SPH simulations of magnetic fields in galaxy clusters

We perform cosmological, hydrodynamic simulations of magnetic fields in galaxy clusters. The computational code combines the special-purpose hardware Grape for calculating gravitational interaction, and smooth-particle hydrodynamics for the gas component. We employ the usual MHD equations for the ev...

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Bibliographic Details
Main Authors: Dolag, Klaus (Author) , Bartelmann, Matthias (Author) , Lesch, Harald (Author)
Format: Article (Journal) Chapter/Article
Language:English
Published: 15 Jul 1999
In: Arxiv

Online Access:Verlag, kostenfrei, Volltext: http://arxiv.org/abs/astro-ph/9907199
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Author Notes:Klaus Dolag, Matthias Bartelmann and Harald Lesch
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SPH simulations of magnetic fields in galaxy clusters by Dolag, Klaus (Author) , Bartelmann, Matthias (Author) , Lesch, Harald (Author) ,


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