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Peculiar features arising from merging galaxy clusters: the case of A1644 and A2034
2021
Zenodo
Galaxy clusters constitute the building blocks of the large scale structure, and some interesting events arise during the collisions among them. For example, we can cite the intracluster medium gas (ICM) sloshing or, in more extreme events, the temporary ICM stripping of the cluster potential well. A combination of weak lensing + spectroscopy + hydrodynamical simulations has been proven powerful to describe the three cluster main components (sorted in ascending mass), galaxies, ICM and dark
doi:10.5281/zenodo.4911126
fatcat:7kizj2gipjdmnczcrn4a5v6eh4