Fig 2 (IMAGE)

The University of Hong Kong

Fig 2

Caption

Stellar kinematics of MRG-M0138 compared with dynamical models. The prominent central peak in the stellar second velocity moment can only be reproduced when the model includes a black hole of about six billion solar masses; models without a black hole cannot explain the observations. Image adapted from Newman et al., Science 392, 1065–1068 (2026).

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The University of Hong Kong

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