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Radiative magneto-hydrodynamics in massive star formation and accretion disks
Published online by Cambridge University Press: 01 November 2008
Abstract
We briefly overview our newly developed radiation transport module for MHD simulations and two actual applications. The method combines the advantage of the speed of the Flux-Limited Diffusion approximation and the high accuracy obtained in ray-tracing methods.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Symposium S259: Cosmic Magnetic Fields: From Planets, to Stars and Galaxies , November 2008 , pp. 103 - 104
- Copyright
- Copyright © International Astronomical Union 2009
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