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By using cosmological hydrodynamic simulations, we have studied how supernovae (SNe) and active galactic nuclei (AGN) feedback affect the mass transport (MT) process in high‐redshift (z ∼ 6) galaxies and what the consequence of these processes is on black hole (BH) growth. Intergalactic gas falls through cooling flows onto the outer galactic edge. There, the pressure gradient torque associated with...
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