6533b872fe1ef96bd12d3723

RESEARCH PRODUCT

Exploring Mergers of Galaxy Clusters in a Cosmological Context

Susana PlanellesVicent Quilis

subject

PhysicsN-body simulationStar formationProtogalaxyElliptical galaxyAstronomyContext (language use)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalaxy mergerInteracting galaxyAstrophysics::Galaxy AstrophysicsGalaxy cluster

description

We present results of an Eulerian Adaptive Mesh Refinement (AMR) hydrodynamical and N-body simulation in a ΛCDM cosmology. The simulation incorporates common cooling and heating processes, a phenomenological description of the star formation and supernovae feedback. A specific halo finder has been designed and applied in order to extract a sample of galaxy clusters directly obtained from the simulation without considering any resimulating scheme. We have studied the evolutionary history of the cluster halos, and classified them in three categories depending on the merger events they have undergone. We pay special attention to discuss the role of merger events as a source of feedback and reheating.

https://doi.org/10.1007/978-3-642-11250-8_70