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Title: An examination of magnetized outflows from active galactic nuclei in galaxy clusters: Magnetized outflows in galaxy clusters

Abstract

We present 3D adaptive mesh refinement magnetohydrodynamic (MHD) simulations of an isolated galaxy cluster that include injection of kinetic, thermal and magnetic energy via a central active galactic nucleus (AGN) in order to study and evaluate the role that AGN may play in producing the observed cluster-wide magnetic fields. Using the MHD solver in flash 3.3, we compare several subresolution approaches to the evolution of AGN, specifically focusing on large-scale jet and bubble models. We examine the effects of magnetized outflows on the accretion history of the black hole and cluster thermodynamic properties, discuss the ability of various models to magnetize the cluster medium, and assess the sensitivity of these models to their underlying subgrid parameters. We find that magnetized jet-based models suffer a severe reduction in accretion rate compared to hydrodynamic jets; however, bubble models remain largely unaffected. While both jets and sporadically placed bubbles have difficulty reproducing the observed strength and topology of cluster magnetic fields, models based on centrally located bubbles come closest to observations. Finally, whereas jet models are relatively insensitive to changes in their subgrid parameters, the accretion rate and average magnetic field produced by the bubbles vary by as much as an order ofmore » magnitude depending on the grid resolution and accretion strength.« less

Authors:
 [1];  [1];  [1];  [1];  [2]
  1. Univ. of Illinois at Urbana-Champaign, IL (United States)
  2. Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
Publication Date:
Research Org.:
Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States). Oak Ridge Leadership Computing Facility (OLCF); UT-Battelle LLC/ORNL, Oak Ridge, TN (United States); Krell Institute, Ames, IA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1564898
Grant/Contract Number:  
AC05-00OR22725; FG02-97ER25308
Resource Type:
Accepted Manuscript
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Volume: 419; Journal Issue: 3; Journal ID: ISSN 0035-8711
Publisher:
Royal Astronomical Society
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics; methods: numerical; MHD; galaxies: clusters: intracluster medium; galaxies: magnetic fields; galaxies: active

Citation Formats

Sutter, P. M., Yang, H. -Y. Karen, Ricker, P. M., Foreman, G., and Pugmire, D. An examination of magnetized outflows from active galactic nuclei in galaxy clusters: Magnetized outflows in galaxy clusters. United States: N. p., 2011. Web. doi:10.1111/j.1365-2966.2011.19875.x.
Sutter, P. M., Yang, H. -Y. Karen, Ricker, P. M., Foreman, G., & Pugmire, D. An examination of magnetized outflows from active galactic nuclei in galaxy clusters: Magnetized outflows in galaxy clusters. United States. https://doi.org/10.1111/j.1365-2966.2011.19875.x
Sutter, P. M., Yang, H. -Y. Karen, Ricker, P. M., Foreman, G., and Pugmire, D. Tue . "An examination of magnetized outflows from active galactic nuclei in galaxy clusters: Magnetized outflows in galaxy clusters". United States. https://doi.org/10.1111/j.1365-2966.2011.19875.x. https://www.osti.gov/servlets/purl/1564898.
@article{osti_1564898,
title = {An examination of magnetized outflows from active galactic nuclei in galaxy clusters: Magnetized outflows in galaxy clusters},
author = {Sutter, P. M. and Yang, H. -Y. Karen and Ricker, P. M. and Foreman, G. and Pugmire, D.},
abstractNote = {We present 3D adaptive mesh refinement magnetohydrodynamic (MHD) simulations of an isolated galaxy cluster that include injection of kinetic, thermal and magnetic energy via a central active galactic nucleus (AGN) in order to study and evaluate the role that AGN may play in producing the observed cluster-wide magnetic fields. Using the MHD solver in flash 3.3, we compare several subresolution approaches to the evolution of AGN, specifically focusing on large-scale jet and bubble models. We examine the effects of magnetized outflows on the accretion history of the black hole and cluster thermodynamic properties, discuss the ability of various models to magnetize the cluster medium, and assess the sensitivity of these models to their underlying subgrid parameters. We find that magnetized jet-based models suffer a severe reduction in accretion rate compared to hydrodynamic jets; however, bubble models remain largely unaffected. While both jets and sporadically placed bubbles have difficulty reproducing the observed strength and topology of cluster magnetic fields, models based on centrally located bubbles come closest to observations. Finally, whereas jet models are relatively insensitive to changes in their subgrid parameters, the accretion rate and average magnetic field produced by the bubbles vary by as much as an order of magnitude depending on the grid resolution and accretion strength.},
doi = {10.1111/j.1365-2966.2011.19875.x},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 419,
place = {United States},
year = {Tue Nov 22 00:00:00 EST 2011},
month = {Tue Nov 22 00:00:00 EST 2011}
}

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