Infall and accretion of substructure in hydrodynamical simulations of galaxy clusters

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Infall and accretion of substructure in hydrodynamical simulations of galaxy clusters

The evolution of galaxies is heavily influenced by the environment in which they are found. Dense regions of the Universe can quench a galaxy's star formation by removing its gas, and transform a galaxy's morphology from being disk-dominated to bulge-dominated. Galaxy clusters represent th...

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Bibliographic Details
Main Author:	Haggar, Roan
Format:	Thesis (University of Nottingham only)
Language:	English
Published:	2022
Subjects:	Galaxies Galaxy clusters
Online Access:	https://eprints.nottingham.ac.uk/69844/

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