In a single simulated Milky Way-mass halo, increasing Seyfert jet accretion efficiency pushes star formation to larger radii, reduces stellar mass, and can nearly quench star formation.
Cosmological Evolution of Galaxies
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abstract
I review the subject of the cosmological evolution of galaxies, including different aspects of growth in disk galaxies, by focussing on the angular momentum problem, mergers, and their by-products. I discuss the alternative to merger-driven growth -- cold accretion and related issues. In the follow-up, I review possible feedback mechanisms and their role in galaxy evolution. Special attention is paid to high-redshift galaxies and their properties. In the next step, I discuss a number of processes, gas- and stellar-dynamical, within the central kiloparsec of disk galaxies, and their effect on the larger spatial scales, as well as on the formation and fuelling of the seed black holes in galactic centres at high redshifts.
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Jetted Seyfert Galaxies at z = 0: Simulating Feedback Effects on Galactic Morphology and Beyond
In a single simulated Milky Way-mass halo, increasing Seyfert jet accretion efficiency pushes star formation to larger radii, reduces stellar mass, and can nearly quench star formation.