Published in
American Astronomical Society, Astrophysical Journal, 1(692), p. L40-L44, 2009
DOI: 10.1088/0004-637x/692/1/l40
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Three-Dimensional Relativistic Magnetohydrodynamic Simulations of the Kelvin-Helmholtz Instability: Magnetic Field Amplification by a Turbulent Dynamo
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