nIFTy galaxy cluster simulations – IV. Quantifying the influence of baryons on halo properties

nIFTy galaxy cluster simulations – IV. Quantifying the influence of baryons on halo properties

Building on the initial results of the nIFTy simulated galaxy cluster comparison, we compare and contrast the impact of baryonic physics with a single massive galaxy cluster, run with 11 state-of-the-art codes, spanning adaptive mesh, moving mesh, classic and modern smoothed particle hydrodynamics (...

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Bibliographic Details
Main Authors: Cui, Weiguang, Power, Chris, Knebe, Alexander, Kay, Scott T., Sembolini, Federico, Elahi, Pascal J., Yepes, Gustavo, Pearce, Frazer, Cunnama, Daniel, Beck, Alexander M., Vecchia, Claudio Dalla, Davé, Romeel, February, Sean, Huang, Shuiyao, Hobbs, Alex, Katz, Neal, McCarthy, Ian G., Murante, Giuseppe, Perret, Valentin, Puchwein, Ewald, Read, Justin I., Saro, Alexandro, Teyssier, Romain, Thacker, Robert J.
Format: Article
Published: Oxford University Press 2016
Subjects:
methods: numerical
galaxies: clusters: general
galaxies: evolution
galaxies: formation
galaxies: haloes
cosmology: theory
Online Access:https://eprints.nottingham.ac.uk/42482/

Internet

https://eprints.nottingham.ac.uk/42482/

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