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American Astronomical Society, Astrophysical Journal, 1(735), p. 48, 2011
DOI: 10.1088/0004-637x/735/1/48
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TYPE 2 ACTIVE GALACTIC NUCLEI WITH DOUBLE-PEAKED [O III] LINES. II. SINGLE AGNs WITH COMPLEX NARROW-LINE REGION KINEMATICS ARE MORE COMMON THAN BINARY AGNs
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