Cluster magnetic fields from active galactic nuclei

P. M. Sutter, P. M. Ricker, H. Y. Yang

Research output: Chapter in Book/Report/Conference proceedingConference contribution


Active galactic nuclei (AGN) found at the centers of clusters of galaxies are a possible source for weak cluster-wide magnetic fields. To evaluate this scenario, we present 3D adaptive mesh refinement MHD simulations of a cool-core cluster that include injection of kinetic, thermal, and magnetic energy via an AGN-powered jet. Using the MHD solver in FLASH 2, we compare several sub-resolution approaches that link the estimated accretion rate as measured on the simulation mesh to the accretion rate onto the central black hole and the resulting feedback. We examine the effects of magnetized outflows on the accretion history of the black hole and discuss the ability of these models to magnetize the cluster medium.

Original languageEnglish (US)
Title of host publicationMonster's Fiery Breath
Subtitle of host publicationFeedback in Galaxies, Groups, and Clusters - Proceedings of the International Conference
Number of pages4
StatePublished - 2009
EventInternational Conference on Monster's Fiery Breath: Feedback in Galaxies, Groups, and Clusters - Madison, WI, United States
Duration: Jun 1 2009Jun 5 2009

Publication series

NameAIP Conference Proceedings
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616


OtherInternational Conference on Monster's Fiery Breath: Feedback in Galaxies, Groups, and Clusters
Country/TerritoryUnited States
CityMadison, WI


  • Active galatic nuclei
  • Cooling flows
  • Galaxies: clusters
  • MHD
  • Methods: numerical

ASJC Scopus subject areas

  • Physics and Astronomy(all)


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