Next: 3C 272.1 (NGC 4374, M 84); z=0.003536
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A well-studied nearby FR I with a boxy elliptical host galaxy and a circumnuclear dust disk. [Ferrarese et al.1996] used imaging and spectroscopy of this source to determine its black-hole mass. A faint unresolved nuclear point source is visible in the IR. Data first published by [Quillen et al.2000].
David James Elford Floyd