Fig. 3.
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Projected distribution of the gas density (left column) and stars (u − g − r band images using SUNSET, right column) for BH-G9685 and its host galaxy at three different epochs. Vectors correspond to the spin of the stellar (cyan), gas accretion disk (red) and BH (black). ① At high redshift, a proto-galaxy is forming and is displaying a disturbed morphology. ② Once the galactic disk is formed, the three spins are well aligned. ③ This Galaxy has a very quiet evolution and turns to a S0 galaxy due to the quenching of star formation. The three spins remains aligned.
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