Structure in galaxy clusters
Gastao B. Lima Neto (1), Tatiana F. Lagana (2), Felipe Andrade-Santos, (3), Rubens E.G. Machado (1) ((1) IAG/USP, Brazil (2), NAT/Unicsul, Brazil,, (3) CfA, USA)
TL;DR
This paper explores how structures in galaxy clusters, observed mainly through X-ray data and hydrodynamical simulations, shed light on their formation and evolution processes.
Contribution
It provides an integrated analysis of observational X-ray data and simulation results to understand galaxy cluster structure formation.
Findings
X-ray observations reveal complex substructures in clusters.
Hydrodynamical simulations reproduce observed features.
Insights into cluster evolution mechanisms.
Abstract
We will discuss here how structures observed in clusters of galaxies can provide us insight on the formation and evolution of these objects. We will focus primarily on X-ray observations and results from hydrodynamical -body simulations. This paper is based on a talk given at the School of Cosmology Jose Plinio Baptista -- `Cosmological perturbations and Structure Formation' in Ubu/ES, Brazil.
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Taxonomy
TopicsHistory and Developments in Astronomy