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AGN in Idealized Clusters

strict warning: Only variables should be passed by reference in /.amd_mnt/inverness/export/web/webgroups/astroweb/docs/groups/compastro/modules/book/book.module on line 559.
Submitted by peter on Sat, 01/08/2011 - 20:11

Introduction
For these investigations we study jet and lobe morphology as well as energy deposition in analytically defined clusters. The clusters for the double lobe AGN jets are initialized from NFW dark matter density profiles and set in quasi-hydrostatic equilibrium.

Nat19: Color and Vorticity a
  • Relic (RE) Simulation
  • Synthetic Observations of Radio Jets in Cluster Environments
  • Narrow Angle Tail Simulation
‹ Intermittent Jet - Test Calculation up Relic (RE) Simulation ›

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    • AGN in Idealized Clusters
      • Relic (RE) Simulation
      • Synthetic Observations of Radio Jets in Cluster Environments
      • Narrow Angle Tail Simulation
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University of Minnesota :: Minnesota Institute of Astrophysics
Contact :: Tom Jones :: twj@msi.umn.edu