Figure1-1-4-5.png

Left: ALMA image CO 2-1 velocity field at 75mas (7pc) resolution of the barred lenticular galaxy NGC1574, which hosts a supermassive black hole. Center: the velocity field along the major axis, plus the best fit model including a SMBH. Right: separating the mass contributions from the galaxy and the SMBH, indicating a black hole mass of 6.2x107 M⊙ (Zhang et al. arXiv:2507.10662).

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