JWST stellar dynamical modeling of the compact elliptical NGC 4486B yields MBH = 3.6+0.7-0.7 x 10^8 solar masses, and MBH/M* of roughly 4-13%, confirming an overmassive black hole.
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A JWST View of the Overmassive Black Hole in NGC 4486B
JWST stellar dynamical modeling of the compact elliptical NGC 4486B yields MBH = 3.6+0.7-0.7 x 10^8 solar masses, and MBH/M* of roughly 4-13%, confirming an overmassive black hole.