of interferometry and synthesis imaging analysis of the Interferometer Response Geometric Relationships and Polarimetry Antennas and Arrays Response of the receiving system Design of the Analog Receiving System Digital Signal Processing Very-Long-Baseline Interferometry Calibration and Fourier Transformation of Visibility Data Deconvolution, Adaptive Calibrration, and Applications Interferometers Techniques for Astrometry and Geodesy Propagation Effects Van Cittert-Zernike Theorem, Spatial Coherence, and
Journal ArticleDOI

Massive black hole binaries in active galactic nuclei

TL;DR: In this article, the authors explore the possibility that some active galactic nuclei may contain two massive black holes in orbit about each other, which suggests a new interpretation for the observed bending and apparent precession of radio jets emerging from these objects.
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