nIFTy galaxy cluster simulations – II. Radiative models

We have simulated the formation of a massive galaxy cluster ( $M_{200}^{\rm crit}$ = 1.1 × 1015 h −1 M⊙) in a Λ cold dark matter universe using 10 different codes (ramses, 2 incarnations of arepo and 7 of gadget), modelling hydrodynamics with full radiative subgrid physics. These codes include smoot...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2016-07, Vol.459 (3), p.2973-2991
Hauptverfasser:	Sembolini, Federico, Elahi, Pascal Jahan, Pearce, Frazer R., Power, Chris, Knebe, Alexander, Kay, Scott T., Cui, Weiguang, Yepes, Gustavo, Beck, Alexander M., Borgani, Stefano, Cunnama, Daniel, Davé, Romeel, February, Sean, Huang, Shuiyao, Katz, Neal, McCarthy, Ian G., Murante, Giuseppe, Newton, Richard D. A., Perret, Valentin, Puchwein, Ewald, Saro, Alexandro, Schaye, Joop, Teyssier, Romain
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Clusters Computer simulation Dark matter Entropy Feedback Fluid flow Galactic clusters Hydrodynamics Simulation Star & galaxy formation Thermodynamics Universe
Online-Zugang:	Volltext
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