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• W2037503531 startingPage "L125" @default.
• W2037503531 abstract "We discuss the merger rate, close galaxy environment, and clustering on scales up to an Mpc of the Swift BAT hard X-ray sample of nearby (z<0.05), moderate-luminosity active galactic nuclei (AGNs). We find a higher incidence of galaxies with signs of disruption compared to a matched control sample (18% versus 1%) and of close pairs within 30 kpc (24% versus 1%). We also find a larger fraction with companions compared to normal galaxies and optical emission line selected AGNs at scales up to 250 kpc. We hypothesize that these merging AGNs may not be identified using optical emission line diagnostics because of optical extinction and dilution by star formation. In support of this hypothesis, in merging systems we find a higher hard X-ray to [O iii] flux ratio, as well as emission line diagnostics characteristic of composite or star-forming galaxies, and a larger IRAS 60 μm to stellar mass ratio." @default.
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• W2037503531 date "2010-05-27" @default.
• W2037503531 modified "2023-09-28" @default.
• W2037503531 title "MERGING AND CLUSTERING OF THE <i>SWIFT</i> BAT AGN SAMPLE" @default.
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• W2037503531 doi "https://doi.org/10.1088/2041-8205/716/2/l125" @default.
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