The growth of baryonic structure in the presence of an isotropic magnetic field

Details The growth of baryonic structure in the presence of an isotropic magnetic field The growth of baryonic structure in the presence of an isotropic magnetic field

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006an....327..431g&link_type=abstract

Astronomische Nachrichten, Vol.327, Issue 5/6, p.431

Astronomy and Astrophysics

Astronomy

Galaxies: Clusters: General, Magnetic Fields, Magnetohydrodynamics (Mhd), Methods: Numerical

Scientific paper

We follow the passive evolution of magnetic fields in SPH simulations to
study their role in structure formation and galaxy clusters properties.
Despite magnetic fields are not dynamically important for massive
objects, they can still affect the properties of group-size objects and
core regions and also affect particle's entropy.

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