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astro-ph2007★ 131 cited
Impact of tangled magnetic fields on AGN-blown bubbles
M. Ruszkowski, T. A. Ensslin, M. Bruggen +2
There is growing consensus that feedback from AGN is the main mechanism responsible for stopping cooling flows in clusters of galaxies. AGN are known to inflate buoyant bubbles tha…
astro-ph2005
Simulations of magnetic fields in filaments
M. Bruggen, M. Ruszkowski, A. Simionescu +2
The intergalactic magnetic field within filaments should be less polluted by magnetised outflows from active galaxies than magnetic fields in clusters. Therefore, filaments may be…
astro-ph1998
On Solar Frequency Changes
M. Cunha, M. Bruggen, D. O. Gough
The structure of the surface layers of the Sun is changed by magnetic activity which, in turn, changes the eigenfrequencies of the acoustic modes. These frequency shifts have been…