A candidate sub-parsec binary black hole in the Seyfert galaxy NGC 7674
arXiv:1709.06258 · doi:10.1038/s41550-017-0256-4
Abstract
The existence of binary supermassive black holes (SBHs) is predicted by models of hierarchical galaxy formation. To date, only a single binary SBH has been imaged, at a projected separation of 7.3 parsecs. Here we report the detection of a candidate dual SBH with projected separation of 0.35 pc in the gas-rich interacting spiral galaxy NGC 7674 (Mrk 533). This peculiar Seyfert galaxy possesses a 0.7 kpc Z-shaped radio jet; the leading model for the formation of such sources postulates the presence of an uncoalesced binary SBH created during the infall of a satellite galaxy. Using very long baseline interferometry (VLBI), we imaged the central region of Mrk 533 at radio frequencies of 2, 5, 8 and 15 GHz. Two, possibly inverted-spectrum radio cores were detected at 15 GHz only; the 8-15 GHz spectral indices of the two cores are and (), consistent with accreting SBHs. We derive a jet speed from multi-epoch parsec-scale data of the hotspot region, and a source age yrs.
arXiv comment7 pages, 6 figures, published in Nature Astronomy
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