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3D modeling of accretion shocks in young stellar objects : Simulation of laboratory experiments
Published online by Cambridge University Press: 13 February 2013
Abstract
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In order to improve the understanding of the physics of accretion shocks around young stellar objects, we have performed a three dimensional simulation of a radiative shock generated in a laser installation. We depict the 3D structure of such a shock. Radiation hydrodynamics is modeled with the HERACLES code; then, radiative transfer post-processing is performed with the IRIS code.
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- Research Article
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- © The Author(s) 2013
References
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