Variation of Inner Radius of Dust Torus in NGC4151
Long-term optical and near-infrared monitoring observations for a type 1 active galactic nucleus (AGN) NGC4151 were carried out for six years from 2001 to 2006 by using the MAGNUM telescope, and delayed response of flux variations in the K(2.2 μm) band t
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|Source:||Astrophysical Journal, The|
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