Turbulence and vorticity in Galaxy clusters generated by structure formation

Turbulence is a key ingredient for the evolution of the intracluster medium, whose properties can be predicted with high-resolution numerical simulations. We present initial results on the generation of solenoidal and compressive turbulence in the intracluster medium during the formation of a small-...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2017-01, Vol.464 (1), p.210-210
Hauptverfasser:	Vazza, F, Jones, T W, Brueggen, M, Brunetti, G, Gheller, C, Porter, D, Ryu, D
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Clusters Computational fluid dynamics Computer simulation Dissipation Formations Simulation Star & galaxy formation Turbulence Turbulent flow Vorticity
Online-Zugang:	Volltext
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