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3D MHD interactions of jets with cluster media
Author(s) -
O'Neill S. M.,
Jones T. W.,
Tregillis I. L.,
Ryu D.
Publication year - 2006
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.200610581
Subject(s) - physics , magnetohydrodynamics , jet (fluid) , dissipative system , intracluster medium , cluster (spacecraft) , astrophysics , backflow , mach number , mechanics , thermal , magnetohydrodynamic drive , luminosity , computational physics , magnetic field , galaxy cluster , meteorology , thermodynamics , mechanical engineering , quantum mechanics , galaxy , computer science , engineering , inlet , programming language
As an initial step in a program to examine the interactions of AGN jets with magnetized cluster media, we have carried out high resolution, 3D MHD medium‐to‐high luminosity jet simulations in both uniform and stratified, cluster‐like atmospheres extending over distances ∼ 200 kpc. The steady jets asymptotically deposit approximately 1/2 of their power into ambient thermal energy, almost independent of the jet Mach number or the external density gradient. Nearly 1/4 of the jet power goes directly into irreversible, dissipative heating of the ICM. The remaining energy is mostly stored in the jet backflow cocoon. Magnetic energy introduced by the jet is generally amplified, especially by sheared flows. We also examined the dynamical evolution of the jets and their cocoons, comparing them to simple analytic models. (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)