%0 Generic %1 martizzi2014brightest %A Martizzi, Davide %A Teyssier, Romain %A Moore, Ben %D 2014 %K cluster cooling cosmological flows galaxies simulations %T Brightest Cluster Galaxies in Cosmological Simulations with Adaptive Mesh Refinement: Successes and Failures %U http://arxiv.org/abs/1405.0528 %X A large sample of cosmological hydrodynamical zoom-in simulations with Adaptive Mesh Refinement (AMR) is analysed to study the properties of simulated Brightest Cluster Galaxies (BCGs). Following the formation and evolution of BCGs requires modeling an entire galaxy cluster, because the BCG properties are largely influenced by the state of the gas in the cluster and by interactions and mergers with satellites. BCG evolution is also deeply influenced by the presence of gas heating sources such as Active Galactic Nuclei (AGNs) that prevent catastrophic cooling of large amounts of gas. We show that AGN feedback is one of the most important mechanisms in shaping the properties of BCGs at low redshift by analysing our statistical sample of simulations with and without AGN feedback. When AGN feedback is included BCG masses, sizes, star formation rates and kinematic properties are closer to those of the observed systems. Some small discrepancies are observed only for the most massive BCGs, an effect that might be due to physical processes that are not included in our model.

@misc{martizzi2014brightest, abstract = {A large sample of cosmological hydrodynamical zoom-in simulations with Adaptive Mesh Refinement (AMR) is analysed to study the properties of simulated Brightest Cluster Galaxies (BCGs). Following the formation and evolution of BCGs requires modeling an entire galaxy cluster, because the BCG properties are largely influenced by the state of the gas in the cluster and by interactions and mergers with satellites. BCG evolution is also deeply influenced by the presence of gas heating sources such as Active Galactic Nuclei (AGNs) that prevent catastrophic cooling of large amounts of gas. We show that AGN feedback is one of the most important mechanisms in shaping the properties of BCGs at low redshift by analysing our statistical sample of simulations with and without AGN feedback. When AGN feedback is included BCG masses, sizes, star formation rates and kinematic properties are closer to those of the observed systems. Some small discrepancies are observed only for the most massive BCGs, an effect that might be due to physical processes that are not included in our model.}, added-at = {2014-05-06T09:56:20.000+0200}, author = {Martizzi, Davide and Teyssier, Romain and Moore, Ben}, biburl = {https://www.bibsonomy.org/bibtex/23c2ec7fe5fc693ba4b9d031abadd4306/miki}, description = {[1405.0528] Brightest Cluster Galaxies in Cosmological Simulations with Adaptive Mesh Refinement: Successes and Failures}, interhash = {fa2d29498e20d499379a4740d5f7cd1f}, intrahash = {3c2ec7fe5fc693ba4b9d031abadd4306}, keywords = {cluster cooling cosmological flows galaxies simulations}, note = {cite arxiv:1405.0528Comment: 10 pages, 2 tables, 7 figures. Submitted to MNRAS}, timestamp = {2014-05-06T09:56:20.000+0200}, title = {Brightest Cluster Galaxies in Cosmological Simulations with Adaptive Mesh Refinement: Successes and Failures}, url = {http://arxiv.org/abs/1405.0528}, year = 2014 }