European VLBI Network Observations of the Proposed Dual AGN SDSS J101022.95+141300.9
arXiv:2110.10182 · doi:10.3847/1538-4357/ac307d
Abstract
During galaxy merger events, the supermassive black holes in the center of the galaxies may form a pair of active galactic nuclei (AGN) with kpc-scale or even pc-scale separation. Recently, optical observations revealed a promising dual AGN candidate at the center of the galaxy SDSS J101022.95141300.9 (hereafter J10101413). The presence of two distinct [O III]-emitting point sources with a projected separation of pc indicates a dual AGN system. To search for AGN-dominated radio emission originating from the Hubble Space Telescope (HST) point sources, we carried out very long baseline interferometry observations. We resolved the radio structure of J10101413 and detected a single feature offset from the HST point sources and also from the Gaia optical position of the object. Our multi-wavelength analysis of J10101413 inferred two possible interpretations of the observed properties challenging its proposed dual AGN classification.
arXiv commentaccepted to ApJ 16 pages, 3 figures
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