Fig 3 (IMAGE)

The University of Hong Kong

Fig 3

Caption

In the relation between black hole mass and stellar velocity dispersion, MRG-M0138 appears similar to nearby galaxies. However, when compared with bulge mass, its black hole appears unusually overmassive, about 12 times more massive than expected from the local black hole-bulge mass relation. Image adapted from Newman et al., Science 392, 1065–1068 (2026).

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The University of Hong Kong

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