0402+379 |
 | Minimum credit line: Image courtesy of NRAO/AUI
and Greg Taylor, University of New Mexico(for details, see .
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VLBA 2 cm image of the radio galaxy 0402+379, which hosts two active supermassive black holes at its center. The location of each supermassive black hole is indicated on the image by an artist's conception of an accretion disk with narrow twin jets. These results are based upon multi-epoch, multi-frequency monitoring with the VLBA. The projected separation between the two black holes is 7.3 parsecs, making this the most compact binary black hole pair yet found by more than two orders of magnitude. The combined mass of the system is estimated at ~1.5 x 10^8 solar masses, and assuming equal masses the orbital period is 150,000 years. Though gravitational radiation from this system is not yet enough to cause the orbit to decay, the discovery of this system has implications for the number of compact binary black holes that might be detectable sources of gravitational radiation.
Investigator(s): C. Rodriguez, G. B. Taylor, R. T. Zavala, A. B. Peck, L. K. Pollack, and R. W. Romani This image is available in the following downloadable versions:
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Telescope
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VLBA
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Date of Observation
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2005-01-24
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Type of Observation
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Continuum Observations
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Band
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U
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Wavelength
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2.0 cm
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Frequency
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15 GHz
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Center of Image
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RA: 04:05:49.26, Dec: 38:03:32.23
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Field of View
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0.0000 x 0.0000 degrees
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